Research Article Classical Analog of Extended Phase Space SUSY...
Transcript of Research Article Classical Analog of Extended Phase Space SUSY...
Hindawi Publishing CorporationISRNMathematical PhysicsVolume 2013 Article ID 639424 10 pageshttpdxdoiorg1011552013639424
Research ArticleClassical Analog of Extended Phase Space SUSY and Its Breaking
Gagik Ter-Kazarian
Byurakan Astrophysical Observatory Aragatsotn District 378433 Byurakan Armenia
Correspondence should be addressed to Gagik Ter-Kazarian gago 50yahoocom
Received 21 April 2013 Accepted 12 May 2013
Academic Editors Z Qiao and P Roy
Copyright copy 2013 Gagik Ter-KazarianThis is an open access article distributed under the Creative Commons Attribution Licensewhich permits unrestricted use distribution and reproduction in any medium provided the original work is properly cited
We derive the classical analog of the extended phase space quantum mechanics of the particle with odd degrees of freedom whichgives rise to (119873 = 2)-realization of supersymmetry (SUSY) algebra By means of an iterative procedure we find the approximateground state solutions to the extended Schrodinger-like equation and use these solutions further to calculate the parameters whichmeasure the breaking of extended SUSY such as the ground state energy Consequently we calculate a more practical measure forthe SUSY breaking which is the expectation value of an auxiliary field We analyze nonperturbative mechanism for extended phasespace SUSY breaking in the instanton picture and show that this has resulted from tunneling between the classical vacua of thetheory Particular attention is given to the algebraic properties of shape invariance and spectrum generating algebra
1 Introduction
An interesting question of keeping the symmetry betweencanonical coordinates and momenta in the process ofquantization deserves an investigation From its historicaldevelopment this aspect of statistical quantum mechanicsunfortunately has attracted little attention However muchuse has been made of the technique of ordering of canonicalcoordinates (119902) and momenta (119901) in quantum mechanics[1 2] It was observed that the concept of an extendedLagrangian L(119901 119902 119902) in phase space allows a subsequentextension of Hamiltonrsquos principle to actions minimum alongthe actual trajectories in (119901 119902)- rather than in 119902-space Thisleads to the phase space formulation of quantum mechanicsConsequently this formalism was developed further in [3]by addressing the extended phase space stochastic quanti-zation of Hamiltonian systems with first class holonomicconstraints This in a natural way results in the Faddeev-Popov conventional path-integral measure for gauge systemsContinuing along this line in the present paper we addressthe classical analog of the extended phase space (119873 = 2)-SUSY quantum mechanics [4] of the particles which haveboth bosonic and fermionic degrees of freedom that isthe quantum field theory in (0 + 1)-dimensions in (119902 119901)-space exhibiting supersymmetry (for conventional SUSY
quantummechanics see [5ndash12])We analyze in detail the non-perturbative mechanism for supersymmetry breaking in theinstanton picture ([13]) This paper has been organized asfollows In the first part (Sections 2 and 3) we derive theclassical analog of the extended phase space SUSY quantummechanics and obtain the integrals of motion Consequentlywe describe the extended phase space (119873 = 2)-SUSY algebraIn the second part (Sections 4 and 5) by means of an iterativescheme first we find the approximate ground state solutionsto the extended Schrodinger-like equation and then calculatethe parameters which measure the breaking of extendedSUSY such as the ground state energy We calculate a morepractical measure for the SUSY breaking in particular infield theories which is the expectation value of an auxiliaryfield We analyze nonsperturbative mechanism for extendedphase space SUSY breaking in the instanton picture and showthat this has resulted from tunneling between the classicalvacua of the theory Section 6 deals with the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the perspective of extended phase space SUSYquantum mechanics and further shows how it can be usefulfor spectrum generating algebra The concluding remarksare given in Section 7 Unless otherwise stated we take thegeometrized units (ℎ = 119888 = 1) Also an implicit summationon repeated indices is assumed throughout this paper
2 ISRNMathematical Physics
2 The Integrals of Motion
For the benefit of those not familiar with the framework ofextended phase space quantization enough details are givenin the following tomake the rest of the paper understandableThe interested reader is invited to consult the original papers[1 2] for further details In the framework of the proposedformalism the extended Lagrangian can be written as
Lext (119901 119902 119902) = minus 119902119894119901119894minus 119902
119894119894+L
119902+L
119901 (1)
where a dynamical system with 119873 degrees of freedomdescribed by the 2119873 independent coordinates 119902= (119902
1 119902
119873)
and momenta 119901 = (1199011 119901
119873) which are not in gen-
eral canonical pairs A Lagrangian L119902(119902 119902) is given in
119902-representation and the corresponding L119901(119901 ) in 119901-
representation Adotwill indicate differentiationwith respectto 119905 The independent nature of 119901 and 119902 gives the freedom ofintroducing a second set of canonical momenta for both 119901and 119902 through the extended Lagrangian
120587119902119894=120597Lext120597 119902
119894
=120597L119902
120597 119902119894
minus 119901119894
120587119901119894=120597Lext120597
119894
=120597L119901
120597119894
minus 119902119894
(2)
One may now define an extended Hamiltonian
119867ext (119901 119902 120587119901 120587119902) = 120587119902119894 119902119894 + 120587119901119894 119894 minusLext (119901 119902 119902)
= 119867 (119901 + 120587119902 119902) minus 119867 (119901 119902 + 120587
119901)
(3)
where 119867(119901 119902) = 119901119894119902119894minusL119902
= 119902119894119894minusL119901 is the conventional
Hamiltonian of the system In particular vanishing of 120587119902or
120587119901is the condition for 119901 and 119902 to constitute a canonical
pair In the language of statistical quantum mechanics thischoice picks up a pure state (actual path) Otherwise one isdealing with a mixed state (virtual path) One may howeverenvisage that the full machinery of the conventional quantummechanical dynamics is extendible to the extended dynamicsas alluded to the above Here 119901 and 119902 will be considered asindependent 119888-number operators on the integrable complexfunction 120594(119902 119901) One of the key assumptions of extendedphase space quantization [1 2] is the differential operatorsand commutation brackets for 120587
119901and 120587
119902borrowed from the
conventional quantum mechanics as follows
120587119902119894= minus119894
120597
120597119902119894
[120587119902119894 119902119895] = minus119894120575
119894119895
120587119901119894= minus119894
120597
120597119901119894
[120587119901119894 119901
119895] = minus119894120575
119894119895
(4)
Note also the following
[119901119894 119902119895] = [119901
119894 119901
119895] = [119902
119894 119902119895] = [120587
119901119894 120587
119902119895]
= [120587119901119894 120587
119901119895] = [120587
119902119894 120587
119902119895] = 0
(5)
By the virtue of (4) and (5) 119867ext is now an operator on 120594Along the trajectories in (119901 119902)-space however it producesthe state functions 120594(119901 119902 119905) via the following Schrodinger-like equation
119894120597
120597119905120594 = 119867ext 120594 (6)
Solutions of (6) are
120594 (119902 119901 119905) = 120594119903(119902 119901 119905) 119890
minus119894119901119902
= 119886120572120573120595120572(119902 119905) 120601
lowast
120573(119901 119905) 119890
minus119894119901119902
(7)
where 119886 = 119886dagger positive definite tr 119886 = 1 and 120595
120572and
120601lowast
120572are solutions of the conventional Schrodinger equation
in 119902- and 119901-representations respectively They are mutuallyFourier transforms Note that the 120572 and 120573 are not in generaleigenindices The normalizable 120594 (int120594119889119901119889119902 = tr(119886) = 1)is a physically acceptable solution The exponential factor isa consequence of the total time derivative minus119889(119902119901)119889119905 in (1)which can be eliminated Actually it is easily verified that
(119901 + 120587119902) 120594
119903(119902 119901 119905) = (120587
119902120594119903(119902 119901 119905)) 119890
minus119894119901119902 (8)
and so on Substitution of (8) in (6) gives
119894120597
120597119905120594 (119902 119901 119905) = 119867ext 120594119903 (119902 119901 119905) (9)
provided by the reducedHamiltonian119867ext From now onwereplace119867ext by119867ext and 120594119903(119902 119901 119905) by 120594119903(119902 119901 119905) respectivelyand retain former notational conventions
It is certainly desirable to derive the classical analog of theextended phase space quantummechanics of the particlewithodd degrees of freedom directly from what may be taken asthe first principleTherefore following [10ndash12] let us considera nonrelativistic particle of unit mass with two (120572 = 1 2)odd (Grassmann) degrees of freedomThe classical extendedLagrangian equation (1) can be written
Lext (119901 119902 119902) = minus 119902119901 minus 119902 +1
21199022minus 119865 (119902) +
1
22
minus 119866 (119901) minus 119877 (119902 119901)119873 +1
2120595120572120572
(10)
provided by 119873 = 12059511205952= minus119894120595
+120595minus Here 119865(119902) R rarr
R 119866(119901) R rarr R and 119877(119902 119901) R rarr R are arbitrarypiecewise continuously differentiable functions given overthe 1-dimensional Euclidean space R The 120595
120572are two odd
(Grassmann) degrees of freedom The nontrivial Poisson-Dirac brackets of the system (10) are
119902 120587119902 = 1 119901 120587
119901 = 1 120595
120572 120595
120573 = 120575
120572120573
120595+ 120595
minus = 1 120595
2
plusmn= 0 120595
plusmn=1
radic2(120595
1plusmn 119894120595
2)
(11)
The extended Hamiltonian119867ext (3) reads
119867ext (119901 119902 120587119901 120587119902) =1
2(119901 + 120587
119902)2
+ 1198652(119902) minus
1
2(119902 + 120587
119901)2
minus 1198662(119901) + 119877 (119902 119901)119873
(12)
ISRNMathematical Physics 3
which according to (8) reduces to
119867ext (119901 119902 120587119901 120587119902) =1
21205872
119902+ 119865
2(119902) minus
1
21205872
119901
minus 1198662(119901) + 119877 (119902 119901)119873
(13)
TheHamiltonian equation (13) yields the following equationsof motion
119902 = 120587119902 = 120587
119901
119902= minus119865
1015840
119902(119902) minus 119877
1015840
119902(119902 119901)119873
119901= minus119866
1015840
119901(119901) + 119877
1015840
119901(119902 119901)119873
plusmn= plusmn119894119877 (119902 119901) 120595
plusmn
(14)
Aprimewill indicate differentiationwith respect either to 119902 or119901 Thus119873 is the integral of motion additional to119867ext Alongthe trajectories 119902(119905) and 119901(119905) in (119901 119902)-spaces the solution toequations of motion for odd variables is
120595plusmn (119905) = 120595plusmn (1199050) exp [plusmn119894 int
119905
1199050
119877 (119902 (120591) 119901 (120591)) 119889120591] (15)
Hence the odd quantities
120579plusmn= 120579
plusmn (119905) exp [∓119894 int119905
1199050
119877 (119902 (120591) 119901 (120591)) 119889120591] (16)
are nonlocal in time integrals of motion In trivial case 119877 =
0 we have plusmn= 0 and 120579
plusmn= 120579
plusmn Suppose that the system
has even complex conjugate quantities119861119902119901plusmn
(119861119902119901+
)lowast= 119861
119902119901minus
whose evolution looks up to the term proportional to119873 likethe evolution of odd variables in (14)Then local odd integralsof motion could be constructed in the form
119876119902119901plusmn
= 119861119902119901∓
120595plusmn (17)
Let us introduce the oscillator-like bosonic variables 119861119902119901plusmn
in119902- and 119901-representations as follows
119861119902∓L
2(R) 997888rarrL
2(R) 119861
119902∓= [119901 + 120587
119902plusmn 119894119882 (119902)]
119861119901∓L
2(R) 997888rarrL
2(R) 119861
119901∓= [119902 + 120587
119901plusmn 119894119881 (119901)]
(18)
In the expressions (18)119882(119902) R rarr R and119881(119901) R rarr Rare the piecewise continuously differentiable functions calledSUSY potentials In particular case if119877(119902 119901) = 119877
119902(119902)minus119877
119901(119901)
for the evolution of 119861119902119901plusmn
we obtain
119902∓= [minus (119865
1015840
119902+ 119877
1015840
119902119873) plusmn 119894119882
1015840
119902(119902) (119901 + 120587
119902)]
119901∓= [minus (119866
1015840
119901+ 119877
1015840
119901119873) plusmn 119894119881
1015840
119901(119901) (119902 + 120587
119901)]
(19)
Consequently
119902plusmn= plusmn119894 [(119882
1015840
119902minus 119877
1015840
119902plusmn) plusmn 119894 (119865
1015840
119902minus119882119882
1015840
119902) 120595
∓]
119901plusmn= plusmn119894 [(119881
1015840
119901minus 119877
1015840
119901plusmn) plusmn 119894 (119866
1015840
119901minus 119881119881
1015840
119901) 120595
∓]
(20)
This shows that either 119902plusmn= 0 or
119901plusmn= 0 when 1198821015840
119902(119902) =
1198771015840
119902plusmn(119902) and 119865
1015840
119902= (12)(119882
2)1015840
119902or 1198811015840
119901(119901) = 119877
1015840
119901plusmn(119901) and
1198661015840
119901= (12)(119881
2)1015840
119901 respectively Therefore when the functions
119877119902119901
and 119865(119902) 119866(119901) are related as
1198771015840
119902plusmn(119902) = 119882
1015840
119902(119902) 119865
119902=1
2(119882
2) + 119862
119902
1198771015840
119901plusmn(119901) = 119881
1015840
119901(119901) 119865
119901=1
2(119881
2) + 119862
119901
(21)
where 119862119902119901
are constants then odd quantities 119876119902119901plusmn
areintegrals of motion in addition to 119867ext and 119873 According to(3) and (13) let us present119867ext in the form119867ext = 119867119902
minus 119867119901
where
119867119902=1
21205872
119902+ 119865
2(119902) + 119877
119902119873
119867119901=1
21205872
119901+ 119866
2(119901) + 119877
119901119873
(22)
Then 119876119902119901plusmn
and 119873 together with the 119867119902and 119867
119901form the
classical analog of the extended phase space SUSY algebra asfollows
119876119902119901+
119876119902119901minus
= minus119894 (119867119902119901minus 119862
119902119901)
119867119902119901 119876
119902119901plusmn = 119876
119902119901plusmn 119876
119902119901plusmn = 0
119873119876119902119901plusmn
= plusmn119894119876119902119901plusmn
119873119867119902119901 = 0
(23)
with constants119862119902119901
playing a role of a central charges in (119902 119901)-spaces 119873 is classical analog of the grading operator Putting119862119902= 119862
119901= 0 we arrive at the classical analog of the extended
phase space SUSY quantummechanics given by the extendedLagrangian
Lext (119901 119902 119902) =1
21205872
119902minus1
2119882
2(119902) +
1
21205872
119901minus1
21198812(119901)
+ 12059511205952(119882
1015840
119902+ 119881
1015840
119901) +
1
2120595120572120572
(24)
We conclude that the classical system (10) is characterizedby the presence of two additional local in time odd integralsof motion equation (17) being supersymmetry generatorsAlong the actual trajectories in 119902-space (24) reproduces theresults obtained in [6]
3 The Path Integral Formulation
In the matrix formulation of extended phase space (119873 = 2)-SUSY quantum mechanics the
plusmnwill be two real fermionic
creation and annihilation nilpotent operators describingthe fermionic variables The
plusmn having anticommuting 119888-
number eigenvalues imply
plusmn= radic
1
2(
1plusmn 119894
2)
120572
120573 = 120575
120572120573
+
minus = 1
2
plusmn= 0
(25)
They can be represented by finite dimensional matrices plusmn=
120590plusmn where 120590plusmn = (120590
1plusmn120590
2)2 are the usual raising and lowering
4 ISRNMathematical Physics
operators for the eigenvalues of 1205903which is the diagonal Pauli
matrix The fermionic operator 119891 reads 119891 C2rarr C2
119891 =
(12)[+
minus] which commutes with the119867ext and is diagonal
in this representation with conserved eigenvalues plusmn12 Dueto it the wave functions become two-component objects asfollows
120594 (119902 119901) = (120594+12
(119902 119901)
120594minus12
(119902 119901)) = (
1205941(119902 119901)
1205942(119902 119901)
) = (
1205951(119902) 120601
1(119901)
1205952(119902) 120601
2(119901))
(26)
where the states 12059512(119902) 120601
12(119901) correspond to fermionic
quantum number 119891 = plusmn12 respectively in 119902- and 119901-spacesThey belong to Hilbert space H = H
0otimes C2
= [L2(R) otimes
L2(R)]otimesC2 Hence theHamiltonian119867ext of extended phase
space (119873 = 2)-SUSY quantummechanical system becomes a2 times 2matrix as follows
119867ext = (119867+
0
0 119867minus
) =1
2(
2
119902+119882
2(119902) + 119894119882
1015840
119902(119902) [
1
2])
minus1
2(
2
119901+ 119881
2(119901) + 119894119881
1015840
119902(119901) [
1
2])
(27)
To infer the extendedHamiltonian equation (27) equivalentlyone may start from the 119888-number extended Lagrangian ofextended phase space quantum field theory in (0 + 1)-dimensions in 119902- and 119901-spaces as follows
Lext (119901 119902 119902) = minus 119902119901 minus 119902 +1
2[(119889119902
119889119905)
2
minus1198822(119902)]
+ 1198911198821015840
119902(119902) +
1
2[(119889119901
119889119905)
2
minus 1198812(119901)]
+ 1198911198811015840
119901(119901)
(28)
In dealing with abstract space of eigenstates of the conjugateoperator
plusmnwhich have anticommuting 119888-number eigenval-
ues suppose that |00minus⟩ is the normalized zero-eigenstate of 119902and
minusas follows
119902 |00minus⟩ = 0 minus |00minus⟩ = 0 (29)
The state |00+⟩ is defined by
|00+⟩ = + |00minus⟩ = 0 (30)
then +|00+⟩ = 0
minus|00+⟩ = |00minus⟩ Taking into account
that daggerplusmn=
∓ we get
⟨∓00| plusmn = 0 ⟨∓00| ∓ = ⟨plusmn00| (31)
Now we may introduce the notation 120572 120573 for the anticom-muting eigenvalues of
plusmn Consistency requires
120572plusmn= minus
plusmn120572 120572 |00plusmn⟩ = plusmn |00plusmn⟩ 120572 (32)
The eigenstates of 119902 minuscan be constructed as
1003816100381610038161003816119902120572minus⟩ = 119890minus119894119902119901minus120572+
|00minus⟩ (33)
and thus
1199021003816100381610038161003816119902120572minus⟩ = 119902
1003816100381610038161003816119902120572minus⟩ minus
1003816100381610038161003816119902120572minus⟩ = 1205721003816100381610038161003816119902120572minus⟩ (34)
Then the 119902and
+eigenstates are obtained by Fourier
transformation as follows
1003816100381610038161003816 119902120573+⟩ = minusint119889120572119890120572120573 1003816100381610038161003816 119902120572minus⟩
10038161003816100381610038161003816120587119902120572plusmn⟩ = minusint119889119902119890
119894119902120587119902 1003816100381610038161003816 119902120572plusmn⟩
1003816100381610038161003816119901120573+⟩ = minusint119889120572119890120572120573 1003816100381610038161003816119901120572minus⟩
10038161003816100381610038161003816120587119901120572plusmn⟩ = minusint119889119901119890
119894119901120587119901 1003816100381610038161003816119901120572plusmn⟩
(35)
which gives
119902
10038161003816100381610038161003816120587119902120572plusmn⟩ = 120587
119902
10038161003816100381610038161003816120587119902120572plusmn⟩
+
10038161003816100381610038161003816(119902 120587
119902) 120573+⟩ = 120573
10038161003816100381610038161003816(119902 120587
119902) 120573+⟩
119901
10038161003816100381610038161003816120587119901120572plusmn⟩ = 120587
119901
10038161003816100381610038161003816120587119901120572plusmn⟩
+
10038161003816100381610038161003816(119901 120587
119901) 120573+⟩ = 120573
10038161003816100381610038161003816(119901 120587
119901) 120573+⟩
(36)
The following completeness relations hold
minus int1198891205721198891199021003816100381610038161003816 119902120572plusmn⟩⟨∓120572
lowast1199021003816100381610038161003816 = 1
minus int119889120572
119889120587119902
2120587
10038161003816100381610038161003816120587119902120572plusmn⟩⟨∓120572
lowast120587119902
10038161003816100381610038161003816= 1
minus int1198891205721198891199011003816100381610038161003816119901120572plusmn⟩⟨∓120572
lowast1199011003816100381610038161003816 = 1
minus int119889120572
119889120587119901
2120587
10038161003816100381610038161003816120587119901120572plusmn⟩⟨∓120572
lowast120587119901
10038161003816100381610038161003816= 1
(37)
The time evolution of the state |119905⟩ is now given as follows
120594minus(119902120572119901120573119905) = minusint119889120572
1015840119889119902
1015840119889120573
1015840119889119901
1015840119870(119902120572119901120573119905 | 119902
10158401205721015840119901101584012057310158401199051015840)
(38)
The kernel reads
119870(119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840)
= ⟨+119902120572lowast119901120573
lowast1003816100381610038161003816 119890minus119894119867ext(119905minus119905
1015840) 100381610038161003816100381610038161199021015840120572101584011990110158401205731015840⟩
(39)
which can be evaluated by the path integral Actually analternative approach to describe the state space and dynamicsof the extended phase space quantum system is by the pathintegral [3] which reads
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) = ⟨119902119901119891
1003816100381610038161003816 119890minus119894119867ext(119905minus119905
1015840) 10038161003816100381610038161003816119902101584011990110158401198911015840⟩ (40)
In the path integral equation (40) the individual states arecharacterized by the energy and the fermionic quantum
ISRNMathematical Physics 5
number 119891 With the Hamiltonian 119867ext the path integralequation (40) is diagonal as follows
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840)
=K1198911198911015840 (119902119905 | 119902
10158401199051015840)K
1198911198911015840 (119901119905 | 119901
10158401199051015840)
= 1205751198911198911015840 int
119902
1199021015840
D119902int119901
1199011015840
D119901 exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(41)
Knowing the path integral equation (41) it is sufficient tospecify the initial wave function 120594
119891(1199021015840 119901
1015840 1199051015840) to obtain all
possible information about the system at any later time 119905 by
120594119891(119902 119901 119905) = sum
1198911015840
int1198891199021015840119889119901
1015840K
1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) 120594
1198911015840 (119902
1015840 119901
1015840 1199051015840)
(42)
with 120594plusmn12
(119902 119901 119905) = 12059412(119902 119901 119905) (26) In terms of anti-
commuting 119888-number operators 120577 and 120578 defining 120595 =
radic12 (120578+120577
119894(120578minus120577)) the path integral equation (41) becomes
K (119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840) = int
119902120572119901120573
1199021015840120572101584011990110158401205731015840
D119902D119901D120577D120578
times exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(43)
The functional integral is taken over all trajectories from 1199021015840 1205721015840to 119902 120572 and 1199011015840 1205731015840 to 119901 120573 between the times 1199051015840 and 119905
4 Solution of the Extended SchroumldingerEquation with Small Energy Eigenvalue 120576
Adopting the technique developed in [13] first we usethe iterative scheme to find the approximate ground statesolutions to the extended Schrodinger-like equation
119867ext120594 (119902 119901) = (119867119902minus 119867
119901) 120594 (119902 119901) = 120576120594 (119902 119901) (44)
with energy 120576Wewill then use these solutions to calculate theparameters which measure the breaking of extended SUSYsuch as the ground state energy The approximation whichwent into the derivation of solutions of (44) meets ourinterest that the ground state energy 120576 is supposedly smallAs we mentioned above the solutions for nonzero 120576 come inpairs of the form
120594uarr(119902 119901) = (
1205941(119902 119901)
0) or 120594
darr(119902 119901) = (
0
1205942(119902 119901)
)
(45)
related by supersymmetry where 12059412(119902 119901) = 120595
12(119902)120601
12(119901)
The state space of the system is defined by all the normalizablesolutions of (44) and the individual states are characterizedby the energies 120576
119902and the fermionic quantumnumber119891 One
of these solutions is acceptable only if119882(119902) and119881(119901) becomeinfinite at both 119902 rarr plusmninfin and 119901 rarr plusmninfin respectivelywith the same sign If this condition is not satisfied neitherof the solutions is normalizable nor they can represent theground state of the system Equation (44) yields the followingrelations between energy eigenstates with fermionic quantumnumber plusmn12
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205952 (119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206012 (119901)
(46)
[(minus120597
120597119902+119882
119902(119902)) minus (minus
120597
120597119901+ 119881
119901(119901))]120595
2(119902) 120601
2(119901)
= radic21205761199021205951 (119902) 1206012 (119901) minus radic2120576119901 1205952 (119902) 1206011 (119901)
(47)
where 120576 = 120576119902minus120576
119901and 120576
119902and 120576
119901are the eigenvalues of119867
119902and
119867119901 respectively The technique now is to devise an iterative
approximation scheme to solve (46) and (47) by taking atrial wave function for 120594
2(119902 119901) substitute this into the first
equation (46) and integrate it to obtain an approximationfor 120594
1(119902 119901) This can be used as an ansatz in the second
equation (47) to find an improved solution for 1205942(119902 119901) and
so forth As it was shown in [13] the procedure converges forwell-behaved potentials with a judicious choice of initial trialfunction If the119882
119902and 119881
119901are odd then
1205951(minus119902) = 120595
2(119902) 120601
1(minus119901) = 120601
2(119901) (48)
since they satisfy the same eigenvalue equation It is straight-forward then for example to obtain
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205951 (minus119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206011 (minus119901)
(49)
The independent nature of 119902 and119901 gives the freedomof taking119902 = 0 119901 = 0 which yield an expression for energies asfollows
radic2120576119902 = 119882(0) +1205951015840
1(0)
1205951 (0)
radic2120576119901 = 119881 (0) +1206011015840
1(0)
1206011 (0)
(50)
Suppose that the potentials 119882119902(119902) and 119881
119901(119901) have a maxi-
mum at 119902minusand 119901
minus and minimum at 119902
+and 119901
+ respectively
For the simplicity sake we choose the trial wave functions as
120595(0)
12(119902) = 120575 (119902 minus 119902
plusmn) 120601
(0)
12(119901) = 120575 (119901 minus 119901
plusmn) (51)
6 ISRNMathematical Physics
After one iteration we obtain
120594(1)
1(119902 119901) =
1
119873119902119873119901
120579 (119902 minus 119902minus) 120579 (119901 minus 119901
minus)
times 119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
120594(1)
2(119902 119901) =
1
119873119902119873119901
120579 (119902+minus 119902) 120579 (119901
+minus 119901)
times 119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
(52)
where 119873119902and 119873
119901are the normalization factors The next
approximation leads to
120594(2)
1(119902 119901) =
1
1198731015840119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
times int
infin
max(minus119902119902minus)119890minus2int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
infin
max(minus119901119901minus)1198902 int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
120594(2)
2(119902 119901) =
1
1198731015840119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
times int
min(minus119902119902+)
infin
1198902 int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
min(minus119901119901+)
infin
119890minus2int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
(53)
It can be easily verified that to this level of precision (52) isself-consistent solution Actually for example for 1199021015840 gt 119902
minusthe
exponential 119890minus2int1199021015840
0119882(11990210158401015840)11988911990210158401015840
will peak sharply around 119902+and
may be approximated by a 120575-function 119888120575(119902+minus 119902
1015840) similarly
1198902 int1199021015840
0119882(11990210158401015840)11988911990210158401015840
may be replaced approximately by 119888120575(119902minusminus 119902
1015840)
for 1199021015840 lt 119902+ The same arguments hold for the 119901-space
With these approximations equations (53) reduce to (52)Thenormalization constant1198731015840 is
1198731015840= (int
infin
119902minus
119889119902119890minus2int119902
0119882(1199021015840)1198891199021015840
int
infin
119901minus
119889119901119890minus2 int1199011015840
0119881(1199011015840)1198891199011015840
)
32
(54)
The energy expectation value
120576 = (1205941 119867ext1205941) (55)
gives the same result as that obtained for odd potentialsby means of (50) and (53) Assuming the exponentials119890minus2int0
119902minus119882(119902)119889119902 and 119890minus2int
0
119901minus119881(119901)119889119901 to be small which is correct to
the same approximations underlying (55) the difference isnegligible and the integrals in both cases may be replacedby Gaussians around 119902
+and 119901
+ respectively Hence it is
straightforward to obtain
120576 =ℎ119882
1015840(119902+)
2120587119890minus2Δ119882ℎ
minusℎ119881
1015840(119901
+)
2120587119890minus2Δ119881ℎ
(56)
which gives direct evidence for the SUSY breaking in theextended phase space quantum mechanical system Here wehave reinstated ℎ to show the order of adopted approxima-tion and its non-perturbative nature We also denoted
Δ119882 = int
119902minus
119902+
119882(119902) 119889119902 Δ119881 = int
119901minus
119901+
119881 (119901) 119889119901 (57)
However a more practical measure for the SUSY breakingin particular in field theories is the expectation value ofan auxiliary field which can be replaced by its equation ofmotion right from the start as follows
⟨119865⟩ = (120594uarr 119894 119876+ 120590minus120594uarr) (58)
Taking into account the relation 119876+120594uarr
= 0 with 119876+
commuting with 119867ext which means that the intermediatestate must have the same energy as 120594 (58) can be written interms of a complete set of states as
⟨119865⟩ = 119894 (120594uarr 119876+120594darr) (120594darr 120590minus 120594uarr) (59)
According to (55) we have
120576 = ⟨119867ext⟩ = (120594uarr 119867ext120594uarr) =1
2(120594
uarr 119876
+120594darr) (120594
darr 119876
minus120594uarr)
= 120576119902minus 120576
119901= ⟨119867
119902⟩ minus ⟨119867
119901⟩ = (120595
uarr 119867
119902120595uarr) minus (120601
uarr 119867
119901120601uarr)
=1
2(120595
uarr 119876
119902+120595darr) (120595
darr 119876
119902minus120595uarr)
minus1
2(120601
uarr 119876
119901+120601darr) (120601
darr 119876
119901minus120601uarr)
(60)
where 120594uarrdarr= 120595
uarrdarr120601uarrdarr 120595
uarr= (
1205951
0) 120595
darr= (
0
1205952) 120601
uarr= (
1206011
0) and
120601darr= (
0
1206012) From SUSY algebra it follows immediately that
1
radic120576119876minus120594uarr= 120594
darr=
minus120594uarr
1
radic120576119902
119876119902minus120595uarr= 120595
darr=
minus120595uarr
1
radic120576119901
119876119901minus120601uarr= 120601
darr=
minus120601uarr
(61)
By virtue of (61) (60) reads
radic120576 (120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= radic120576119902 (120595uarr 119876119902+120595darr) (120595darr minus120595uarr)
minus radic120576119901 (120601uarr 119876119901+120601darr) (120601darr minus120601uarr)
(62)
ISRNMathematical Physics 7
Using the matrix representations of119876119902+ 119876
119901+ and
minusand the
wave functions equation (53) one gets [13]
(120595darr
minus120595uarr) = radic
1198821015840(119902+)
120587119890minusΔ119882
Δ119902
(120601darr
minus120601uarr) = radic
1198811015840(119901
+)
120587119890minusΔ119881
Δ119901
(120595uarr 119876
119902+120595darr) = 119894radic
1198821015840(119902minus)
120587119890minusΔ119882
(120601uarr 119876
119901+120601darr) = 119894radic
1198811015840(119901
minus)
120587119890minusΔ119881
(63)
where Δ119902 = 119902+minus 119902
minusand Δ119901 = 119901
+minus 119901
minus Hence
(120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= 2119894radic120576[
[
(
120576119902
120576)radic120576
119902radic119882
1015840(119902minus)
120587Δ119902
minus (
120576119901
120576)radic120576
119901radic1198811015840(119901
minus)
120587Δ119901]
]
(64)
⟨119865⟩ = minus2radic120576 [
[
(
120576119902
120576)radic
1198821015840(119902+)
120587119890minus2Δ119882
Δ119902
minus (
120576119901
120576)radic
1198811015840(119901)
120587119890minus2Δ119881
Δ119901]
]
(65)
Along the actual trajectories in 119902-space (65) reproduces theresults obtained in [13]
5 An Extended SUSY Breaking in theInstanton Picture
In this Section our goal is to show that the expressionsequations (64) and (65) can be obtained in the path integralformulation of the theory by calculating the matrix elementsthat is the effect of tunneling between two classical vacuaby using a one-instanton background That is the matrixelements of
plusmn 119876
119902plusmn and 119876
119901plusmncan be calculated in the
background of the classical solution 119902119888= minus119882
119888and
119888= minus119881
119888
In doing this we rewrite the matrix element equation (62) interms of eigenstates of the conjugate operator
plusmnas follows
radic120576 [⟨+0119902+119901+
1003816100381610038161003816 119890minus119894119867ext(119879minus119905)119876
+119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816
times 119890minus119894119867ext(119879minus119905)
minus119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902+119901+0+⟩]119879rarrminus119894infin
= radic120576119902 [⟨+0119902+1003816100381610038161003816 119890
minus119894119867119902(119879minus119905)119876119902+119890minus119894119867119902(119879+119905) 1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus
1003816100381610038161003816
times 119890minus119894119867119902(119879minus119905)
minus
10038161003816100381610038161003816119890minus119894119867119902(119879+119905)119902
+0+⟩]
119879rarrminus119894infin
minus radic120576119901 [⟨+0119901+1003816100381610038161003816 119890minus119894119867119901(119879minus119905)119876
119901+119890minus119894119867119901(119879+119905)
times1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus
1003816100381610038161003816 minus
10038161003816100381610038161003816119901+0+⟩ ]
119879rarrminus119894infin
(66)
in the limit 119879 rarr minus119894infin This reduces to
radic120576 ⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= radic120576119902 ⟨+0119902+1003816100381610038161003816119876119902+
1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus1003816100381610038161003816 minus
1003816100381610038161003816 119902+0+⟩
minus radic120576119901 ⟨+0119901+1003816100381610038161003816119876119901+
1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus1003816100381610038161003816 minus
1003816100381610038161003816119901+0+⟩
(67)
which in turn can be presented by path integrals definedin terms of anticommuting 119888-number operators 120577 and 120578
with Euclidean actions of the instantons in 119902- and 119901-spacesrespectively Following [13] these functional integrals includean integration over instanton time 120591
0which is due to the
problem of zero modes of the bilinear terms in Euclideanactions This arises from time-transformation of instantonsand SUSY transformations on them respectively The exis-tence of zero modes gives rise to non-Gaussian behaviour ofthe functional integral Due to it the matrix elements abovedo not receive any contributions from either no-instantonor anti-instanton configurations The zero mode problem issolved by introducing a collective coordinate 120591
0replacing the
bosonic zero mode [14] Whereas the functional integralsdepend only on the difference 120591 minus 120591
0 Note also that multi-
instanton configurations could contribute in principle pro-vided they have not more than one normalizable fermioniczero mode But as it was shown in [13] their contribution isclearly smaller with respect to radic2120576119902 and radic2120576119901 In the casewhen the SUSY potentials in 119902- and 119901-spaces have morethan two extrema 119902] and 119901120583 ] 120583 = 1 2 119873 one can putconditions on the SUSY potentials as follows
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr infin at 119902 997888rarr plusmninfin for 120595+
0
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr minusinfin at 119902 997888rarr plusmninfin for 120595minus
0
(68)
and similar to 119881(119901) that the extrema are well separated asfollows int119902]+1
119902]
119882(1199021015840)119889119902
1015840≫ 1 int119902120583+1
119901120583
119881(1199011015840)119889119901
1015840≫ 1 Around
each of the classical minima 119902] and119901120583 of the potentials1198822(119902)
and 1198812(119901) respectively one can approximate the theory
by a supersymmetric harmonic oscillator Then there are119873 ground states which have zero energy These states aredescribed by upper or lower component of the wave functiondepending on whether ] and 120583 are odd or even With thisprovision the functional integrals are calculated in [13] whichallow us consequently to write
⟨+0119902+
1003816100381610038161003816119876119902+1003816100381610038161003816 119902minus0minus⟩ = 119894
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888
⟨minus0119902minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+0+⟩ =
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888Δ119902
119888
(69)
8 ISRNMathematical Physics
and so forth Inserting this in (67) we arrive at (64)
⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= 2119894radic120576[
[
(
120576119902
120576)radic120576119902
radic119882
1015840
119888(119902+)
120587Δ119902
119888
minus (
120576119901
120576)radic120576119901
radic1198811015840
119888(119901
+)
120587Δ119901
119888]
]
(70)
and thus of (65) as its inevitable corollary This proves thatthe extended SUSY breaking has resulted from tunnelingbetween the classical vacua of the theory The correctionsto this picture are due to higher-order terms and quantum-tunneling effects
6 Spectrum Generating Algebra
An extended Hamiltonian 119867ext equation (27) can be treatedas a set of two ordinary two-dimensional partner Hamiltoni-ans [4] as follows
119867plusmn=1
2[120587
2
119902minus 120587
2
119901+ 119880
plusmn(119902 119901)] (71)
provided by partner potentials
119880plusmn(119902 119901) = 119880
119902plusmn(119902) minus 119880
119901plusmn(119901)
119880119902plusmn(119902) = 119882
2(119902 119886
119902) ∓119882
1015840
119902(119902 119886
119902)
119880119901plusmn(119901) = 119881
2(119901 119886
119901) ∓ 119881
1015840
119901(119901 119886
119901)
(72)
A subset of the SUSY potentials for which the Schrodinger-like equations are exactly solvable share an integrabilityconditions of shape-invariance [15] as follows
119880+(1198860 119902 119901) = 119880
minus(1198861 119902 119901) + 119877 (119886
0) 119886
1= 119891 (119886
0)
(73)
where 1198860and 119886
1are a set of parameters that specify phase-
space-independent properties of the potentials and thereminder 119877(119886
0) is independent of (119902 119901)
61 Algebraic Properties of Shape Invariance Using the stan-dard technique we may construct a series of Hamiltonians119867119873 119873 = 0 1 2
119867119873=1
2[120587
2
119902minus 120587
2
119901+ 119880
minus(119886119873 119902 119901) +
119873
sum
119896=1
119877 (119886119896)] (74)
where 119886119873= 119891
(119873)(119886) (119873 is the number of iterations) From
(72) and (73) we obtain then 119873 = 119899 + 119898 coupled nonlineardifferential equations which are the two recurrence relationsof Riccati-type differential equations as follows
1198822
119899+1(119902) + 119882
1015840
119902(119899+1)(119902) = 119882
2
119899(119902) minus 119882
1015840
119902119899(119902) minus 120583
119899
1198812
119898+1(119901) + 119881
1015840
119901(119898+1)(119901) = 119881
2
119898(119901) minus 119881
1015840
119901119898(119901) minus ]
119898
(75)
where we denote 119882119899(119902) equiv 119882(119902 119886
119902119899) 119881
119898(119901) equiv 119881(119901 119886
119901119898)
120583119899equiv 119877
119902(119886119902119899) and ]
119898equiv 119877
119901(119886119901119898) Here we admit that
for unbroken SUSY the eigenstates of the potentials 119880119902119901
respectively are
119864(minus)
1199020= 0 119864
(minus)
119902119899=
119899minus1
sum
119894=0
120583119894 119864
(minus)
1199010= 0 119864
(minus)
119901119898=
119898minus1
sum
119895=0
]119895
(76)
that is the ground states are at zero energies characteristic ofunbroken supersymmetryThe differential equations (75) canbe investigated to find exactly solvable potentials The shapeinvariance condition equation (73) can be expressed in termsof bosonic operators as
119861+(119909 119886
0) 119861
minus(119909 119886
0) minus 119861
minus(119909 119886
1) 119861
+(119909 119886
1)
= 119877 (1198860) = 120583
0minus ]
0
119861aelig+ (aelig 119886aelig0) 119861aeligminus (aelig 119886aelig0) minus 119861aeligminus (aelig 119886aelig1) 119861aelig+ (aelig 119886aelig1)
= (1205830or ]
0)
(77)
where 119909(119902 119901)- is the coordinate in (119902 119901)-space aelig denotesconcisely either 119902- or 119901-representations (no summation onaelig is assumed) To classify algebras associated with the shapeinvariance following [16] we introduce an auxiliary variables120601(120601
119902 120601119901) and define the following creation and annihilation
operators
119869+= 119890
119894119896120601119861+(119909 120594 (119894120597
120601)) 119869
minus= 119861
minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601
(78)
where 119896(119896119902 119896119901) are an arbitrary real constants and 120594(120594
119902 120594119901)
are an arbitrary real functions Consequently the creationand annihilation operators in (119902 119901)-spaces can be written as
119869aelig+ = 119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig))
119869aeligminus = 119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig
(79)
The operators 119861plusmn(119909 120594(119894120597
120601)) and 119861aeligplusmn(aelig 120594aelig(119894120597120601aelig )) are the
generalization of (77) where 1198860rarr 120594(119894120597
120601) and 119886aelig0 rarr
120594aelig(119894120597120601aelig ) One can easily prove the following relations
119890119894119896120601119861+(119909 120594 (119894120597
120601)) = 119861
+(119909 120594 (119894120597
120601+ 119896)) 119890
119894119896120601
119861minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601= 119890
minus119894119896120601119861minus(119909 120594 (119894120597
120601+ 119896))
(80)
and that
119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig)) = 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119890
119894119896aelig120601aelig
119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig = 119890
minus119894119896aelig120601aelig119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) (81)
If we choose a function 120594(119894120597120601) such that 120594(119894120597
120601+ 119896) =
119891[120594(119894120597120601)] then we have identified 119886
0rarr 120594(119894120597
120601) and
1198861= 119891(119886
0) rarr 119891[120594(119894120597
120601)] = 120594(119894120597
120601+ 119896) Similar relations can
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
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Volume 2014 Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Stochastic AnalysisInternational Journal of
2 ISRNMathematical Physics
2 The Integrals of Motion
For the benefit of those not familiar with the framework ofextended phase space quantization enough details are givenin the following tomake the rest of the paper understandableThe interested reader is invited to consult the original papers[1 2] for further details In the framework of the proposedformalism the extended Lagrangian can be written as
Lext (119901 119902 119902) = minus 119902119894119901119894minus 119902
119894119894+L
119902+L
119901 (1)
where a dynamical system with 119873 degrees of freedomdescribed by the 2119873 independent coordinates 119902= (119902
1 119902
119873)
and momenta 119901 = (1199011 119901
119873) which are not in gen-
eral canonical pairs A Lagrangian L119902(119902 119902) is given in
119902-representation and the corresponding L119901(119901 ) in 119901-
representation Adotwill indicate differentiationwith respectto 119905 The independent nature of 119901 and 119902 gives the freedom ofintroducing a second set of canonical momenta for both 119901and 119902 through the extended Lagrangian
120587119902119894=120597Lext120597 119902
119894
=120597L119902
120597 119902119894
minus 119901119894
120587119901119894=120597Lext120597
119894
=120597L119901
120597119894
minus 119902119894
(2)
One may now define an extended Hamiltonian
119867ext (119901 119902 120587119901 120587119902) = 120587119902119894 119902119894 + 120587119901119894 119894 minusLext (119901 119902 119902)
= 119867 (119901 + 120587119902 119902) minus 119867 (119901 119902 + 120587
119901)
(3)
where 119867(119901 119902) = 119901119894119902119894minusL119902
= 119902119894119894minusL119901 is the conventional
Hamiltonian of the system In particular vanishing of 120587119902or
120587119901is the condition for 119901 and 119902 to constitute a canonical
pair In the language of statistical quantum mechanics thischoice picks up a pure state (actual path) Otherwise one isdealing with a mixed state (virtual path) One may howeverenvisage that the full machinery of the conventional quantummechanical dynamics is extendible to the extended dynamicsas alluded to the above Here 119901 and 119902 will be considered asindependent 119888-number operators on the integrable complexfunction 120594(119902 119901) One of the key assumptions of extendedphase space quantization [1 2] is the differential operatorsand commutation brackets for 120587
119901and 120587
119902borrowed from the
conventional quantum mechanics as follows
120587119902119894= minus119894
120597
120597119902119894
[120587119902119894 119902119895] = minus119894120575
119894119895
120587119901119894= minus119894
120597
120597119901119894
[120587119901119894 119901
119895] = minus119894120575
119894119895
(4)
Note also the following
[119901119894 119902119895] = [119901
119894 119901
119895] = [119902
119894 119902119895] = [120587
119901119894 120587
119902119895]
= [120587119901119894 120587
119901119895] = [120587
119902119894 120587
119902119895] = 0
(5)
By the virtue of (4) and (5) 119867ext is now an operator on 120594Along the trajectories in (119901 119902)-space however it producesthe state functions 120594(119901 119902 119905) via the following Schrodinger-like equation
119894120597
120597119905120594 = 119867ext 120594 (6)
Solutions of (6) are
120594 (119902 119901 119905) = 120594119903(119902 119901 119905) 119890
minus119894119901119902
= 119886120572120573120595120572(119902 119905) 120601
lowast
120573(119901 119905) 119890
minus119894119901119902
(7)
where 119886 = 119886dagger positive definite tr 119886 = 1 and 120595
120572and
120601lowast
120572are solutions of the conventional Schrodinger equation
in 119902- and 119901-representations respectively They are mutuallyFourier transforms Note that the 120572 and 120573 are not in generaleigenindices The normalizable 120594 (int120594119889119901119889119902 = tr(119886) = 1)is a physically acceptable solution The exponential factor isa consequence of the total time derivative minus119889(119902119901)119889119905 in (1)which can be eliminated Actually it is easily verified that
(119901 + 120587119902) 120594
119903(119902 119901 119905) = (120587
119902120594119903(119902 119901 119905)) 119890
minus119894119901119902 (8)
and so on Substitution of (8) in (6) gives
119894120597
120597119905120594 (119902 119901 119905) = 119867ext 120594119903 (119902 119901 119905) (9)
provided by the reducedHamiltonian119867ext From now onwereplace119867ext by119867ext and 120594119903(119902 119901 119905) by 120594119903(119902 119901 119905) respectivelyand retain former notational conventions
It is certainly desirable to derive the classical analog of theextended phase space quantummechanics of the particlewithodd degrees of freedom directly from what may be taken asthe first principleTherefore following [10ndash12] let us considera nonrelativistic particle of unit mass with two (120572 = 1 2)odd (Grassmann) degrees of freedomThe classical extendedLagrangian equation (1) can be written
Lext (119901 119902 119902) = minus 119902119901 minus 119902 +1
21199022minus 119865 (119902) +
1
22
minus 119866 (119901) minus 119877 (119902 119901)119873 +1
2120595120572120572
(10)
provided by 119873 = 12059511205952= minus119894120595
+120595minus Here 119865(119902) R rarr
R 119866(119901) R rarr R and 119877(119902 119901) R rarr R are arbitrarypiecewise continuously differentiable functions given overthe 1-dimensional Euclidean space R The 120595
120572are two odd
(Grassmann) degrees of freedom The nontrivial Poisson-Dirac brackets of the system (10) are
119902 120587119902 = 1 119901 120587
119901 = 1 120595
120572 120595
120573 = 120575
120572120573
120595+ 120595
minus = 1 120595
2
plusmn= 0 120595
plusmn=1
radic2(120595
1plusmn 119894120595
2)
(11)
The extended Hamiltonian119867ext (3) reads
119867ext (119901 119902 120587119901 120587119902) =1
2(119901 + 120587
119902)2
+ 1198652(119902) minus
1
2(119902 + 120587
119901)2
minus 1198662(119901) + 119877 (119902 119901)119873
(12)
ISRNMathematical Physics 3
which according to (8) reduces to
119867ext (119901 119902 120587119901 120587119902) =1
21205872
119902+ 119865
2(119902) minus
1
21205872
119901
minus 1198662(119901) + 119877 (119902 119901)119873
(13)
TheHamiltonian equation (13) yields the following equationsof motion
119902 = 120587119902 = 120587
119901
119902= minus119865
1015840
119902(119902) minus 119877
1015840
119902(119902 119901)119873
119901= minus119866
1015840
119901(119901) + 119877
1015840
119901(119902 119901)119873
plusmn= plusmn119894119877 (119902 119901) 120595
plusmn
(14)
Aprimewill indicate differentiationwith respect either to 119902 or119901 Thus119873 is the integral of motion additional to119867ext Alongthe trajectories 119902(119905) and 119901(119905) in (119901 119902)-spaces the solution toequations of motion for odd variables is
120595plusmn (119905) = 120595plusmn (1199050) exp [plusmn119894 int
119905
1199050
119877 (119902 (120591) 119901 (120591)) 119889120591] (15)
Hence the odd quantities
120579plusmn= 120579
plusmn (119905) exp [∓119894 int119905
1199050
119877 (119902 (120591) 119901 (120591)) 119889120591] (16)
are nonlocal in time integrals of motion In trivial case 119877 =
0 we have plusmn= 0 and 120579
plusmn= 120579
plusmn Suppose that the system
has even complex conjugate quantities119861119902119901plusmn
(119861119902119901+
)lowast= 119861
119902119901minus
whose evolution looks up to the term proportional to119873 likethe evolution of odd variables in (14)Then local odd integralsof motion could be constructed in the form
119876119902119901plusmn
= 119861119902119901∓
120595plusmn (17)
Let us introduce the oscillator-like bosonic variables 119861119902119901plusmn
in119902- and 119901-representations as follows
119861119902∓L
2(R) 997888rarrL
2(R) 119861
119902∓= [119901 + 120587
119902plusmn 119894119882 (119902)]
119861119901∓L
2(R) 997888rarrL
2(R) 119861
119901∓= [119902 + 120587
119901plusmn 119894119881 (119901)]
(18)
In the expressions (18)119882(119902) R rarr R and119881(119901) R rarr Rare the piecewise continuously differentiable functions calledSUSY potentials In particular case if119877(119902 119901) = 119877
119902(119902)minus119877
119901(119901)
for the evolution of 119861119902119901plusmn
we obtain
119902∓= [minus (119865
1015840
119902+ 119877
1015840
119902119873) plusmn 119894119882
1015840
119902(119902) (119901 + 120587
119902)]
119901∓= [minus (119866
1015840
119901+ 119877
1015840
119901119873) plusmn 119894119881
1015840
119901(119901) (119902 + 120587
119901)]
(19)
Consequently
119902plusmn= plusmn119894 [(119882
1015840
119902minus 119877
1015840
119902plusmn) plusmn 119894 (119865
1015840
119902minus119882119882
1015840
119902) 120595
∓]
119901plusmn= plusmn119894 [(119881
1015840
119901minus 119877
1015840
119901plusmn) plusmn 119894 (119866
1015840
119901minus 119881119881
1015840
119901) 120595
∓]
(20)
This shows that either 119902plusmn= 0 or
119901plusmn= 0 when 1198821015840
119902(119902) =
1198771015840
119902plusmn(119902) and 119865
1015840
119902= (12)(119882
2)1015840
119902or 1198811015840
119901(119901) = 119877
1015840
119901plusmn(119901) and
1198661015840
119901= (12)(119881
2)1015840
119901 respectively Therefore when the functions
119877119902119901
and 119865(119902) 119866(119901) are related as
1198771015840
119902plusmn(119902) = 119882
1015840
119902(119902) 119865
119902=1
2(119882
2) + 119862
119902
1198771015840
119901plusmn(119901) = 119881
1015840
119901(119901) 119865
119901=1
2(119881
2) + 119862
119901
(21)
where 119862119902119901
are constants then odd quantities 119876119902119901plusmn
areintegrals of motion in addition to 119867ext and 119873 According to(3) and (13) let us present119867ext in the form119867ext = 119867119902
minus 119867119901
where
119867119902=1
21205872
119902+ 119865
2(119902) + 119877
119902119873
119867119901=1
21205872
119901+ 119866
2(119901) + 119877
119901119873
(22)
Then 119876119902119901plusmn
and 119873 together with the 119867119902and 119867
119901form the
classical analog of the extended phase space SUSY algebra asfollows
119876119902119901+
119876119902119901minus
= minus119894 (119867119902119901minus 119862
119902119901)
119867119902119901 119876
119902119901plusmn = 119876
119902119901plusmn 119876
119902119901plusmn = 0
119873119876119902119901plusmn
= plusmn119894119876119902119901plusmn
119873119867119902119901 = 0
(23)
with constants119862119902119901
playing a role of a central charges in (119902 119901)-spaces 119873 is classical analog of the grading operator Putting119862119902= 119862
119901= 0 we arrive at the classical analog of the extended
phase space SUSY quantummechanics given by the extendedLagrangian
Lext (119901 119902 119902) =1
21205872
119902minus1
2119882
2(119902) +
1
21205872
119901minus1
21198812(119901)
+ 12059511205952(119882
1015840
119902+ 119881
1015840
119901) +
1
2120595120572120572
(24)
We conclude that the classical system (10) is characterizedby the presence of two additional local in time odd integralsof motion equation (17) being supersymmetry generatorsAlong the actual trajectories in 119902-space (24) reproduces theresults obtained in [6]
3 The Path Integral Formulation
In the matrix formulation of extended phase space (119873 = 2)-SUSY quantum mechanics the
plusmnwill be two real fermionic
creation and annihilation nilpotent operators describingthe fermionic variables The
plusmn having anticommuting 119888-
number eigenvalues imply
plusmn= radic
1
2(
1plusmn 119894
2)
120572
120573 = 120575
120572120573
+
minus = 1
2
plusmn= 0
(25)
They can be represented by finite dimensional matrices plusmn=
120590plusmn where 120590plusmn = (120590
1plusmn120590
2)2 are the usual raising and lowering
4 ISRNMathematical Physics
operators for the eigenvalues of 1205903which is the diagonal Pauli
matrix The fermionic operator 119891 reads 119891 C2rarr C2
119891 =
(12)[+
minus] which commutes with the119867ext and is diagonal
in this representation with conserved eigenvalues plusmn12 Dueto it the wave functions become two-component objects asfollows
120594 (119902 119901) = (120594+12
(119902 119901)
120594minus12
(119902 119901)) = (
1205941(119902 119901)
1205942(119902 119901)
) = (
1205951(119902) 120601
1(119901)
1205952(119902) 120601
2(119901))
(26)
where the states 12059512(119902) 120601
12(119901) correspond to fermionic
quantum number 119891 = plusmn12 respectively in 119902- and 119901-spacesThey belong to Hilbert space H = H
0otimes C2
= [L2(R) otimes
L2(R)]otimesC2 Hence theHamiltonian119867ext of extended phase
space (119873 = 2)-SUSY quantummechanical system becomes a2 times 2matrix as follows
119867ext = (119867+
0
0 119867minus
) =1
2(
2
119902+119882
2(119902) + 119894119882
1015840
119902(119902) [
1
2])
minus1
2(
2
119901+ 119881
2(119901) + 119894119881
1015840
119902(119901) [
1
2])
(27)
To infer the extendedHamiltonian equation (27) equivalentlyone may start from the 119888-number extended Lagrangian ofextended phase space quantum field theory in (0 + 1)-dimensions in 119902- and 119901-spaces as follows
Lext (119901 119902 119902) = minus 119902119901 minus 119902 +1
2[(119889119902
119889119905)
2
minus1198822(119902)]
+ 1198911198821015840
119902(119902) +
1
2[(119889119901
119889119905)
2
minus 1198812(119901)]
+ 1198911198811015840
119901(119901)
(28)
In dealing with abstract space of eigenstates of the conjugateoperator
plusmnwhich have anticommuting 119888-number eigenval-
ues suppose that |00minus⟩ is the normalized zero-eigenstate of 119902and
minusas follows
119902 |00minus⟩ = 0 minus |00minus⟩ = 0 (29)
The state |00+⟩ is defined by
|00+⟩ = + |00minus⟩ = 0 (30)
then +|00+⟩ = 0
minus|00+⟩ = |00minus⟩ Taking into account
that daggerplusmn=
∓ we get
⟨∓00| plusmn = 0 ⟨∓00| ∓ = ⟨plusmn00| (31)
Now we may introduce the notation 120572 120573 for the anticom-muting eigenvalues of
plusmn Consistency requires
120572plusmn= minus
plusmn120572 120572 |00plusmn⟩ = plusmn |00plusmn⟩ 120572 (32)
The eigenstates of 119902 minuscan be constructed as
1003816100381610038161003816119902120572minus⟩ = 119890minus119894119902119901minus120572+
|00minus⟩ (33)
and thus
1199021003816100381610038161003816119902120572minus⟩ = 119902
1003816100381610038161003816119902120572minus⟩ minus
1003816100381610038161003816119902120572minus⟩ = 1205721003816100381610038161003816119902120572minus⟩ (34)
Then the 119902and
+eigenstates are obtained by Fourier
transformation as follows
1003816100381610038161003816 119902120573+⟩ = minusint119889120572119890120572120573 1003816100381610038161003816 119902120572minus⟩
10038161003816100381610038161003816120587119902120572plusmn⟩ = minusint119889119902119890
119894119902120587119902 1003816100381610038161003816 119902120572plusmn⟩
1003816100381610038161003816119901120573+⟩ = minusint119889120572119890120572120573 1003816100381610038161003816119901120572minus⟩
10038161003816100381610038161003816120587119901120572plusmn⟩ = minusint119889119901119890
119894119901120587119901 1003816100381610038161003816119901120572plusmn⟩
(35)
which gives
119902
10038161003816100381610038161003816120587119902120572plusmn⟩ = 120587
119902
10038161003816100381610038161003816120587119902120572plusmn⟩
+
10038161003816100381610038161003816(119902 120587
119902) 120573+⟩ = 120573
10038161003816100381610038161003816(119902 120587
119902) 120573+⟩
119901
10038161003816100381610038161003816120587119901120572plusmn⟩ = 120587
119901
10038161003816100381610038161003816120587119901120572plusmn⟩
+
10038161003816100381610038161003816(119901 120587
119901) 120573+⟩ = 120573
10038161003816100381610038161003816(119901 120587
119901) 120573+⟩
(36)
The following completeness relations hold
minus int1198891205721198891199021003816100381610038161003816 119902120572plusmn⟩⟨∓120572
lowast1199021003816100381610038161003816 = 1
minus int119889120572
119889120587119902
2120587
10038161003816100381610038161003816120587119902120572plusmn⟩⟨∓120572
lowast120587119902
10038161003816100381610038161003816= 1
minus int1198891205721198891199011003816100381610038161003816119901120572plusmn⟩⟨∓120572
lowast1199011003816100381610038161003816 = 1
minus int119889120572
119889120587119901
2120587
10038161003816100381610038161003816120587119901120572plusmn⟩⟨∓120572
lowast120587119901
10038161003816100381610038161003816= 1
(37)
The time evolution of the state |119905⟩ is now given as follows
120594minus(119902120572119901120573119905) = minusint119889120572
1015840119889119902
1015840119889120573
1015840119889119901
1015840119870(119902120572119901120573119905 | 119902
10158401205721015840119901101584012057310158401199051015840)
(38)
The kernel reads
119870(119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840)
= ⟨+119902120572lowast119901120573
lowast1003816100381610038161003816 119890minus119894119867ext(119905minus119905
1015840) 100381610038161003816100381610038161199021015840120572101584011990110158401205731015840⟩
(39)
which can be evaluated by the path integral Actually analternative approach to describe the state space and dynamicsof the extended phase space quantum system is by the pathintegral [3] which reads
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) = ⟨119902119901119891
1003816100381610038161003816 119890minus119894119867ext(119905minus119905
1015840) 10038161003816100381610038161003816119902101584011990110158401198911015840⟩ (40)
In the path integral equation (40) the individual states arecharacterized by the energy and the fermionic quantum
ISRNMathematical Physics 5
number 119891 With the Hamiltonian 119867ext the path integralequation (40) is diagonal as follows
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840)
=K1198911198911015840 (119902119905 | 119902
10158401199051015840)K
1198911198911015840 (119901119905 | 119901
10158401199051015840)
= 1205751198911198911015840 int
119902
1199021015840
D119902int119901
1199011015840
D119901 exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(41)
Knowing the path integral equation (41) it is sufficient tospecify the initial wave function 120594
119891(1199021015840 119901
1015840 1199051015840) to obtain all
possible information about the system at any later time 119905 by
120594119891(119902 119901 119905) = sum
1198911015840
int1198891199021015840119889119901
1015840K
1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) 120594
1198911015840 (119902
1015840 119901
1015840 1199051015840)
(42)
with 120594plusmn12
(119902 119901 119905) = 12059412(119902 119901 119905) (26) In terms of anti-
commuting 119888-number operators 120577 and 120578 defining 120595 =
radic12 (120578+120577
119894(120578minus120577)) the path integral equation (41) becomes
K (119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840) = int
119902120572119901120573
1199021015840120572101584011990110158401205731015840
D119902D119901D120577D120578
times exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(43)
The functional integral is taken over all trajectories from 1199021015840 1205721015840to 119902 120572 and 1199011015840 1205731015840 to 119901 120573 between the times 1199051015840 and 119905
4 Solution of the Extended SchroumldingerEquation with Small Energy Eigenvalue 120576
Adopting the technique developed in [13] first we usethe iterative scheme to find the approximate ground statesolutions to the extended Schrodinger-like equation
119867ext120594 (119902 119901) = (119867119902minus 119867
119901) 120594 (119902 119901) = 120576120594 (119902 119901) (44)
with energy 120576Wewill then use these solutions to calculate theparameters which measure the breaking of extended SUSYsuch as the ground state energy The approximation whichwent into the derivation of solutions of (44) meets ourinterest that the ground state energy 120576 is supposedly smallAs we mentioned above the solutions for nonzero 120576 come inpairs of the form
120594uarr(119902 119901) = (
1205941(119902 119901)
0) or 120594
darr(119902 119901) = (
0
1205942(119902 119901)
)
(45)
related by supersymmetry where 12059412(119902 119901) = 120595
12(119902)120601
12(119901)
The state space of the system is defined by all the normalizablesolutions of (44) and the individual states are characterizedby the energies 120576
119902and the fermionic quantumnumber119891 One
of these solutions is acceptable only if119882(119902) and119881(119901) becomeinfinite at both 119902 rarr plusmninfin and 119901 rarr plusmninfin respectivelywith the same sign If this condition is not satisfied neitherof the solutions is normalizable nor they can represent theground state of the system Equation (44) yields the followingrelations between energy eigenstates with fermionic quantumnumber plusmn12
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205952 (119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206012 (119901)
(46)
[(minus120597
120597119902+119882
119902(119902)) minus (minus
120597
120597119901+ 119881
119901(119901))]120595
2(119902) 120601
2(119901)
= radic21205761199021205951 (119902) 1206012 (119901) minus radic2120576119901 1205952 (119902) 1206011 (119901)
(47)
where 120576 = 120576119902minus120576
119901and 120576
119902and 120576
119901are the eigenvalues of119867
119902and
119867119901 respectively The technique now is to devise an iterative
approximation scheme to solve (46) and (47) by taking atrial wave function for 120594
2(119902 119901) substitute this into the first
equation (46) and integrate it to obtain an approximationfor 120594
1(119902 119901) This can be used as an ansatz in the second
equation (47) to find an improved solution for 1205942(119902 119901) and
so forth As it was shown in [13] the procedure converges forwell-behaved potentials with a judicious choice of initial trialfunction If the119882
119902and 119881
119901are odd then
1205951(minus119902) = 120595
2(119902) 120601
1(minus119901) = 120601
2(119901) (48)
since they satisfy the same eigenvalue equation It is straight-forward then for example to obtain
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205951 (minus119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206011 (minus119901)
(49)
The independent nature of 119902 and119901 gives the freedomof taking119902 = 0 119901 = 0 which yield an expression for energies asfollows
radic2120576119902 = 119882(0) +1205951015840
1(0)
1205951 (0)
radic2120576119901 = 119881 (0) +1206011015840
1(0)
1206011 (0)
(50)
Suppose that the potentials 119882119902(119902) and 119881
119901(119901) have a maxi-
mum at 119902minusand 119901
minus and minimum at 119902
+and 119901
+ respectively
For the simplicity sake we choose the trial wave functions as
120595(0)
12(119902) = 120575 (119902 minus 119902
plusmn) 120601
(0)
12(119901) = 120575 (119901 minus 119901
plusmn) (51)
6 ISRNMathematical Physics
After one iteration we obtain
120594(1)
1(119902 119901) =
1
119873119902119873119901
120579 (119902 minus 119902minus) 120579 (119901 minus 119901
minus)
times 119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
120594(1)
2(119902 119901) =
1
119873119902119873119901
120579 (119902+minus 119902) 120579 (119901
+minus 119901)
times 119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
(52)
where 119873119902and 119873
119901are the normalization factors The next
approximation leads to
120594(2)
1(119902 119901) =
1
1198731015840119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
times int
infin
max(minus119902119902minus)119890minus2int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
infin
max(minus119901119901minus)1198902 int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
120594(2)
2(119902 119901) =
1
1198731015840119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
times int
min(minus119902119902+)
infin
1198902 int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
min(minus119901119901+)
infin
119890minus2int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
(53)
It can be easily verified that to this level of precision (52) isself-consistent solution Actually for example for 1199021015840 gt 119902
minusthe
exponential 119890minus2int1199021015840
0119882(11990210158401015840)11988911990210158401015840
will peak sharply around 119902+and
may be approximated by a 120575-function 119888120575(119902+minus 119902
1015840) similarly
1198902 int1199021015840
0119882(11990210158401015840)11988911990210158401015840
may be replaced approximately by 119888120575(119902minusminus 119902
1015840)
for 1199021015840 lt 119902+ The same arguments hold for the 119901-space
With these approximations equations (53) reduce to (52)Thenormalization constant1198731015840 is
1198731015840= (int
infin
119902minus
119889119902119890minus2int119902
0119882(1199021015840)1198891199021015840
int
infin
119901minus
119889119901119890minus2 int1199011015840
0119881(1199011015840)1198891199011015840
)
32
(54)
The energy expectation value
120576 = (1205941 119867ext1205941) (55)
gives the same result as that obtained for odd potentialsby means of (50) and (53) Assuming the exponentials119890minus2int0
119902minus119882(119902)119889119902 and 119890minus2int
0
119901minus119881(119901)119889119901 to be small which is correct to
the same approximations underlying (55) the difference isnegligible and the integrals in both cases may be replacedby Gaussians around 119902
+and 119901
+ respectively Hence it is
straightforward to obtain
120576 =ℎ119882
1015840(119902+)
2120587119890minus2Δ119882ℎ
minusℎ119881
1015840(119901
+)
2120587119890minus2Δ119881ℎ
(56)
which gives direct evidence for the SUSY breaking in theextended phase space quantum mechanical system Here wehave reinstated ℎ to show the order of adopted approxima-tion and its non-perturbative nature We also denoted
Δ119882 = int
119902minus
119902+
119882(119902) 119889119902 Δ119881 = int
119901minus
119901+
119881 (119901) 119889119901 (57)
However a more practical measure for the SUSY breakingin particular in field theories is the expectation value ofan auxiliary field which can be replaced by its equation ofmotion right from the start as follows
⟨119865⟩ = (120594uarr 119894 119876+ 120590minus120594uarr) (58)
Taking into account the relation 119876+120594uarr
= 0 with 119876+
commuting with 119867ext which means that the intermediatestate must have the same energy as 120594 (58) can be written interms of a complete set of states as
⟨119865⟩ = 119894 (120594uarr 119876+120594darr) (120594darr 120590minus 120594uarr) (59)
According to (55) we have
120576 = ⟨119867ext⟩ = (120594uarr 119867ext120594uarr) =1
2(120594
uarr 119876
+120594darr) (120594
darr 119876
minus120594uarr)
= 120576119902minus 120576
119901= ⟨119867
119902⟩ minus ⟨119867
119901⟩ = (120595
uarr 119867
119902120595uarr) minus (120601
uarr 119867
119901120601uarr)
=1
2(120595
uarr 119876
119902+120595darr) (120595
darr 119876
119902minus120595uarr)
minus1
2(120601
uarr 119876
119901+120601darr) (120601
darr 119876
119901minus120601uarr)
(60)
where 120594uarrdarr= 120595
uarrdarr120601uarrdarr 120595
uarr= (
1205951
0) 120595
darr= (
0
1205952) 120601
uarr= (
1206011
0) and
120601darr= (
0
1206012) From SUSY algebra it follows immediately that
1
radic120576119876minus120594uarr= 120594
darr=
minus120594uarr
1
radic120576119902
119876119902minus120595uarr= 120595
darr=
minus120595uarr
1
radic120576119901
119876119901minus120601uarr= 120601
darr=
minus120601uarr
(61)
By virtue of (61) (60) reads
radic120576 (120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= radic120576119902 (120595uarr 119876119902+120595darr) (120595darr minus120595uarr)
minus radic120576119901 (120601uarr 119876119901+120601darr) (120601darr minus120601uarr)
(62)
ISRNMathematical Physics 7
Using the matrix representations of119876119902+ 119876
119901+ and
minusand the
wave functions equation (53) one gets [13]
(120595darr
minus120595uarr) = radic
1198821015840(119902+)
120587119890minusΔ119882
Δ119902
(120601darr
minus120601uarr) = radic
1198811015840(119901
+)
120587119890minusΔ119881
Δ119901
(120595uarr 119876
119902+120595darr) = 119894radic
1198821015840(119902minus)
120587119890minusΔ119882
(120601uarr 119876
119901+120601darr) = 119894radic
1198811015840(119901
minus)
120587119890minusΔ119881
(63)
where Δ119902 = 119902+minus 119902
minusand Δ119901 = 119901
+minus 119901
minus Hence
(120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= 2119894radic120576[
[
(
120576119902
120576)radic120576
119902radic119882
1015840(119902minus)
120587Δ119902
minus (
120576119901
120576)radic120576
119901radic1198811015840(119901
minus)
120587Δ119901]
]
(64)
⟨119865⟩ = minus2radic120576 [
[
(
120576119902
120576)radic
1198821015840(119902+)
120587119890minus2Δ119882
Δ119902
minus (
120576119901
120576)radic
1198811015840(119901)
120587119890minus2Δ119881
Δ119901]
]
(65)
Along the actual trajectories in 119902-space (65) reproduces theresults obtained in [13]
5 An Extended SUSY Breaking in theInstanton Picture
In this Section our goal is to show that the expressionsequations (64) and (65) can be obtained in the path integralformulation of the theory by calculating the matrix elementsthat is the effect of tunneling between two classical vacuaby using a one-instanton background That is the matrixelements of
plusmn 119876
119902plusmn and 119876
119901plusmncan be calculated in the
background of the classical solution 119902119888= minus119882
119888and
119888= minus119881
119888
In doing this we rewrite the matrix element equation (62) interms of eigenstates of the conjugate operator
plusmnas follows
radic120576 [⟨+0119902+119901+
1003816100381610038161003816 119890minus119894119867ext(119879minus119905)119876
+119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816
times 119890minus119894119867ext(119879minus119905)
minus119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902+119901+0+⟩]119879rarrminus119894infin
= radic120576119902 [⟨+0119902+1003816100381610038161003816 119890
minus119894119867119902(119879minus119905)119876119902+119890minus119894119867119902(119879+119905) 1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus
1003816100381610038161003816
times 119890minus119894119867119902(119879minus119905)
minus
10038161003816100381610038161003816119890minus119894119867119902(119879+119905)119902
+0+⟩]
119879rarrminus119894infin
minus radic120576119901 [⟨+0119901+1003816100381610038161003816 119890minus119894119867119901(119879minus119905)119876
119901+119890minus119894119867119901(119879+119905)
times1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus
1003816100381610038161003816 minus
10038161003816100381610038161003816119901+0+⟩ ]
119879rarrminus119894infin
(66)
in the limit 119879 rarr minus119894infin This reduces to
radic120576 ⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= radic120576119902 ⟨+0119902+1003816100381610038161003816119876119902+
1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus1003816100381610038161003816 minus
1003816100381610038161003816 119902+0+⟩
minus radic120576119901 ⟨+0119901+1003816100381610038161003816119876119901+
1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus1003816100381610038161003816 minus
1003816100381610038161003816119901+0+⟩
(67)
which in turn can be presented by path integrals definedin terms of anticommuting 119888-number operators 120577 and 120578
with Euclidean actions of the instantons in 119902- and 119901-spacesrespectively Following [13] these functional integrals includean integration over instanton time 120591
0which is due to the
problem of zero modes of the bilinear terms in Euclideanactions This arises from time-transformation of instantonsand SUSY transformations on them respectively The exis-tence of zero modes gives rise to non-Gaussian behaviour ofthe functional integral Due to it the matrix elements abovedo not receive any contributions from either no-instantonor anti-instanton configurations The zero mode problem issolved by introducing a collective coordinate 120591
0replacing the
bosonic zero mode [14] Whereas the functional integralsdepend only on the difference 120591 minus 120591
0 Note also that multi-
instanton configurations could contribute in principle pro-vided they have not more than one normalizable fermioniczero mode But as it was shown in [13] their contribution isclearly smaller with respect to radic2120576119902 and radic2120576119901 In the casewhen the SUSY potentials in 119902- and 119901-spaces have morethan two extrema 119902] and 119901120583 ] 120583 = 1 2 119873 one can putconditions on the SUSY potentials as follows
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr infin at 119902 997888rarr plusmninfin for 120595+
0
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr minusinfin at 119902 997888rarr plusmninfin for 120595minus
0
(68)
and similar to 119881(119901) that the extrema are well separated asfollows int119902]+1
119902]
119882(1199021015840)119889119902
1015840≫ 1 int119902120583+1
119901120583
119881(1199011015840)119889119901
1015840≫ 1 Around
each of the classical minima 119902] and119901120583 of the potentials1198822(119902)
and 1198812(119901) respectively one can approximate the theory
by a supersymmetric harmonic oscillator Then there are119873 ground states which have zero energy These states aredescribed by upper or lower component of the wave functiondepending on whether ] and 120583 are odd or even With thisprovision the functional integrals are calculated in [13] whichallow us consequently to write
⟨+0119902+
1003816100381610038161003816119876119902+1003816100381610038161003816 119902minus0minus⟩ = 119894
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888
⟨minus0119902minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+0+⟩ =
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888Δ119902
119888
(69)
8 ISRNMathematical Physics
and so forth Inserting this in (67) we arrive at (64)
⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= 2119894radic120576[
[
(
120576119902
120576)radic120576119902
radic119882
1015840
119888(119902+)
120587Δ119902
119888
minus (
120576119901
120576)radic120576119901
radic1198811015840
119888(119901
+)
120587Δ119901
119888]
]
(70)
and thus of (65) as its inevitable corollary This proves thatthe extended SUSY breaking has resulted from tunnelingbetween the classical vacua of the theory The correctionsto this picture are due to higher-order terms and quantum-tunneling effects
6 Spectrum Generating Algebra
An extended Hamiltonian 119867ext equation (27) can be treatedas a set of two ordinary two-dimensional partner Hamiltoni-ans [4] as follows
119867plusmn=1
2[120587
2
119902minus 120587
2
119901+ 119880
plusmn(119902 119901)] (71)
provided by partner potentials
119880plusmn(119902 119901) = 119880
119902plusmn(119902) minus 119880
119901plusmn(119901)
119880119902plusmn(119902) = 119882
2(119902 119886
119902) ∓119882
1015840
119902(119902 119886
119902)
119880119901plusmn(119901) = 119881
2(119901 119886
119901) ∓ 119881
1015840
119901(119901 119886
119901)
(72)
A subset of the SUSY potentials for which the Schrodinger-like equations are exactly solvable share an integrabilityconditions of shape-invariance [15] as follows
119880+(1198860 119902 119901) = 119880
minus(1198861 119902 119901) + 119877 (119886
0) 119886
1= 119891 (119886
0)
(73)
where 1198860and 119886
1are a set of parameters that specify phase-
space-independent properties of the potentials and thereminder 119877(119886
0) is independent of (119902 119901)
61 Algebraic Properties of Shape Invariance Using the stan-dard technique we may construct a series of Hamiltonians119867119873 119873 = 0 1 2
119867119873=1
2[120587
2
119902minus 120587
2
119901+ 119880
minus(119886119873 119902 119901) +
119873
sum
119896=1
119877 (119886119896)] (74)
where 119886119873= 119891
(119873)(119886) (119873 is the number of iterations) From
(72) and (73) we obtain then 119873 = 119899 + 119898 coupled nonlineardifferential equations which are the two recurrence relationsof Riccati-type differential equations as follows
1198822
119899+1(119902) + 119882
1015840
119902(119899+1)(119902) = 119882
2
119899(119902) minus 119882
1015840
119902119899(119902) minus 120583
119899
1198812
119898+1(119901) + 119881
1015840
119901(119898+1)(119901) = 119881
2
119898(119901) minus 119881
1015840
119901119898(119901) minus ]
119898
(75)
where we denote 119882119899(119902) equiv 119882(119902 119886
119902119899) 119881
119898(119901) equiv 119881(119901 119886
119901119898)
120583119899equiv 119877
119902(119886119902119899) and ]
119898equiv 119877
119901(119886119901119898) Here we admit that
for unbroken SUSY the eigenstates of the potentials 119880119902119901
respectively are
119864(minus)
1199020= 0 119864
(minus)
119902119899=
119899minus1
sum
119894=0
120583119894 119864
(minus)
1199010= 0 119864
(minus)
119901119898=
119898minus1
sum
119895=0
]119895
(76)
that is the ground states are at zero energies characteristic ofunbroken supersymmetryThe differential equations (75) canbe investigated to find exactly solvable potentials The shapeinvariance condition equation (73) can be expressed in termsof bosonic operators as
119861+(119909 119886
0) 119861
minus(119909 119886
0) minus 119861
minus(119909 119886
1) 119861
+(119909 119886
1)
= 119877 (1198860) = 120583
0minus ]
0
119861aelig+ (aelig 119886aelig0) 119861aeligminus (aelig 119886aelig0) minus 119861aeligminus (aelig 119886aelig1) 119861aelig+ (aelig 119886aelig1)
= (1205830or ]
0)
(77)
where 119909(119902 119901)- is the coordinate in (119902 119901)-space aelig denotesconcisely either 119902- or 119901-representations (no summation onaelig is assumed) To classify algebras associated with the shapeinvariance following [16] we introduce an auxiliary variables120601(120601
119902 120601119901) and define the following creation and annihilation
operators
119869+= 119890
119894119896120601119861+(119909 120594 (119894120597
120601)) 119869
minus= 119861
minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601
(78)
where 119896(119896119902 119896119901) are an arbitrary real constants and 120594(120594
119902 120594119901)
are an arbitrary real functions Consequently the creationand annihilation operators in (119902 119901)-spaces can be written as
119869aelig+ = 119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig))
119869aeligminus = 119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig
(79)
The operators 119861plusmn(119909 120594(119894120597
120601)) and 119861aeligplusmn(aelig 120594aelig(119894120597120601aelig )) are the
generalization of (77) where 1198860rarr 120594(119894120597
120601) and 119886aelig0 rarr
120594aelig(119894120597120601aelig ) One can easily prove the following relations
119890119894119896120601119861+(119909 120594 (119894120597
120601)) = 119861
+(119909 120594 (119894120597
120601+ 119896)) 119890
119894119896120601
119861minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601= 119890
minus119894119896120601119861minus(119909 120594 (119894120597
120601+ 119896))
(80)
and that
119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig)) = 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119890
119894119896aelig120601aelig
119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig = 119890
minus119894119896aelig120601aelig119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) (81)
If we choose a function 120594(119894120597120601) such that 120594(119894120597
120601+ 119896) =
119891[120594(119894120597120601)] then we have identified 119886
0rarr 120594(119894120597
120601) and
1198861= 119891(119886
0) rarr 119891[120594(119894120597
120601)] = 120594(119894120597
120601+ 119896) Similar relations can
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
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Stochastic AnalysisInternational Journal of
ISRNMathematical Physics 3
which according to (8) reduces to
119867ext (119901 119902 120587119901 120587119902) =1
21205872
119902+ 119865
2(119902) minus
1
21205872
119901
minus 1198662(119901) + 119877 (119902 119901)119873
(13)
TheHamiltonian equation (13) yields the following equationsof motion
119902 = 120587119902 = 120587
119901
119902= minus119865
1015840
119902(119902) minus 119877
1015840
119902(119902 119901)119873
119901= minus119866
1015840
119901(119901) + 119877
1015840
119901(119902 119901)119873
plusmn= plusmn119894119877 (119902 119901) 120595
plusmn
(14)
Aprimewill indicate differentiationwith respect either to 119902 or119901 Thus119873 is the integral of motion additional to119867ext Alongthe trajectories 119902(119905) and 119901(119905) in (119901 119902)-spaces the solution toequations of motion for odd variables is
120595plusmn (119905) = 120595plusmn (1199050) exp [plusmn119894 int
119905
1199050
119877 (119902 (120591) 119901 (120591)) 119889120591] (15)
Hence the odd quantities
120579plusmn= 120579
plusmn (119905) exp [∓119894 int119905
1199050
119877 (119902 (120591) 119901 (120591)) 119889120591] (16)
are nonlocal in time integrals of motion In trivial case 119877 =
0 we have plusmn= 0 and 120579
plusmn= 120579
plusmn Suppose that the system
has even complex conjugate quantities119861119902119901plusmn
(119861119902119901+
)lowast= 119861
119902119901minus
whose evolution looks up to the term proportional to119873 likethe evolution of odd variables in (14)Then local odd integralsof motion could be constructed in the form
119876119902119901plusmn
= 119861119902119901∓
120595plusmn (17)
Let us introduce the oscillator-like bosonic variables 119861119902119901plusmn
in119902- and 119901-representations as follows
119861119902∓L
2(R) 997888rarrL
2(R) 119861
119902∓= [119901 + 120587
119902plusmn 119894119882 (119902)]
119861119901∓L
2(R) 997888rarrL
2(R) 119861
119901∓= [119902 + 120587
119901plusmn 119894119881 (119901)]
(18)
In the expressions (18)119882(119902) R rarr R and119881(119901) R rarr Rare the piecewise continuously differentiable functions calledSUSY potentials In particular case if119877(119902 119901) = 119877
119902(119902)minus119877
119901(119901)
for the evolution of 119861119902119901plusmn
we obtain
119902∓= [minus (119865
1015840
119902+ 119877
1015840
119902119873) plusmn 119894119882
1015840
119902(119902) (119901 + 120587
119902)]
119901∓= [minus (119866
1015840
119901+ 119877
1015840
119901119873) plusmn 119894119881
1015840
119901(119901) (119902 + 120587
119901)]
(19)
Consequently
119902plusmn= plusmn119894 [(119882
1015840
119902minus 119877
1015840
119902plusmn) plusmn 119894 (119865
1015840
119902minus119882119882
1015840
119902) 120595
∓]
119901plusmn= plusmn119894 [(119881
1015840
119901minus 119877
1015840
119901plusmn) plusmn 119894 (119866
1015840
119901minus 119881119881
1015840
119901) 120595
∓]
(20)
This shows that either 119902plusmn= 0 or
119901plusmn= 0 when 1198821015840
119902(119902) =
1198771015840
119902plusmn(119902) and 119865
1015840
119902= (12)(119882
2)1015840
119902or 1198811015840
119901(119901) = 119877
1015840
119901plusmn(119901) and
1198661015840
119901= (12)(119881
2)1015840
119901 respectively Therefore when the functions
119877119902119901
and 119865(119902) 119866(119901) are related as
1198771015840
119902plusmn(119902) = 119882
1015840
119902(119902) 119865
119902=1
2(119882
2) + 119862
119902
1198771015840
119901plusmn(119901) = 119881
1015840
119901(119901) 119865
119901=1
2(119881
2) + 119862
119901
(21)
where 119862119902119901
are constants then odd quantities 119876119902119901plusmn
areintegrals of motion in addition to 119867ext and 119873 According to(3) and (13) let us present119867ext in the form119867ext = 119867119902
minus 119867119901
where
119867119902=1
21205872
119902+ 119865
2(119902) + 119877
119902119873
119867119901=1
21205872
119901+ 119866
2(119901) + 119877
119901119873
(22)
Then 119876119902119901plusmn
and 119873 together with the 119867119902and 119867
119901form the
classical analog of the extended phase space SUSY algebra asfollows
119876119902119901+
119876119902119901minus
= minus119894 (119867119902119901minus 119862
119902119901)
119867119902119901 119876
119902119901plusmn = 119876
119902119901plusmn 119876
119902119901plusmn = 0
119873119876119902119901plusmn
= plusmn119894119876119902119901plusmn
119873119867119902119901 = 0
(23)
with constants119862119902119901
playing a role of a central charges in (119902 119901)-spaces 119873 is classical analog of the grading operator Putting119862119902= 119862
119901= 0 we arrive at the classical analog of the extended
phase space SUSY quantummechanics given by the extendedLagrangian
Lext (119901 119902 119902) =1
21205872
119902minus1
2119882
2(119902) +
1
21205872
119901minus1
21198812(119901)
+ 12059511205952(119882
1015840
119902+ 119881
1015840
119901) +
1
2120595120572120572
(24)
We conclude that the classical system (10) is characterizedby the presence of two additional local in time odd integralsof motion equation (17) being supersymmetry generatorsAlong the actual trajectories in 119902-space (24) reproduces theresults obtained in [6]
3 The Path Integral Formulation
In the matrix formulation of extended phase space (119873 = 2)-SUSY quantum mechanics the
plusmnwill be two real fermionic
creation and annihilation nilpotent operators describingthe fermionic variables The
plusmn having anticommuting 119888-
number eigenvalues imply
plusmn= radic
1
2(
1plusmn 119894
2)
120572
120573 = 120575
120572120573
+
minus = 1
2
plusmn= 0
(25)
They can be represented by finite dimensional matrices plusmn=
120590plusmn where 120590plusmn = (120590
1plusmn120590
2)2 are the usual raising and lowering
4 ISRNMathematical Physics
operators for the eigenvalues of 1205903which is the diagonal Pauli
matrix The fermionic operator 119891 reads 119891 C2rarr C2
119891 =
(12)[+
minus] which commutes with the119867ext and is diagonal
in this representation with conserved eigenvalues plusmn12 Dueto it the wave functions become two-component objects asfollows
120594 (119902 119901) = (120594+12
(119902 119901)
120594minus12
(119902 119901)) = (
1205941(119902 119901)
1205942(119902 119901)
) = (
1205951(119902) 120601
1(119901)
1205952(119902) 120601
2(119901))
(26)
where the states 12059512(119902) 120601
12(119901) correspond to fermionic
quantum number 119891 = plusmn12 respectively in 119902- and 119901-spacesThey belong to Hilbert space H = H
0otimes C2
= [L2(R) otimes
L2(R)]otimesC2 Hence theHamiltonian119867ext of extended phase
space (119873 = 2)-SUSY quantummechanical system becomes a2 times 2matrix as follows
119867ext = (119867+
0
0 119867minus
) =1
2(
2
119902+119882
2(119902) + 119894119882
1015840
119902(119902) [
1
2])
minus1
2(
2
119901+ 119881
2(119901) + 119894119881
1015840
119902(119901) [
1
2])
(27)
To infer the extendedHamiltonian equation (27) equivalentlyone may start from the 119888-number extended Lagrangian ofextended phase space quantum field theory in (0 + 1)-dimensions in 119902- and 119901-spaces as follows
Lext (119901 119902 119902) = minus 119902119901 minus 119902 +1
2[(119889119902
119889119905)
2
minus1198822(119902)]
+ 1198911198821015840
119902(119902) +
1
2[(119889119901
119889119905)
2
minus 1198812(119901)]
+ 1198911198811015840
119901(119901)
(28)
In dealing with abstract space of eigenstates of the conjugateoperator
plusmnwhich have anticommuting 119888-number eigenval-
ues suppose that |00minus⟩ is the normalized zero-eigenstate of 119902and
minusas follows
119902 |00minus⟩ = 0 minus |00minus⟩ = 0 (29)
The state |00+⟩ is defined by
|00+⟩ = + |00minus⟩ = 0 (30)
then +|00+⟩ = 0
minus|00+⟩ = |00minus⟩ Taking into account
that daggerplusmn=
∓ we get
⟨∓00| plusmn = 0 ⟨∓00| ∓ = ⟨plusmn00| (31)
Now we may introduce the notation 120572 120573 for the anticom-muting eigenvalues of
plusmn Consistency requires
120572plusmn= minus
plusmn120572 120572 |00plusmn⟩ = plusmn |00plusmn⟩ 120572 (32)
The eigenstates of 119902 minuscan be constructed as
1003816100381610038161003816119902120572minus⟩ = 119890minus119894119902119901minus120572+
|00minus⟩ (33)
and thus
1199021003816100381610038161003816119902120572minus⟩ = 119902
1003816100381610038161003816119902120572minus⟩ minus
1003816100381610038161003816119902120572minus⟩ = 1205721003816100381610038161003816119902120572minus⟩ (34)
Then the 119902and
+eigenstates are obtained by Fourier
transformation as follows
1003816100381610038161003816 119902120573+⟩ = minusint119889120572119890120572120573 1003816100381610038161003816 119902120572minus⟩
10038161003816100381610038161003816120587119902120572plusmn⟩ = minusint119889119902119890
119894119902120587119902 1003816100381610038161003816 119902120572plusmn⟩
1003816100381610038161003816119901120573+⟩ = minusint119889120572119890120572120573 1003816100381610038161003816119901120572minus⟩
10038161003816100381610038161003816120587119901120572plusmn⟩ = minusint119889119901119890
119894119901120587119901 1003816100381610038161003816119901120572plusmn⟩
(35)
which gives
119902
10038161003816100381610038161003816120587119902120572plusmn⟩ = 120587
119902
10038161003816100381610038161003816120587119902120572plusmn⟩
+
10038161003816100381610038161003816(119902 120587
119902) 120573+⟩ = 120573
10038161003816100381610038161003816(119902 120587
119902) 120573+⟩
119901
10038161003816100381610038161003816120587119901120572plusmn⟩ = 120587
119901
10038161003816100381610038161003816120587119901120572plusmn⟩
+
10038161003816100381610038161003816(119901 120587
119901) 120573+⟩ = 120573
10038161003816100381610038161003816(119901 120587
119901) 120573+⟩
(36)
The following completeness relations hold
minus int1198891205721198891199021003816100381610038161003816 119902120572plusmn⟩⟨∓120572
lowast1199021003816100381610038161003816 = 1
minus int119889120572
119889120587119902
2120587
10038161003816100381610038161003816120587119902120572plusmn⟩⟨∓120572
lowast120587119902
10038161003816100381610038161003816= 1
minus int1198891205721198891199011003816100381610038161003816119901120572plusmn⟩⟨∓120572
lowast1199011003816100381610038161003816 = 1
minus int119889120572
119889120587119901
2120587
10038161003816100381610038161003816120587119901120572plusmn⟩⟨∓120572
lowast120587119901
10038161003816100381610038161003816= 1
(37)
The time evolution of the state |119905⟩ is now given as follows
120594minus(119902120572119901120573119905) = minusint119889120572
1015840119889119902
1015840119889120573
1015840119889119901
1015840119870(119902120572119901120573119905 | 119902
10158401205721015840119901101584012057310158401199051015840)
(38)
The kernel reads
119870(119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840)
= ⟨+119902120572lowast119901120573
lowast1003816100381610038161003816 119890minus119894119867ext(119905minus119905
1015840) 100381610038161003816100381610038161199021015840120572101584011990110158401205731015840⟩
(39)
which can be evaluated by the path integral Actually analternative approach to describe the state space and dynamicsof the extended phase space quantum system is by the pathintegral [3] which reads
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) = ⟨119902119901119891
1003816100381610038161003816 119890minus119894119867ext(119905minus119905
1015840) 10038161003816100381610038161003816119902101584011990110158401198911015840⟩ (40)
In the path integral equation (40) the individual states arecharacterized by the energy and the fermionic quantum
ISRNMathematical Physics 5
number 119891 With the Hamiltonian 119867ext the path integralequation (40) is diagonal as follows
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840)
=K1198911198911015840 (119902119905 | 119902
10158401199051015840)K
1198911198911015840 (119901119905 | 119901
10158401199051015840)
= 1205751198911198911015840 int
119902
1199021015840
D119902int119901
1199011015840
D119901 exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(41)
Knowing the path integral equation (41) it is sufficient tospecify the initial wave function 120594
119891(1199021015840 119901
1015840 1199051015840) to obtain all
possible information about the system at any later time 119905 by
120594119891(119902 119901 119905) = sum
1198911015840
int1198891199021015840119889119901
1015840K
1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) 120594
1198911015840 (119902
1015840 119901
1015840 1199051015840)
(42)
with 120594plusmn12
(119902 119901 119905) = 12059412(119902 119901 119905) (26) In terms of anti-
commuting 119888-number operators 120577 and 120578 defining 120595 =
radic12 (120578+120577
119894(120578minus120577)) the path integral equation (41) becomes
K (119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840) = int
119902120572119901120573
1199021015840120572101584011990110158401205731015840
D119902D119901D120577D120578
times exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(43)
The functional integral is taken over all trajectories from 1199021015840 1205721015840to 119902 120572 and 1199011015840 1205731015840 to 119901 120573 between the times 1199051015840 and 119905
4 Solution of the Extended SchroumldingerEquation with Small Energy Eigenvalue 120576
Adopting the technique developed in [13] first we usethe iterative scheme to find the approximate ground statesolutions to the extended Schrodinger-like equation
119867ext120594 (119902 119901) = (119867119902minus 119867
119901) 120594 (119902 119901) = 120576120594 (119902 119901) (44)
with energy 120576Wewill then use these solutions to calculate theparameters which measure the breaking of extended SUSYsuch as the ground state energy The approximation whichwent into the derivation of solutions of (44) meets ourinterest that the ground state energy 120576 is supposedly smallAs we mentioned above the solutions for nonzero 120576 come inpairs of the form
120594uarr(119902 119901) = (
1205941(119902 119901)
0) or 120594
darr(119902 119901) = (
0
1205942(119902 119901)
)
(45)
related by supersymmetry where 12059412(119902 119901) = 120595
12(119902)120601
12(119901)
The state space of the system is defined by all the normalizablesolutions of (44) and the individual states are characterizedby the energies 120576
119902and the fermionic quantumnumber119891 One
of these solutions is acceptable only if119882(119902) and119881(119901) becomeinfinite at both 119902 rarr plusmninfin and 119901 rarr plusmninfin respectivelywith the same sign If this condition is not satisfied neitherof the solutions is normalizable nor they can represent theground state of the system Equation (44) yields the followingrelations between energy eigenstates with fermionic quantumnumber plusmn12
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205952 (119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206012 (119901)
(46)
[(minus120597
120597119902+119882
119902(119902)) minus (minus
120597
120597119901+ 119881
119901(119901))]120595
2(119902) 120601
2(119901)
= radic21205761199021205951 (119902) 1206012 (119901) minus radic2120576119901 1205952 (119902) 1206011 (119901)
(47)
where 120576 = 120576119902minus120576
119901and 120576
119902and 120576
119901are the eigenvalues of119867
119902and
119867119901 respectively The technique now is to devise an iterative
approximation scheme to solve (46) and (47) by taking atrial wave function for 120594
2(119902 119901) substitute this into the first
equation (46) and integrate it to obtain an approximationfor 120594
1(119902 119901) This can be used as an ansatz in the second
equation (47) to find an improved solution for 1205942(119902 119901) and
so forth As it was shown in [13] the procedure converges forwell-behaved potentials with a judicious choice of initial trialfunction If the119882
119902and 119881
119901are odd then
1205951(minus119902) = 120595
2(119902) 120601
1(minus119901) = 120601
2(119901) (48)
since they satisfy the same eigenvalue equation It is straight-forward then for example to obtain
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205951 (minus119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206011 (minus119901)
(49)
The independent nature of 119902 and119901 gives the freedomof taking119902 = 0 119901 = 0 which yield an expression for energies asfollows
radic2120576119902 = 119882(0) +1205951015840
1(0)
1205951 (0)
radic2120576119901 = 119881 (0) +1206011015840
1(0)
1206011 (0)
(50)
Suppose that the potentials 119882119902(119902) and 119881
119901(119901) have a maxi-
mum at 119902minusand 119901
minus and minimum at 119902
+and 119901
+ respectively
For the simplicity sake we choose the trial wave functions as
120595(0)
12(119902) = 120575 (119902 minus 119902
plusmn) 120601
(0)
12(119901) = 120575 (119901 minus 119901
plusmn) (51)
6 ISRNMathematical Physics
After one iteration we obtain
120594(1)
1(119902 119901) =
1
119873119902119873119901
120579 (119902 minus 119902minus) 120579 (119901 minus 119901
minus)
times 119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
120594(1)
2(119902 119901) =
1
119873119902119873119901
120579 (119902+minus 119902) 120579 (119901
+minus 119901)
times 119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
(52)
where 119873119902and 119873
119901are the normalization factors The next
approximation leads to
120594(2)
1(119902 119901) =
1
1198731015840119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
times int
infin
max(minus119902119902minus)119890minus2int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
infin
max(minus119901119901minus)1198902 int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
120594(2)
2(119902 119901) =
1
1198731015840119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
times int
min(minus119902119902+)
infin
1198902 int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
min(minus119901119901+)
infin
119890minus2int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
(53)
It can be easily verified that to this level of precision (52) isself-consistent solution Actually for example for 1199021015840 gt 119902
minusthe
exponential 119890minus2int1199021015840
0119882(11990210158401015840)11988911990210158401015840
will peak sharply around 119902+and
may be approximated by a 120575-function 119888120575(119902+minus 119902
1015840) similarly
1198902 int1199021015840
0119882(11990210158401015840)11988911990210158401015840
may be replaced approximately by 119888120575(119902minusminus 119902
1015840)
for 1199021015840 lt 119902+ The same arguments hold for the 119901-space
With these approximations equations (53) reduce to (52)Thenormalization constant1198731015840 is
1198731015840= (int
infin
119902minus
119889119902119890minus2int119902
0119882(1199021015840)1198891199021015840
int
infin
119901minus
119889119901119890minus2 int1199011015840
0119881(1199011015840)1198891199011015840
)
32
(54)
The energy expectation value
120576 = (1205941 119867ext1205941) (55)
gives the same result as that obtained for odd potentialsby means of (50) and (53) Assuming the exponentials119890minus2int0
119902minus119882(119902)119889119902 and 119890minus2int
0
119901minus119881(119901)119889119901 to be small which is correct to
the same approximations underlying (55) the difference isnegligible and the integrals in both cases may be replacedby Gaussians around 119902
+and 119901
+ respectively Hence it is
straightforward to obtain
120576 =ℎ119882
1015840(119902+)
2120587119890minus2Δ119882ℎ
minusℎ119881
1015840(119901
+)
2120587119890minus2Δ119881ℎ
(56)
which gives direct evidence for the SUSY breaking in theextended phase space quantum mechanical system Here wehave reinstated ℎ to show the order of adopted approxima-tion and its non-perturbative nature We also denoted
Δ119882 = int
119902minus
119902+
119882(119902) 119889119902 Δ119881 = int
119901minus
119901+
119881 (119901) 119889119901 (57)
However a more practical measure for the SUSY breakingin particular in field theories is the expectation value ofan auxiliary field which can be replaced by its equation ofmotion right from the start as follows
⟨119865⟩ = (120594uarr 119894 119876+ 120590minus120594uarr) (58)
Taking into account the relation 119876+120594uarr
= 0 with 119876+
commuting with 119867ext which means that the intermediatestate must have the same energy as 120594 (58) can be written interms of a complete set of states as
⟨119865⟩ = 119894 (120594uarr 119876+120594darr) (120594darr 120590minus 120594uarr) (59)
According to (55) we have
120576 = ⟨119867ext⟩ = (120594uarr 119867ext120594uarr) =1
2(120594
uarr 119876
+120594darr) (120594
darr 119876
minus120594uarr)
= 120576119902minus 120576
119901= ⟨119867
119902⟩ minus ⟨119867
119901⟩ = (120595
uarr 119867
119902120595uarr) minus (120601
uarr 119867
119901120601uarr)
=1
2(120595
uarr 119876
119902+120595darr) (120595
darr 119876
119902minus120595uarr)
minus1
2(120601
uarr 119876
119901+120601darr) (120601
darr 119876
119901minus120601uarr)
(60)
where 120594uarrdarr= 120595
uarrdarr120601uarrdarr 120595
uarr= (
1205951
0) 120595
darr= (
0
1205952) 120601
uarr= (
1206011
0) and
120601darr= (
0
1206012) From SUSY algebra it follows immediately that
1
radic120576119876minus120594uarr= 120594
darr=
minus120594uarr
1
radic120576119902
119876119902minus120595uarr= 120595
darr=
minus120595uarr
1
radic120576119901
119876119901minus120601uarr= 120601
darr=
minus120601uarr
(61)
By virtue of (61) (60) reads
radic120576 (120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= radic120576119902 (120595uarr 119876119902+120595darr) (120595darr minus120595uarr)
minus radic120576119901 (120601uarr 119876119901+120601darr) (120601darr minus120601uarr)
(62)
ISRNMathematical Physics 7
Using the matrix representations of119876119902+ 119876
119901+ and
minusand the
wave functions equation (53) one gets [13]
(120595darr
minus120595uarr) = radic
1198821015840(119902+)
120587119890minusΔ119882
Δ119902
(120601darr
minus120601uarr) = radic
1198811015840(119901
+)
120587119890minusΔ119881
Δ119901
(120595uarr 119876
119902+120595darr) = 119894radic
1198821015840(119902minus)
120587119890minusΔ119882
(120601uarr 119876
119901+120601darr) = 119894radic
1198811015840(119901
minus)
120587119890minusΔ119881
(63)
where Δ119902 = 119902+minus 119902
minusand Δ119901 = 119901
+minus 119901
minus Hence
(120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= 2119894radic120576[
[
(
120576119902
120576)radic120576
119902radic119882
1015840(119902minus)
120587Δ119902
minus (
120576119901
120576)radic120576
119901radic1198811015840(119901
minus)
120587Δ119901]
]
(64)
⟨119865⟩ = minus2radic120576 [
[
(
120576119902
120576)radic
1198821015840(119902+)
120587119890minus2Δ119882
Δ119902
minus (
120576119901
120576)radic
1198811015840(119901)
120587119890minus2Δ119881
Δ119901]
]
(65)
Along the actual trajectories in 119902-space (65) reproduces theresults obtained in [13]
5 An Extended SUSY Breaking in theInstanton Picture
In this Section our goal is to show that the expressionsequations (64) and (65) can be obtained in the path integralformulation of the theory by calculating the matrix elementsthat is the effect of tunneling between two classical vacuaby using a one-instanton background That is the matrixelements of
plusmn 119876
119902plusmn and 119876
119901plusmncan be calculated in the
background of the classical solution 119902119888= minus119882
119888and
119888= minus119881
119888
In doing this we rewrite the matrix element equation (62) interms of eigenstates of the conjugate operator
plusmnas follows
radic120576 [⟨+0119902+119901+
1003816100381610038161003816 119890minus119894119867ext(119879minus119905)119876
+119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816
times 119890minus119894119867ext(119879minus119905)
minus119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902+119901+0+⟩]119879rarrminus119894infin
= radic120576119902 [⟨+0119902+1003816100381610038161003816 119890
minus119894119867119902(119879minus119905)119876119902+119890minus119894119867119902(119879+119905) 1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus
1003816100381610038161003816
times 119890minus119894119867119902(119879minus119905)
minus
10038161003816100381610038161003816119890minus119894119867119902(119879+119905)119902
+0+⟩]
119879rarrminus119894infin
minus radic120576119901 [⟨+0119901+1003816100381610038161003816 119890minus119894119867119901(119879minus119905)119876
119901+119890minus119894119867119901(119879+119905)
times1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus
1003816100381610038161003816 minus
10038161003816100381610038161003816119901+0+⟩ ]
119879rarrminus119894infin
(66)
in the limit 119879 rarr minus119894infin This reduces to
radic120576 ⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= radic120576119902 ⟨+0119902+1003816100381610038161003816119876119902+
1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus1003816100381610038161003816 minus
1003816100381610038161003816 119902+0+⟩
minus radic120576119901 ⟨+0119901+1003816100381610038161003816119876119901+
1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus1003816100381610038161003816 minus
1003816100381610038161003816119901+0+⟩
(67)
which in turn can be presented by path integrals definedin terms of anticommuting 119888-number operators 120577 and 120578
with Euclidean actions of the instantons in 119902- and 119901-spacesrespectively Following [13] these functional integrals includean integration over instanton time 120591
0which is due to the
problem of zero modes of the bilinear terms in Euclideanactions This arises from time-transformation of instantonsand SUSY transformations on them respectively The exis-tence of zero modes gives rise to non-Gaussian behaviour ofthe functional integral Due to it the matrix elements abovedo not receive any contributions from either no-instantonor anti-instanton configurations The zero mode problem issolved by introducing a collective coordinate 120591
0replacing the
bosonic zero mode [14] Whereas the functional integralsdepend only on the difference 120591 minus 120591
0 Note also that multi-
instanton configurations could contribute in principle pro-vided they have not more than one normalizable fermioniczero mode But as it was shown in [13] their contribution isclearly smaller with respect to radic2120576119902 and radic2120576119901 In the casewhen the SUSY potentials in 119902- and 119901-spaces have morethan two extrema 119902] and 119901120583 ] 120583 = 1 2 119873 one can putconditions on the SUSY potentials as follows
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr infin at 119902 997888rarr plusmninfin for 120595+
0
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr minusinfin at 119902 997888rarr plusmninfin for 120595minus
0
(68)
and similar to 119881(119901) that the extrema are well separated asfollows int119902]+1
119902]
119882(1199021015840)119889119902
1015840≫ 1 int119902120583+1
119901120583
119881(1199011015840)119889119901
1015840≫ 1 Around
each of the classical minima 119902] and119901120583 of the potentials1198822(119902)
and 1198812(119901) respectively one can approximate the theory
by a supersymmetric harmonic oscillator Then there are119873 ground states which have zero energy These states aredescribed by upper or lower component of the wave functiondepending on whether ] and 120583 are odd or even With thisprovision the functional integrals are calculated in [13] whichallow us consequently to write
⟨+0119902+
1003816100381610038161003816119876119902+1003816100381610038161003816 119902minus0minus⟩ = 119894
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888
⟨minus0119902minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+0+⟩ =
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888Δ119902
119888
(69)
8 ISRNMathematical Physics
and so forth Inserting this in (67) we arrive at (64)
⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= 2119894radic120576[
[
(
120576119902
120576)radic120576119902
radic119882
1015840
119888(119902+)
120587Δ119902
119888
minus (
120576119901
120576)radic120576119901
radic1198811015840
119888(119901
+)
120587Δ119901
119888]
]
(70)
and thus of (65) as its inevitable corollary This proves thatthe extended SUSY breaking has resulted from tunnelingbetween the classical vacua of the theory The correctionsto this picture are due to higher-order terms and quantum-tunneling effects
6 Spectrum Generating Algebra
An extended Hamiltonian 119867ext equation (27) can be treatedas a set of two ordinary two-dimensional partner Hamiltoni-ans [4] as follows
119867plusmn=1
2[120587
2
119902minus 120587
2
119901+ 119880
plusmn(119902 119901)] (71)
provided by partner potentials
119880plusmn(119902 119901) = 119880
119902plusmn(119902) minus 119880
119901plusmn(119901)
119880119902plusmn(119902) = 119882
2(119902 119886
119902) ∓119882
1015840
119902(119902 119886
119902)
119880119901plusmn(119901) = 119881
2(119901 119886
119901) ∓ 119881
1015840
119901(119901 119886
119901)
(72)
A subset of the SUSY potentials for which the Schrodinger-like equations are exactly solvable share an integrabilityconditions of shape-invariance [15] as follows
119880+(1198860 119902 119901) = 119880
minus(1198861 119902 119901) + 119877 (119886
0) 119886
1= 119891 (119886
0)
(73)
where 1198860and 119886
1are a set of parameters that specify phase-
space-independent properties of the potentials and thereminder 119877(119886
0) is independent of (119902 119901)
61 Algebraic Properties of Shape Invariance Using the stan-dard technique we may construct a series of Hamiltonians119867119873 119873 = 0 1 2
119867119873=1
2[120587
2
119902minus 120587
2
119901+ 119880
minus(119886119873 119902 119901) +
119873
sum
119896=1
119877 (119886119896)] (74)
where 119886119873= 119891
(119873)(119886) (119873 is the number of iterations) From
(72) and (73) we obtain then 119873 = 119899 + 119898 coupled nonlineardifferential equations which are the two recurrence relationsof Riccati-type differential equations as follows
1198822
119899+1(119902) + 119882
1015840
119902(119899+1)(119902) = 119882
2
119899(119902) minus 119882
1015840
119902119899(119902) minus 120583
119899
1198812
119898+1(119901) + 119881
1015840
119901(119898+1)(119901) = 119881
2
119898(119901) minus 119881
1015840
119901119898(119901) minus ]
119898
(75)
where we denote 119882119899(119902) equiv 119882(119902 119886
119902119899) 119881
119898(119901) equiv 119881(119901 119886
119901119898)
120583119899equiv 119877
119902(119886119902119899) and ]
119898equiv 119877
119901(119886119901119898) Here we admit that
for unbroken SUSY the eigenstates of the potentials 119880119902119901
respectively are
119864(minus)
1199020= 0 119864
(minus)
119902119899=
119899minus1
sum
119894=0
120583119894 119864
(minus)
1199010= 0 119864
(minus)
119901119898=
119898minus1
sum
119895=0
]119895
(76)
that is the ground states are at zero energies characteristic ofunbroken supersymmetryThe differential equations (75) canbe investigated to find exactly solvable potentials The shapeinvariance condition equation (73) can be expressed in termsof bosonic operators as
119861+(119909 119886
0) 119861
minus(119909 119886
0) minus 119861
minus(119909 119886
1) 119861
+(119909 119886
1)
= 119877 (1198860) = 120583
0minus ]
0
119861aelig+ (aelig 119886aelig0) 119861aeligminus (aelig 119886aelig0) minus 119861aeligminus (aelig 119886aelig1) 119861aelig+ (aelig 119886aelig1)
= (1205830or ]
0)
(77)
where 119909(119902 119901)- is the coordinate in (119902 119901)-space aelig denotesconcisely either 119902- or 119901-representations (no summation onaelig is assumed) To classify algebras associated with the shapeinvariance following [16] we introduce an auxiliary variables120601(120601
119902 120601119901) and define the following creation and annihilation
operators
119869+= 119890
119894119896120601119861+(119909 120594 (119894120597
120601)) 119869
minus= 119861
minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601
(78)
where 119896(119896119902 119896119901) are an arbitrary real constants and 120594(120594
119902 120594119901)
are an arbitrary real functions Consequently the creationand annihilation operators in (119902 119901)-spaces can be written as
119869aelig+ = 119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig))
119869aeligminus = 119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig
(79)
The operators 119861plusmn(119909 120594(119894120597
120601)) and 119861aeligplusmn(aelig 120594aelig(119894120597120601aelig )) are the
generalization of (77) where 1198860rarr 120594(119894120597
120601) and 119886aelig0 rarr
120594aelig(119894120597120601aelig ) One can easily prove the following relations
119890119894119896120601119861+(119909 120594 (119894120597
120601)) = 119861
+(119909 120594 (119894120597
120601+ 119896)) 119890
119894119896120601
119861minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601= 119890
minus119894119896120601119861minus(119909 120594 (119894120597
120601+ 119896))
(80)
and that
119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig)) = 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119890
119894119896aelig120601aelig
119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig = 119890
minus119894119896aelig120601aelig119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) (81)
If we choose a function 120594(119894120597120601) such that 120594(119894120597
120601+ 119896) =
119891[120594(119894120597120601)] then we have identified 119886
0rarr 120594(119894120597
120601) and
1198861= 119891(119886
0) rarr 119891[120594(119894120597
120601)] = 120594(119894120597
120601+ 119896) Similar relations can
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
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Stochastic AnalysisInternational Journal of
4 ISRNMathematical Physics
operators for the eigenvalues of 1205903which is the diagonal Pauli
matrix The fermionic operator 119891 reads 119891 C2rarr C2
119891 =
(12)[+
minus] which commutes with the119867ext and is diagonal
in this representation with conserved eigenvalues plusmn12 Dueto it the wave functions become two-component objects asfollows
120594 (119902 119901) = (120594+12
(119902 119901)
120594minus12
(119902 119901)) = (
1205941(119902 119901)
1205942(119902 119901)
) = (
1205951(119902) 120601
1(119901)
1205952(119902) 120601
2(119901))
(26)
where the states 12059512(119902) 120601
12(119901) correspond to fermionic
quantum number 119891 = plusmn12 respectively in 119902- and 119901-spacesThey belong to Hilbert space H = H
0otimes C2
= [L2(R) otimes
L2(R)]otimesC2 Hence theHamiltonian119867ext of extended phase
space (119873 = 2)-SUSY quantummechanical system becomes a2 times 2matrix as follows
119867ext = (119867+
0
0 119867minus
) =1
2(
2
119902+119882
2(119902) + 119894119882
1015840
119902(119902) [
1
2])
minus1
2(
2
119901+ 119881
2(119901) + 119894119881
1015840
119902(119901) [
1
2])
(27)
To infer the extendedHamiltonian equation (27) equivalentlyone may start from the 119888-number extended Lagrangian ofextended phase space quantum field theory in (0 + 1)-dimensions in 119902- and 119901-spaces as follows
Lext (119901 119902 119902) = minus 119902119901 minus 119902 +1
2[(119889119902
119889119905)
2
minus1198822(119902)]
+ 1198911198821015840
119902(119902) +
1
2[(119889119901
119889119905)
2
minus 1198812(119901)]
+ 1198911198811015840
119901(119901)
(28)
In dealing with abstract space of eigenstates of the conjugateoperator
plusmnwhich have anticommuting 119888-number eigenval-
ues suppose that |00minus⟩ is the normalized zero-eigenstate of 119902and
minusas follows
119902 |00minus⟩ = 0 minus |00minus⟩ = 0 (29)
The state |00+⟩ is defined by
|00+⟩ = + |00minus⟩ = 0 (30)
then +|00+⟩ = 0
minus|00+⟩ = |00minus⟩ Taking into account
that daggerplusmn=
∓ we get
⟨∓00| plusmn = 0 ⟨∓00| ∓ = ⟨plusmn00| (31)
Now we may introduce the notation 120572 120573 for the anticom-muting eigenvalues of
plusmn Consistency requires
120572plusmn= minus
plusmn120572 120572 |00plusmn⟩ = plusmn |00plusmn⟩ 120572 (32)
The eigenstates of 119902 minuscan be constructed as
1003816100381610038161003816119902120572minus⟩ = 119890minus119894119902119901minus120572+
|00minus⟩ (33)
and thus
1199021003816100381610038161003816119902120572minus⟩ = 119902
1003816100381610038161003816119902120572minus⟩ minus
1003816100381610038161003816119902120572minus⟩ = 1205721003816100381610038161003816119902120572minus⟩ (34)
Then the 119902and
+eigenstates are obtained by Fourier
transformation as follows
1003816100381610038161003816 119902120573+⟩ = minusint119889120572119890120572120573 1003816100381610038161003816 119902120572minus⟩
10038161003816100381610038161003816120587119902120572plusmn⟩ = minusint119889119902119890
119894119902120587119902 1003816100381610038161003816 119902120572plusmn⟩
1003816100381610038161003816119901120573+⟩ = minusint119889120572119890120572120573 1003816100381610038161003816119901120572minus⟩
10038161003816100381610038161003816120587119901120572plusmn⟩ = minusint119889119901119890
119894119901120587119901 1003816100381610038161003816119901120572plusmn⟩
(35)
which gives
119902
10038161003816100381610038161003816120587119902120572plusmn⟩ = 120587
119902
10038161003816100381610038161003816120587119902120572plusmn⟩
+
10038161003816100381610038161003816(119902 120587
119902) 120573+⟩ = 120573
10038161003816100381610038161003816(119902 120587
119902) 120573+⟩
119901
10038161003816100381610038161003816120587119901120572plusmn⟩ = 120587
119901
10038161003816100381610038161003816120587119901120572plusmn⟩
+
10038161003816100381610038161003816(119901 120587
119901) 120573+⟩ = 120573
10038161003816100381610038161003816(119901 120587
119901) 120573+⟩
(36)
The following completeness relations hold
minus int1198891205721198891199021003816100381610038161003816 119902120572plusmn⟩⟨∓120572
lowast1199021003816100381610038161003816 = 1
minus int119889120572
119889120587119902
2120587
10038161003816100381610038161003816120587119902120572plusmn⟩⟨∓120572
lowast120587119902
10038161003816100381610038161003816= 1
minus int1198891205721198891199011003816100381610038161003816119901120572plusmn⟩⟨∓120572
lowast1199011003816100381610038161003816 = 1
minus int119889120572
119889120587119901
2120587
10038161003816100381610038161003816120587119901120572plusmn⟩⟨∓120572
lowast120587119901
10038161003816100381610038161003816= 1
(37)
The time evolution of the state |119905⟩ is now given as follows
120594minus(119902120572119901120573119905) = minusint119889120572
1015840119889119902
1015840119889120573
1015840119889119901
1015840119870(119902120572119901120573119905 | 119902
10158401205721015840119901101584012057310158401199051015840)
(38)
The kernel reads
119870(119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840)
= ⟨+119902120572lowast119901120573
lowast1003816100381610038161003816 119890minus119894119867ext(119905minus119905
1015840) 100381610038161003816100381610038161199021015840120572101584011990110158401205731015840⟩
(39)
which can be evaluated by the path integral Actually analternative approach to describe the state space and dynamicsof the extended phase space quantum system is by the pathintegral [3] which reads
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) = ⟨119902119901119891
1003816100381610038161003816 119890minus119894119867ext(119905minus119905
1015840) 10038161003816100381610038161003816119902101584011990110158401198911015840⟩ (40)
In the path integral equation (40) the individual states arecharacterized by the energy and the fermionic quantum
ISRNMathematical Physics 5
number 119891 With the Hamiltonian 119867ext the path integralequation (40) is diagonal as follows
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840)
=K1198911198911015840 (119902119905 | 119902
10158401199051015840)K
1198911198911015840 (119901119905 | 119901
10158401199051015840)
= 1205751198911198911015840 int
119902
1199021015840
D119902int119901
1199011015840
D119901 exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(41)
Knowing the path integral equation (41) it is sufficient tospecify the initial wave function 120594
119891(1199021015840 119901
1015840 1199051015840) to obtain all
possible information about the system at any later time 119905 by
120594119891(119902 119901 119905) = sum
1198911015840
int1198891199021015840119889119901
1015840K
1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) 120594
1198911015840 (119902
1015840 119901
1015840 1199051015840)
(42)
with 120594plusmn12
(119902 119901 119905) = 12059412(119902 119901 119905) (26) In terms of anti-
commuting 119888-number operators 120577 and 120578 defining 120595 =
radic12 (120578+120577
119894(120578minus120577)) the path integral equation (41) becomes
K (119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840) = int
119902120572119901120573
1199021015840120572101584011990110158401205731015840
D119902D119901D120577D120578
times exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(43)
The functional integral is taken over all trajectories from 1199021015840 1205721015840to 119902 120572 and 1199011015840 1205731015840 to 119901 120573 between the times 1199051015840 and 119905
4 Solution of the Extended SchroumldingerEquation with Small Energy Eigenvalue 120576
Adopting the technique developed in [13] first we usethe iterative scheme to find the approximate ground statesolutions to the extended Schrodinger-like equation
119867ext120594 (119902 119901) = (119867119902minus 119867
119901) 120594 (119902 119901) = 120576120594 (119902 119901) (44)
with energy 120576Wewill then use these solutions to calculate theparameters which measure the breaking of extended SUSYsuch as the ground state energy The approximation whichwent into the derivation of solutions of (44) meets ourinterest that the ground state energy 120576 is supposedly smallAs we mentioned above the solutions for nonzero 120576 come inpairs of the form
120594uarr(119902 119901) = (
1205941(119902 119901)
0) or 120594
darr(119902 119901) = (
0
1205942(119902 119901)
)
(45)
related by supersymmetry where 12059412(119902 119901) = 120595
12(119902)120601
12(119901)
The state space of the system is defined by all the normalizablesolutions of (44) and the individual states are characterizedby the energies 120576
119902and the fermionic quantumnumber119891 One
of these solutions is acceptable only if119882(119902) and119881(119901) becomeinfinite at both 119902 rarr plusmninfin and 119901 rarr plusmninfin respectivelywith the same sign If this condition is not satisfied neitherof the solutions is normalizable nor they can represent theground state of the system Equation (44) yields the followingrelations between energy eigenstates with fermionic quantumnumber plusmn12
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205952 (119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206012 (119901)
(46)
[(minus120597
120597119902+119882
119902(119902)) minus (minus
120597
120597119901+ 119881
119901(119901))]120595
2(119902) 120601
2(119901)
= radic21205761199021205951 (119902) 1206012 (119901) minus radic2120576119901 1205952 (119902) 1206011 (119901)
(47)
where 120576 = 120576119902minus120576
119901and 120576
119902and 120576
119901are the eigenvalues of119867
119902and
119867119901 respectively The technique now is to devise an iterative
approximation scheme to solve (46) and (47) by taking atrial wave function for 120594
2(119902 119901) substitute this into the first
equation (46) and integrate it to obtain an approximationfor 120594
1(119902 119901) This can be used as an ansatz in the second
equation (47) to find an improved solution for 1205942(119902 119901) and
so forth As it was shown in [13] the procedure converges forwell-behaved potentials with a judicious choice of initial trialfunction If the119882
119902and 119881
119901are odd then
1205951(minus119902) = 120595
2(119902) 120601
1(minus119901) = 120601
2(119901) (48)
since they satisfy the same eigenvalue equation It is straight-forward then for example to obtain
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205951 (minus119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206011 (minus119901)
(49)
The independent nature of 119902 and119901 gives the freedomof taking119902 = 0 119901 = 0 which yield an expression for energies asfollows
radic2120576119902 = 119882(0) +1205951015840
1(0)
1205951 (0)
radic2120576119901 = 119881 (0) +1206011015840
1(0)
1206011 (0)
(50)
Suppose that the potentials 119882119902(119902) and 119881
119901(119901) have a maxi-
mum at 119902minusand 119901
minus and minimum at 119902
+and 119901
+ respectively
For the simplicity sake we choose the trial wave functions as
120595(0)
12(119902) = 120575 (119902 minus 119902
plusmn) 120601
(0)
12(119901) = 120575 (119901 minus 119901
plusmn) (51)
6 ISRNMathematical Physics
After one iteration we obtain
120594(1)
1(119902 119901) =
1
119873119902119873119901
120579 (119902 minus 119902minus) 120579 (119901 minus 119901
minus)
times 119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
120594(1)
2(119902 119901) =
1
119873119902119873119901
120579 (119902+minus 119902) 120579 (119901
+minus 119901)
times 119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
(52)
where 119873119902and 119873
119901are the normalization factors The next
approximation leads to
120594(2)
1(119902 119901) =
1
1198731015840119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
times int
infin
max(minus119902119902minus)119890minus2int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
infin
max(minus119901119901minus)1198902 int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
120594(2)
2(119902 119901) =
1
1198731015840119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
times int
min(minus119902119902+)
infin
1198902 int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
min(minus119901119901+)
infin
119890minus2int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
(53)
It can be easily verified that to this level of precision (52) isself-consistent solution Actually for example for 1199021015840 gt 119902
minusthe
exponential 119890minus2int1199021015840
0119882(11990210158401015840)11988911990210158401015840
will peak sharply around 119902+and
may be approximated by a 120575-function 119888120575(119902+minus 119902
1015840) similarly
1198902 int1199021015840
0119882(11990210158401015840)11988911990210158401015840
may be replaced approximately by 119888120575(119902minusminus 119902
1015840)
for 1199021015840 lt 119902+ The same arguments hold for the 119901-space
With these approximations equations (53) reduce to (52)Thenormalization constant1198731015840 is
1198731015840= (int
infin
119902minus
119889119902119890minus2int119902
0119882(1199021015840)1198891199021015840
int
infin
119901minus
119889119901119890minus2 int1199011015840
0119881(1199011015840)1198891199011015840
)
32
(54)
The energy expectation value
120576 = (1205941 119867ext1205941) (55)
gives the same result as that obtained for odd potentialsby means of (50) and (53) Assuming the exponentials119890minus2int0
119902minus119882(119902)119889119902 and 119890minus2int
0
119901minus119881(119901)119889119901 to be small which is correct to
the same approximations underlying (55) the difference isnegligible and the integrals in both cases may be replacedby Gaussians around 119902
+and 119901
+ respectively Hence it is
straightforward to obtain
120576 =ℎ119882
1015840(119902+)
2120587119890minus2Δ119882ℎ
minusℎ119881
1015840(119901
+)
2120587119890minus2Δ119881ℎ
(56)
which gives direct evidence for the SUSY breaking in theextended phase space quantum mechanical system Here wehave reinstated ℎ to show the order of adopted approxima-tion and its non-perturbative nature We also denoted
Δ119882 = int
119902minus
119902+
119882(119902) 119889119902 Δ119881 = int
119901minus
119901+
119881 (119901) 119889119901 (57)
However a more practical measure for the SUSY breakingin particular in field theories is the expectation value ofan auxiliary field which can be replaced by its equation ofmotion right from the start as follows
⟨119865⟩ = (120594uarr 119894 119876+ 120590minus120594uarr) (58)
Taking into account the relation 119876+120594uarr
= 0 with 119876+
commuting with 119867ext which means that the intermediatestate must have the same energy as 120594 (58) can be written interms of a complete set of states as
⟨119865⟩ = 119894 (120594uarr 119876+120594darr) (120594darr 120590minus 120594uarr) (59)
According to (55) we have
120576 = ⟨119867ext⟩ = (120594uarr 119867ext120594uarr) =1
2(120594
uarr 119876
+120594darr) (120594
darr 119876
minus120594uarr)
= 120576119902minus 120576
119901= ⟨119867
119902⟩ minus ⟨119867
119901⟩ = (120595
uarr 119867
119902120595uarr) minus (120601
uarr 119867
119901120601uarr)
=1
2(120595
uarr 119876
119902+120595darr) (120595
darr 119876
119902minus120595uarr)
minus1
2(120601
uarr 119876
119901+120601darr) (120601
darr 119876
119901minus120601uarr)
(60)
where 120594uarrdarr= 120595
uarrdarr120601uarrdarr 120595
uarr= (
1205951
0) 120595
darr= (
0
1205952) 120601
uarr= (
1206011
0) and
120601darr= (
0
1206012) From SUSY algebra it follows immediately that
1
radic120576119876minus120594uarr= 120594
darr=
minus120594uarr
1
radic120576119902
119876119902minus120595uarr= 120595
darr=
minus120595uarr
1
radic120576119901
119876119901minus120601uarr= 120601
darr=
minus120601uarr
(61)
By virtue of (61) (60) reads
radic120576 (120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= radic120576119902 (120595uarr 119876119902+120595darr) (120595darr minus120595uarr)
minus radic120576119901 (120601uarr 119876119901+120601darr) (120601darr minus120601uarr)
(62)
ISRNMathematical Physics 7
Using the matrix representations of119876119902+ 119876
119901+ and
minusand the
wave functions equation (53) one gets [13]
(120595darr
minus120595uarr) = radic
1198821015840(119902+)
120587119890minusΔ119882
Δ119902
(120601darr
minus120601uarr) = radic
1198811015840(119901
+)
120587119890minusΔ119881
Δ119901
(120595uarr 119876
119902+120595darr) = 119894radic
1198821015840(119902minus)
120587119890minusΔ119882
(120601uarr 119876
119901+120601darr) = 119894radic
1198811015840(119901
minus)
120587119890minusΔ119881
(63)
where Δ119902 = 119902+minus 119902
minusand Δ119901 = 119901
+minus 119901
minus Hence
(120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= 2119894radic120576[
[
(
120576119902
120576)radic120576
119902radic119882
1015840(119902minus)
120587Δ119902
minus (
120576119901
120576)radic120576
119901radic1198811015840(119901
minus)
120587Δ119901]
]
(64)
⟨119865⟩ = minus2radic120576 [
[
(
120576119902
120576)radic
1198821015840(119902+)
120587119890minus2Δ119882
Δ119902
minus (
120576119901
120576)radic
1198811015840(119901)
120587119890minus2Δ119881
Δ119901]
]
(65)
Along the actual trajectories in 119902-space (65) reproduces theresults obtained in [13]
5 An Extended SUSY Breaking in theInstanton Picture
In this Section our goal is to show that the expressionsequations (64) and (65) can be obtained in the path integralformulation of the theory by calculating the matrix elementsthat is the effect of tunneling between two classical vacuaby using a one-instanton background That is the matrixelements of
plusmn 119876
119902plusmn and 119876
119901plusmncan be calculated in the
background of the classical solution 119902119888= minus119882
119888and
119888= minus119881
119888
In doing this we rewrite the matrix element equation (62) interms of eigenstates of the conjugate operator
plusmnas follows
radic120576 [⟨+0119902+119901+
1003816100381610038161003816 119890minus119894119867ext(119879minus119905)119876
+119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816
times 119890minus119894119867ext(119879minus119905)
minus119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902+119901+0+⟩]119879rarrminus119894infin
= radic120576119902 [⟨+0119902+1003816100381610038161003816 119890
minus119894119867119902(119879minus119905)119876119902+119890minus119894119867119902(119879+119905) 1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus
1003816100381610038161003816
times 119890minus119894119867119902(119879minus119905)
minus
10038161003816100381610038161003816119890minus119894119867119902(119879+119905)119902
+0+⟩]
119879rarrminus119894infin
minus radic120576119901 [⟨+0119901+1003816100381610038161003816 119890minus119894119867119901(119879minus119905)119876
119901+119890minus119894119867119901(119879+119905)
times1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus
1003816100381610038161003816 minus
10038161003816100381610038161003816119901+0+⟩ ]
119879rarrminus119894infin
(66)
in the limit 119879 rarr minus119894infin This reduces to
radic120576 ⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= radic120576119902 ⟨+0119902+1003816100381610038161003816119876119902+
1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus1003816100381610038161003816 minus
1003816100381610038161003816 119902+0+⟩
minus radic120576119901 ⟨+0119901+1003816100381610038161003816119876119901+
1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus1003816100381610038161003816 minus
1003816100381610038161003816119901+0+⟩
(67)
which in turn can be presented by path integrals definedin terms of anticommuting 119888-number operators 120577 and 120578
with Euclidean actions of the instantons in 119902- and 119901-spacesrespectively Following [13] these functional integrals includean integration over instanton time 120591
0which is due to the
problem of zero modes of the bilinear terms in Euclideanactions This arises from time-transformation of instantonsand SUSY transformations on them respectively The exis-tence of zero modes gives rise to non-Gaussian behaviour ofthe functional integral Due to it the matrix elements abovedo not receive any contributions from either no-instantonor anti-instanton configurations The zero mode problem issolved by introducing a collective coordinate 120591
0replacing the
bosonic zero mode [14] Whereas the functional integralsdepend only on the difference 120591 minus 120591
0 Note also that multi-
instanton configurations could contribute in principle pro-vided they have not more than one normalizable fermioniczero mode But as it was shown in [13] their contribution isclearly smaller with respect to radic2120576119902 and radic2120576119901 In the casewhen the SUSY potentials in 119902- and 119901-spaces have morethan two extrema 119902] and 119901120583 ] 120583 = 1 2 119873 one can putconditions on the SUSY potentials as follows
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr infin at 119902 997888rarr plusmninfin for 120595+
0
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr minusinfin at 119902 997888rarr plusmninfin for 120595minus
0
(68)
and similar to 119881(119901) that the extrema are well separated asfollows int119902]+1
119902]
119882(1199021015840)119889119902
1015840≫ 1 int119902120583+1
119901120583
119881(1199011015840)119889119901
1015840≫ 1 Around
each of the classical minima 119902] and119901120583 of the potentials1198822(119902)
and 1198812(119901) respectively one can approximate the theory
by a supersymmetric harmonic oscillator Then there are119873 ground states which have zero energy These states aredescribed by upper or lower component of the wave functiondepending on whether ] and 120583 are odd or even With thisprovision the functional integrals are calculated in [13] whichallow us consequently to write
⟨+0119902+
1003816100381610038161003816119876119902+1003816100381610038161003816 119902minus0minus⟩ = 119894
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888
⟨minus0119902minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+0+⟩ =
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888Δ119902
119888
(69)
8 ISRNMathematical Physics
and so forth Inserting this in (67) we arrive at (64)
⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= 2119894radic120576[
[
(
120576119902
120576)radic120576119902
radic119882
1015840
119888(119902+)
120587Δ119902
119888
minus (
120576119901
120576)radic120576119901
radic1198811015840
119888(119901
+)
120587Δ119901
119888]
]
(70)
and thus of (65) as its inevitable corollary This proves thatthe extended SUSY breaking has resulted from tunnelingbetween the classical vacua of the theory The correctionsto this picture are due to higher-order terms and quantum-tunneling effects
6 Spectrum Generating Algebra
An extended Hamiltonian 119867ext equation (27) can be treatedas a set of two ordinary two-dimensional partner Hamiltoni-ans [4] as follows
119867plusmn=1
2[120587
2
119902minus 120587
2
119901+ 119880
plusmn(119902 119901)] (71)
provided by partner potentials
119880plusmn(119902 119901) = 119880
119902plusmn(119902) minus 119880
119901plusmn(119901)
119880119902plusmn(119902) = 119882
2(119902 119886
119902) ∓119882
1015840
119902(119902 119886
119902)
119880119901plusmn(119901) = 119881
2(119901 119886
119901) ∓ 119881
1015840
119901(119901 119886
119901)
(72)
A subset of the SUSY potentials for which the Schrodinger-like equations are exactly solvable share an integrabilityconditions of shape-invariance [15] as follows
119880+(1198860 119902 119901) = 119880
minus(1198861 119902 119901) + 119877 (119886
0) 119886
1= 119891 (119886
0)
(73)
where 1198860and 119886
1are a set of parameters that specify phase-
space-independent properties of the potentials and thereminder 119877(119886
0) is independent of (119902 119901)
61 Algebraic Properties of Shape Invariance Using the stan-dard technique we may construct a series of Hamiltonians119867119873 119873 = 0 1 2
119867119873=1
2[120587
2
119902minus 120587
2
119901+ 119880
minus(119886119873 119902 119901) +
119873
sum
119896=1
119877 (119886119896)] (74)
where 119886119873= 119891
(119873)(119886) (119873 is the number of iterations) From
(72) and (73) we obtain then 119873 = 119899 + 119898 coupled nonlineardifferential equations which are the two recurrence relationsof Riccati-type differential equations as follows
1198822
119899+1(119902) + 119882
1015840
119902(119899+1)(119902) = 119882
2
119899(119902) minus 119882
1015840
119902119899(119902) minus 120583
119899
1198812
119898+1(119901) + 119881
1015840
119901(119898+1)(119901) = 119881
2
119898(119901) minus 119881
1015840
119901119898(119901) minus ]
119898
(75)
where we denote 119882119899(119902) equiv 119882(119902 119886
119902119899) 119881
119898(119901) equiv 119881(119901 119886
119901119898)
120583119899equiv 119877
119902(119886119902119899) and ]
119898equiv 119877
119901(119886119901119898) Here we admit that
for unbroken SUSY the eigenstates of the potentials 119880119902119901
respectively are
119864(minus)
1199020= 0 119864
(minus)
119902119899=
119899minus1
sum
119894=0
120583119894 119864
(minus)
1199010= 0 119864
(minus)
119901119898=
119898minus1
sum
119895=0
]119895
(76)
that is the ground states are at zero energies characteristic ofunbroken supersymmetryThe differential equations (75) canbe investigated to find exactly solvable potentials The shapeinvariance condition equation (73) can be expressed in termsof bosonic operators as
119861+(119909 119886
0) 119861
minus(119909 119886
0) minus 119861
minus(119909 119886
1) 119861
+(119909 119886
1)
= 119877 (1198860) = 120583
0minus ]
0
119861aelig+ (aelig 119886aelig0) 119861aeligminus (aelig 119886aelig0) minus 119861aeligminus (aelig 119886aelig1) 119861aelig+ (aelig 119886aelig1)
= (1205830or ]
0)
(77)
where 119909(119902 119901)- is the coordinate in (119902 119901)-space aelig denotesconcisely either 119902- or 119901-representations (no summation onaelig is assumed) To classify algebras associated with the shapeinvariance following [16] we introduce an auxiliary variables120601(120601
119902 120601119901) and define the following creation and annihilation
operators
119869+= 119890
119894119896120601119861+(119909 120594 (119894120597
120601)) 119869
minus= 119861
minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601
(78)
where 119896(119896119902 119896119901) are an arbitrary real constants and 120594(120594
119902 120594119901)
are an arbitrary real functions Consequently the creationand annihilation operators in (119902 119901)-spaces can be written as
119869aelig+ = 119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig))
119869aeligminus = 119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig
(79)
The operators 119861plusmn(119909 120594(119894120597
120601)) and 119861aeligplusmn(aelig 120594aelig(119894120597120601aelig )) are the
generalization of (77) where 1198860rarr 120594(119894120597
120601) and 119886aelig0 rarr
120594aelig(119894120597120601aelig ) One can easily prove the following relations
119890119894119896120601119861+(119909 120594 (119894120597
120601)) = 119861
+(119909 120594 (119894120597
120601+ 119896)) 119890
119894119896120601
119861minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601= 119890
minus119894119896120601119861minus(119909 120594 (119894120597
120601+ 119896))
(80)
and that
119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig)) = 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119890
119894119896aelig120601aelig
119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig = 119890
minus119894119896aelig120601aelig119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) (81)
If we choose a function 120594(119894120597120601) such that 120594(119894120597
120601+ 119896) =
119891[120594(119894120597120601)] then we have identified 119886
0rarr 120594(119894120597
120601) and
1198861= 119891(119886
0) rarr 119891[120594(119894120597
120601)] = 120594(119894120597
120601+ 119896) Similar relations can
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
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Volume 2014 Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Stochastic AnalysisInternational Journal of
ISRNMathematical Physics 5
number 119891 With the Hamiltonian 119867ext the path integralequation (40) is diagonal as follows
K1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840)
=K1198911198911015840 (119902119905 | 119902
10158401199051015840)K
1198911198911015840 (119901119905 | 119901
10158401199051015840)
= 1205751198911198911015840 int
119902
1199021015840
D119902int119901
1199011015840
D119901 exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(41)
Knowing the path integral equation (41) it is sufficient tospecify the initial wave function 120594
119891(1199021015840 119901
1015840 1199051015840) to obtain all
possible information about the system at any later time 119905 by
120594119891(119902 119901 119905) = sum
1198911015840
int1198891199021015840119889119901
1015840K
1198911198911015840 (119902119901119905 | 119902
101584011990110158401199051015840) 120594
1198911015840 (119902
1015840 119901
1015840 1199051015840)
(42)
with 120594plusmn12
(119902 119901 119905) = 12059412(119902 119901 119905) (26) In terms of anti-
commuting 119888-number operators 120577 and 120578 defining 120595 =
radic12 (120578+120577
119894(120578minus120577)) the path integral equation (41) becomes
K (119902120572119901120573119905 | 11990210158401205721015840119901101584012057310158401199051015840) = int
119902120572119901120573
1199021015840120572101584011990110158401205731015840
D119902D119901D120577D120578
times exp(119894int119905
1199051015840
Lext (119901 119902 119902) 119889119905)
(43)
The functional integral is taken over all trajectories from 1199021015840 1205721015840to 119902 120572 and 1199011015840 1205731015840 to 119901 120573 between the times 1199051015840 and 119905
4 Solution of the Extended SchroumldingerEquation with Small Energy Eigenvalue 120576
Adopting the technique developed in [13] first we usethe iterative scheme to find the approximate ground statesolutions to the extended Schrodinger-like equation
119867ext120594 (119902 119901) = (119867119902minus 119867
119901) 120594 (119902 119901) = 120576120594 (119902 119901) (44)
with energy 120576Wewill then use these solutions to calculate theparameters which measure the breaking of extended SUSYsuch as the ground state energy The approximation whichwent into the derivation of solutions of (44) meets ourinterest that the ground state energy 120576 is supposedly smallAs we mentioned above the solutions for nonzero 120576 come inpairs of the form
120594uarr(119902 119901) = (
1205941(119902 119901)
0) or 120594
darr(119902 119901) = (
0
1205942(119902 119901)
)
(45)
related by supersymmetry where 12059412(119902 119901) = 120595
12(119902)120601
12(119901)
The state space of the system is defined by all the normalizablesolutions of (44) and the individual states are characterizedby the energies 120576
119902and the fermionic quantumnumber119891 One
of these solutions is acceptable only if119882(119902) and119881(119901) becomeinfinite at both 119902 rarr plusmninfin and 119901 rarr plusmninfin respectivelywith the same sign If this condition is not satisfied neitherof the solutions is normalizable nor they can represent theground state of the system Equation (44) yields the followingrelations between energy eigenstates with fermionic quantumnumber plusmn12
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205952 (119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206012 (119901)
(46)
[(minus120597
120597119902+119882
119902(119902)) minus (minus
120597
120597119901+ 119881
119901(119901))]120595
2(119902) 120601
2(119901)
= radic21205761199021205951 (119902) 1206012 (119901) minus radic2120576119901 1205952 (119902) 1206011 (119901)
(47)
where 120576 = 120576119902minus120576
119901and 120576
119902and 120576
119901are the eigenvalues of119867
119902and
119867119901 respectively The technique now is to devise an iterative
approximation scheme to solve (46) and (47) by taking atrial wave function for 120594
2(119902 119901) substitute this into the first
equation (46) and integrate it to obtain an approximationfor 120594
1(119902 119901) This can be used as an ansatz in the second
equation (47) to find an improved solution for 1205942(119902 119901) and
so forth As it was shown in [13] the procedure converges forwell-behaved potentials with a judicious choice of initial trialfunction If the119882
119902and 119881
119901are odd then
1205951(minus119902) = 120595
2(119902) 120601
1(minus119901) = 120601
2(119901) (48)
since they satisfy the same eigenvalue equation It is straight-forward then for example to obtain
[(120597
120597119902+119882
119902(119902)) minus (
120597
120597119901+ 119881
119901(119901))]120595
1(119902) 120601
1(119901)
= radic21205761199021205951 (minus119902) 1206011 (119901) minus radic21205761199011205951 (119902) 1206011 (minus119901)
(49)
The independent nature of 119902 and119901 gives the freedomof taking119902 = 0 119901 = 0 which yield an expression for energies asfollows
radic2120576119902 = 119882(0) +1205951015840
1(0)
1205951 (0)
radic2120576119901 = 119881 (0) +1206011015840
1(0)
1206011 (0)
(50)
Suppose that the potentials 119882119902(119902) and 119881
119901(119901) have a maxi-
mum at 119902minusand 119901
minus and minimum at 119902
+and 119901
+ respectively
For the simplicity sake we choose the trial wave functions as
120595(0)
12(119902) = 120575 (119902 minus 119902
plusmn) 120601
(0)
12(119901) = 120575 (119901 minus 119901
plusmn) (51)
6 ISRNMathematical Physics
After one iteration we obtain
120594(1)
1(119902 119901) =
1
119873119902119873119901
120579 (119902 minus 119902minus) 120579 (119901 minus 119901
minus)
times 119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
120594(1)
2(119902 119901) =
1
119873119902119873119901
120579 (119902+minus 119902) 120579 (119901
+minus 119901)
times 119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
(52)
where 119873119902and 119873
119901are the normalization factors The next
approximation leads to
120594(2)
1(119902 119901) =
1
1198731015840119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
times int
infin
max(minus119902119902minus)119890minus2int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
infin
max(minus119901119901minus)1198902 int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
120594(2)
2(119902 119901) =
1
1198731015840119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
times int
min(minus119902119902+)
infin
1198902 int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
min(minus119901119901+)
infin
119890minus2int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
(53)
It can be easily verified that to this level of precision (52) isself-consistent solution Actually for example for 1199021015840 gt 119902
minusthe
exponential 119890minus2int1199021015840
0119882(11990210158401015840)11988911990210158401015840
will peak sharply around 119902+and
may be approximated by a 120575-function 119888120575(119902+minus 119902
1015840) similarly
1198902 int1199021015840
0119882(11990210158401015840)11988911990210158401015840
may be replaced approximately by 119888120575(119902minusminus 119902
1015840)
for 1199021015840 lt 119902+ The same arguments hold for the 119901-space
With these approximations equations (53) reduce to (52)Thenormalization constant1198731015840 is
1198731015840= (int
infin
119902minus
119889119902119890minus2int119902
0119882(1199021015840)1198891199021015840
int
infin
119901minus
119889119901119890minus2 int1199011015840
0119881(1199011015840)1198891199011015840
)
32
(54)
The energy expectation value
120576 = (1205941 119867ext1205941) (55)
gives the same result as that obtained for odd potentialsby means of (50) and (53) Assuming the exponentials119890minus2int0
119902minus119882(119902)119889119902 and 119890minus2int
0
119901minus119881(119901)119889119901 to be small which is correct to
the same approximations underlying (55) the difference isnegligible and the integrals in both cases may be replacedby Gaussians around 119902
+and 119901
+ respectively Hence it is
straightforward to obtain
120576 =ℎ119882
1015840(119902+)
2120587119890minus2Δ119882ℎ
minusℎ119881
1015840(119901
+)
2120587119890minus2Δ119881ℎ
(56)
which gives direct evidence for the SUSY breaking in theextended phase space quantum mechanical system Here wehave reinstated ℎ to show the order of adopted approxima-tion and its non-perturbative nature We also denoted
Δ119882 = int
119902minus
119902+
119882(119902) 119889119902 Δ119881 = int
119901minus
119901+
119881 (119901) 119889119901 (57)
However a more practical measure for the SUSY breakingin particular in field theories is the expectation value ofan auxiliary field which can be replaced by its equation ofmotion right from the start as follows
⟨119865⟩ = (120594uarr 119894 119876+ 120590minus120594uarr) (58)
Taking into account the relation 119876+120594uarr
= 0 with 119876+
commuting with 119867ext which means that the intermediatestate must have the same energy as 120594 (58) can be written interms of a complete set of states as
⟨119865⟩ = 119894 (120594uarr 119876+120594darr) (120594darr 120590minus 120594uarr) (59)
According to (55) we have
120576 = ⟨119867ext⟩ = (120594uarr 119867ext120594uarr) =1
2(120594
uarr 119876
+120594darr) (120594
darr 119876
minus120594uarr)
= 120576119902minus 120576
119901= ⟨119867
119902⟩ minus ⟨119867
119901⟩ = (120595
uarr 119867
119902120595uarr) minus (120601
uarr 119867
119901120601uarr)
=1
2(120595
uarr 119876
119902+120595darr) (120595
darr 119876
119902minus120595uarr)
minus1
2(120601
uarr 119876
119901+120601darr) (120601
darr 119876
119901minus120601uarr)
(60)
where 120594uarrdarr= 120595
uarrdarr120601uarrdarr 120595
uarr= (
1205951
0) 120595
darr= (
0
1205952) 120601
uarr= (
1206011
0) and
120601darr= (
0
1206012) From SUSY algebra it follows immediately that
1
radic120576119876minus120594uarr= 120594
darr=
minus120594uarr
1
radic120576119902
119876119902minus120595uarr= 120595
darr=
minus120595uarr
1
radic120576119901
119876119901minus120601uarr= 120601
darr=
minus120601uarr
(61)
By virtue of (61) (60) reads
radic120576 (120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= radic120576119902 (120595uarr 119876119902+120595darr) (120595darr minus120595uarr)
minus radic120576119901 (120601uarr 119876119901+120601darr) (120601darr minus120601uarr)
(62)
ISRNMathematical Physics 7
Using the matrix representations of119876119902+ 119876
119901+ and
minusand the
wave functions equation (53) one gets [13]
(120595darr
minus120595uarr) = radic
1198821015840(119902+)
120587119890minusΔ119882
Δ119902
(120601darr
minus120601uarr) = radic
1198811015840(119901
+)
120587119890minusΔ119881
Δ119901
(120595uarr 119876
119902+120595darr) = 119894radic
1198821015840(119902minus)
120587119890minusΔ119882
(120601uarr 119876
119901+120601darr) = 119894radic
1198811015840(119901
minus)
120587119890minusΔ119881
(63)
where Δ119902 = 119902+minus 119902
minusand Δ119901 = 119901
+minus 119901
minus Hence
(120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= 2119894radic120576[
[
(
120576119902
120576)radic120576
119902radic119882
1015840(119902minus)
120587Δ119902
minus (
120576119901
120576)radic120576
119901radic1198811015840(119901
minus)
120587Δ119901]
]
(64)
⟨119865⟩ = minus2radic120576 [
[
(
120576119902
120576)radic
1198821015840(119902+)
120587119890minus2Δ119882
Δ119902
minus (
120576119901
120576)radic
1198811015840(119901)
120587119890minus2Δ119881
Δ119901]
]
(65)
Along the actual trajectories in 119902-space (65) reproduces theresults obtained in [13]
5 An Extended SUSY Breaking in theInstanton Picture
In this Section our goal is to show that the expressionsequations (64) and (65) can be obtained in the path integralformulation of the theory by calculating the matrix elementsthat is the effect of tunneling between two classical vacuaby using a one-instanton background That is the matrixelements of
plusmn 119876
119902plusmn and 119876
119901plusmncan be calculated in the
background of the classical solution 119902119888= minus119882
119888and
119888= minus119881
119888
In doing this we rewrite the matrix element equation (62) interms of eigenstates of the conjugate operator
plusmnas follows
radic120576 [⟨+0119902+119901+
1003816100381610038161003816 119890minus119894119867ext(119879minus119905)119876
+119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816
times 119890minus119894119867ext(119879minus119905)
minus119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902+119901+0+⟩]119879rarrminus119894infin
= radic120576119902 [⟨+0119902+1003816100381610038161003816 119890
minus119894119867119902(119879minus119905)119876119902+119890minus119894119867119902(119879+119905) 1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus
1003816100381610038161003816
times 119890minus119894119867119902(119879minus119905)
minus
10038161003816100381610038161003816119890minus119894119867119902(119879+119905)119902
+0+⟩]
119879rarrminus119894infin
minus radic120576119901 [⟨+0119901+1003816100381610038161003816 119890minus119894119867119901(119879minus119905)119876
119901+119890minus119894119867119901(119879+119905)
times1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus
1003816100381610038161003816 minus
10038161003816100381610038161003816119901+0+⟩ ]
119879rarrminus119894infin
(66)
in the limit 119879 rarr minus119894infin This reduces to
radic120576 ⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= radic120576119902 ⟨+0119902+1003816100381610038161003816119876119902+
1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus1003816100381610038161003816 minus
1003816100381610038161003816 119902+0+⟩
minus radic120576119901 ⟨+0119901+1003816100381610038161003816119876119901+
1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus1003816100381610038161003816 minus
1003816100381610038161003816119901+0+⟩
(67)
which in turn can be presented by path integrals definedin terms of anticommuting 119888-number operators 120577 and 120578
with Euclidean actions of the instantons in 119902- and 119901-spacesrespectively Following [13] these functional integrals includean integration over instanton time 120591
0which is due to the
problem of zero modes of the bilinear terms in Euclideanactions This arises from time-transformation of instantonsand SUSY transformations on them respectively The exis-tence of zero modes gives rise to non-Gaussian behaviour ofthe functional integral Due to it the matrix elements abovedo not receive any contributions from either no-instantonor anti-instanton configurations The zero mode problem issolved by introducing a collective coordinate 120591
0replacing the
bosonic zero mode [14] Whereas the functional integralsdepend only on the difference 120591 minus 120591
0 Note also that multi-
instanton configurations could contribute in principle pro-vided they have not more than one normalizable fermioniczero mode But as it was shown in [13] their contribution isclearly smaller with respect to radic2120576119902 and radic2120576119901 In the casewhen the SUSY potentials in 119902- and 119901-spaces have morethan two extrema 119902] and 119901120583 ] 120583 = 1 2 119873 one can putconditions on the SUSY potentials as follows
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr infin at 119902 997888rarr plusmninfin for 120595+
0
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr minusinfin at 119902 997888rarr plusmninfin for 120595minus
0
(68)
and similar to 119881(119901) that the extrema are well separated asfollows int119902]+1
119902]
119882(1199021015840)119889119902
1015840≫ 1 int119902120583+1
119901120583
119881(1199011015840)119889119901
1015840≫ 1 Around
each of the classical minima 119902] and119901120583 of the potentials1198822(119902)
and 1198812(119901) respectively one can approximate the theory
by a supersymmetric harmonic oscillator Then there are119873 ground states which have zero energy These states aredescribed by upper or lower component of the wave functiondepending on whether ] and 120583 are odd or even With thisprovision the functional integrals are calculated in [13] whichallow us consequently to write
⟨+0119902+
1003816100381610038161003816119876119902+1003816100381610038161003816 119902minus0minus⟩ = 119894
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888
⟨minus0119902minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+0+⟩ =
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888Δ119902
119888
(69)
8 ISRNMathematical Physics
and so forth Inserting this in (67) we arrive at (64)
⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= 2119894radic120576[
[
(
120576119902
120576)radic120576119902
radic119882
1015840
119888(119902+)
120587Δ119902
119888
minus (
120576119901
120576)radic120576119901
radic1198811015840
119888(119901
+)
120587Δ119901
119888]
]
(70)
and thus of (65) as its inevitable corollary This proves thatthe extended SUSY breaking has resulted from tunnelingbetween the classical vacua of the theory The correctionsto this picture are due to higher-order terms and quantum-tunneling effects
6 Spectrum Generating Algebra
An extended Hamiltonian 119867ext equation (27) can be treatedas a set of two ordinary two-dimensional partner Hamiltoni-ans [4] as follows
119867plusmn=1
2[120587
2
119902minus 120587
2
119901+ 119880
plusmn(119902 119901)] (71)
provided by partner potentials
119880plusmn(119902 119901) = 119880
119902plusmn(119902) minus 119880
119901plusmn(119901)
119880119902plusmn(119902) = 119882
2(119902 119886
119902) ∓119882
1015840
119902(119902 119886
119902)
119880119901plusmn(119901) = 119881
2(119901 119886
119901) ∓ 119881
1015840
119901(119901 119886
119901)
(72)
A subset of the SUSY potentials for which the Schrodinger-like equations are exactly solvable share an integrabilityconditions of shape-invariance [15] as follows
119880+(1198860 119902 119901) = 119880
minus(1198861 119902 119901) + 119877 (119886
0) 119886
1= 119891 (119886
0)
(73)
where 1198860and 119886
1are a set of parameters that specify phase-
space-independent properties of the potentials and thereminder 119877(119886
0) is independent of (119902 119901)
61 Algebraic Properties of Shape Invariance Using the stan-dard technique we may construct a series of Hamiltonians119867119873 119873 = 0 1 2
119867119873=1
2[120587
2
119902minus 120587
2
119901+ 119880
minus(119886119873 119902 119901) +
119873
sum
119896=1
119877 (119886119896)] (74)
where 119886119873= 119891
(119873)(119886) (119873 is the number of iterations) From
(72) and (73) we obtain then 119873 = 119899 + 119898 coupled nonlineardifferential equations which are the two recurrence relationsof Riccati-type differential equations as follows
1198822
119899+1(119902) + 119882
1015840
119902(119899+1)(119902) = 119882
2
119899(119902) minus 119882
1015840
119902119899(119902) minus 120583
119899
1198812
119898+1(119901) + 119881
1015840
119901(119898+1)(119901) = 119881
2
119898(119901) minus 119881
1015840
119901119898(119901) minus ]
119898
(75)
where we denote 119882119899(119902) equiv 119882(119902 119886
119902119899) 119881
119898(119901) equiv 119881(119901 119886
119901119898)
120583119899equiv 119877
119902(119886119902119899) and ]
119898equiv 119877
119901(119886119901119898) Here we admit that
for unbroken SUSY the eigenstates of the potentials 119880119902119901
respectively are
119864(minus)
1199020= 0 119864
(minus)
119902119899=
119899minus1
sum
119894=0
120583119894 119864
(minus)
1199010= 0 119864
(minus)
119901119898=
119898minus1
sum
119895=0
]119895
(76)
that is the ground states are at zero energies characteristic ofunbroken supersymmetryThe differential equations (75) canbe investigated to find exactly solvable potentials The shapeinvariance condition equation (73) can be expressed in termsof bosonic operators as
119861+(119909 119886
0) 119861
minus(119909 119886
0) minus 119861
minus(119909 119886
1) 119861
+(119909 119886
1)
= 119877 (1198860) = 120583
0minus ]
0
119861aelig+ (aelig 119886aelig0) 119861aeligminus (aelig 119886aelig0) minus 119861aeligminus (aelig 119886aelig1) 119861aelig+ (aelig 119886aelig1)
= (1205830or ]
0)
(77)
where 119909(119902 119901)- is the coordinate in (119902 119901)-space aelig denotesconcisely either 119902- or 119901-representations (no summation onaelig is assumed) To classify algebras associated with the shapeinvariance following [16] we introduce an auxiliary variables120601(120601
119902 120601119901) and define the following creation and annihilation
operators
119869+= 119890
119894119896120601119861+(119909 120594 (119894120597
120601)) 119869
minus= 119861
minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601
(78)
where 119896(119896119902 119896119901) are an arbitrary real constants and 120594(120594
119902 120594119901)
are an arbitrary real functions Consequently the creationand annihilation operators in (119902 119901)-spaces can be written as
119869aelig+ = 119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig))
119869aeligminus = 119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig
(79)
The operators 119861plusmn(119909 120594(119894120597
120601)) and 119861aeligplusmn(aelig 120594aelig(119894120597120601aelig )) are the
generalization of (77) where 1198860rarr 120594(119894120597
120601) and 119886aelig0 rarr
120594aelig(119894120597120601aelig ) One can easily prove the following relations
119890119894119896120601119861+(119909 120594 (119894120597
120601)) = 119861
+(119909 120594 (119894120597
120601+ 119896)) 119890
119894119896120601
119861minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601= 119890
minus119894119896120601119861minus(119909 120594 (119894120597
120601+ 119896))
(80)
and that
119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig)) = 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119890
119894119896aelig120601aelig
119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig = 119890
minus119894119896aelig120601aelig119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) (81)
If we choose a function 120594(119894120597120601) such that 120594(119894120597
120601+ 119896) =
119891[120594(119894120597120601)] then we have identified 119886
0rarr 120594(119894120597
120601) and
1198861= 119891(119886
0) rarr 119891[120594(119894120597
120601)] = 120594(119894120597
120601+ 119896) Similar relations can
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
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6 ISRNMathematical Physics
After one iteration we obtain
120594(1)
1(119902 119901) =
1
119873119902119873119901
120579 (119902 minus 119902minus) 120579 (119901 minus 119901
minus)
times 119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
120594(1)
2(119902 119901) =
1
119873119902119873119901
120579 (119902+minus 119902) 120579 (119901
+minus 119901)
times 119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
(52)
where 119873119902and 119873
119901are the normalization factors The next
approximation leads to
120594(2)
1(119902 119901) =
1
1198731015840119890minusint119902
01198891199021015840119882(1199021015840)+int119901
01198891199011015840119881(1199011015840)
times int
infin
max(minus119902119902minus)119890minus2int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
infin
max(minus119901119901minus)1198902 int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
120594(2)
2(119902 119901) =
1
1198731015840119890int119902
01198891199021015840119882(1199021015840)minusint119901
01198891199011015840119881(1199011015840)
times int
min(minus119902119902+)
infin
1198902 int1199021015840
011988911990210158401015840119882(11990210158401015840)119889119902
1015840
times int
min(minus119901119901+)
infin
119890minus2int1199011015840
011988911990110158401015840119881(11990110158401015840)119889119901
1015840
(53)
It can be easily verified that to this level of precision (52) isself-consistent solution Actually for example for 1199021015840 gt 119902
minusthe
exponential 119890minus2int1199021015840
0119882(11990210158401015840)11988911990210158401015840
will peak sharply around 119902+and
may be approximated by a 120575-function 119888120575(119902+minus 119902
1015840) similarly
1198902 int1199021015840
0119882(11990210158401015840)11988911990210158401015840
may be replaced approximately by 119888120575(119902minusminus 119902
1015840)
for 1199021015840 lt 119902+ The same arguments hold for the 119901-space
With these approximations equations (53) reduce to (52)Thenormalization constant1198731015840 is
1198731015840= (int
infin
119902minus
119889119902119890minus2int119902
0119882(1199021015840)1198891199021015840
int
infin
119901minus
119889119901119890minus2 int1199011015840
0119881(1199011015840)1198891199011015840
)
32
(54)
The energy expectation value
120576 = (1205941 119867ext1205941) (55)
gives the same result as that obtained for odd potentialsby means of (50) and (53) Assuming the exponentials119890minus2int0
119902minus119882(119902)119889119902 and 119890minus2int
0
119901minus119881(119901)119889119901 to be small which is correct to
the same approximations underlying (55) the difference isnegligible and the integrals in both cases may be replacedby Gaussians around 119902
+and 119901
+ respectively Hence it is
straightforward to obtain
120576 =ℎ119882
1015840(119902+)
2120587119890minus2Δ119882ℎ
minusℎ119881
1015840(119901
+)
2120587119890minus2Δ119881ℎ
(56)
which gives direct evidence for the SUSY breaking in theextended phase space quantum mechanical system Here wehave reinstated ℎ to show the order of adopted approxima-tion and its non-perturbative nature We also denoted
Δ119882 = int
119902minus
119902+
119882(119902) 119889119902 Δ119881 = int
119901minus
119901+
119881 (119901) 119889119901 (57)
However a more practical measure for the SUSY breakingin particular in field theories is the expectation value ofan auxiliary field which can be replaced by its equation ofmotion right from the start as follows
⟨119865⟩ = (120594uarr 119894 119876+ 120590minus120594uarr) (58)
Taking into account the relation 119876+120594uarr
= 0 with 119876+
commuting with 119867ext which means that the intermediatestate must have the same energy as 120594 (58) can be written interms of a complete set of states as
⟨119865⟩ = 119894 (120594uarr 119876+120594darr) (120594darr 120590minus 120594uarr) (59)
According to (55) we have
120576 = ⟨119867ext⟩ = (120594uarr 119867ext120594uarr) =1
2(120594
uarr 119876
+120594darr) (120594
darr 119876
minus120594uarr)
= 120576119902minus 120576
119901= ⟨119867
119902⟩ minus ⟨119867
119901⟩ = (120595
uarr 119867
119902120595uarr) minus (120601
uarr 119867
119901120601uarr)
=1
2(120595
uarr 119876
119902+120595darr) (120595
darr 119876
119902minus120595uarr)
minus1
2(120601
uarr 119876
119901+120601darr) (120601
darr 119876
119901minus120601uarr)
(60)
where 120594uarrdarr= 120595
uarrdarr120601uarrdarr 120595
uarr= (
1205951
0) 120595
darr= (
0
1205952) 120601
uarr= (
1206011
0) and
120601darr= (
0
1206012) From SUSY algebra it follows immediately that
1
radic120576119876minus120594uarr= 120594
darr=
minus120594uarr
1
radic120576119902
119876119902minus120595uarr= 120595
darr=
minus120595uarr
1
radic120576119901
119876119901minus120601uarr= 120601
darr=
minus120601uarr
(61)
By virtue of (61) (60) reads
radic120576 (120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= radic120576119902 (120595uarr 119876119902+120595darr) (120595darr minus120595uarr)
minus radic120576119901 (120601uarr 119876119901+120601darr) (120601darr minus120601uarr)
(62)
ISRNMathematical Physics 7
Using the matrix representations of119876119902+ 119876
119901+ and
minusand the
wave functions equation (53) one gets [13]
(120595darr
minus120595uarr) = radic
1198821015840(119902+)
120587119890minusΔ119882
Δ119902
(120601darr
minus120601uarr) = radic
1198811015840(119901
+)
120587119890minusΔ119881
Δ119901
(120595uarr 119876
119902+120595darr) = 119894radic
1198821015840(119902minus)
120587119890minusΔ119882
(120601uarr 119876
119901+120601darr) = 119894radic
1198811015840(119901
minus)
120587119890minusΔ119881
(63)
where Δ119902 = 119902+minus 119902
minusand Δ119901 = 119901
+minus 119901
minus Hence
(120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= 2119894radic120576[
[
(
120576119902
120576)radic120576
119902radic119882
1015840(119902minus)
120587Δ119902
minus (
120576119901
120576)radic120576
119901radic1198811015840(119901
minus)
120587Δ119901]
]
(64)
⟨119865⟩ = minus2radic120576 [
[
(
120576119902
120576)radic
1198821015840(119902+)
120587119890minus2Δ119882
Δ119902
minus (
120576119901
120576)radic
1198811015840(119901)
120587119890minus2Δ119881
Δ119901]
]
(65)
Along the actual trajectories in 119902-space (65) reproduces theresults obtained in [13]
5 An Extended SUSY Breaking in theInstanton Picture
In this Section our goal is to show that the expressionsequations (64) and (65) can be obtained in the path integralformulation of the theory by calculating the matrix elementsthat is the effect of tunneling between two classical vacuaby using a one-instanton background That is the matrixelements of
plusmn 119876
119902plusmn and 119876
119901plusmncan be calculated in the
background of the classical solution 119902119888= minus119882
119888and
119888= minus119881
119888
In doing this we rewrite the matrix element equation (62) interms of eigenstates of the conjugate operator
plusmnas follows
radic120576 [⟨+0119902+119901+
1003816100381610038161003816 119890minus119894119867ext(119879minus119905)119876
+119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816
times 119890minus119894119867ext(119879minus119905)
minus119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902+119901+0+⟩]119879rarrminus119894infin
= radic120576119902 [⟨+0119902+1003816100381610038161003816 119890
minus119894119867119902(119879minus119905)119876119902+119890minus119894119867119902(119879+119905) 1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus
1003816100381610038161003816
times 119890minus119894119867119902(119879minus119905)
minus
10038161003816100381610038161003816119890minus119894119867119902(119879+119905)119902
+0+⟩]
119879rarrminus119894infin
minus radic120576119901 [⟨+0119901+1003816100381610038161003816 119890minus119894119867119901(119879minus119905)119876
119901+119890minus119894119867119901(119879+119905)
times1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus
1003816100381610038161003816 minus
10038161003816100381610038161003816119901+0+⟩ ]
119879rarrminus119894infin
(66)
in the limit 119879 rarr minus119894infin This reduces to
radic120576 ⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= radic120576119902 ⟨+0119902+1003816100381610038161003816119876119902+
1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus1003816100381610038161003816 minus
1003816100381610038161003816 119902+0+⟩
minus radic120576119901 ⟨+0119901+1003816100381610038161003816119876119901+
1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus1003816100381610038161003816 minus
1003816100381610038161003816119901+0+⟩
(67)
which in turn can be presented by path integrals definedin terms of anticommuting 119888-number operators 120577 and 120578
with Euclidean actions of the instantons in 119902- and 119901-spacesrespectively Following [13] these functional integrals includean integration over instanton time 120591
0which is due to the
problem of zero modes of the bilinear terms in Euclideanactions This arises from time-transformation of instantonsand SUSY transformations on them respectively The exis-tence of zero modes gives rise to non-Gaussian behaviour ofthe functional integral Due to it the matrix elements abovedo not receive any contributions from either no-instantonor anti-instanton configurations The zero mode problem issolved by introducing a collective coordinate 120591
0replacing the
bosonic zero mode [14] Whereas the functional integralsdepend only on the difference 120591 minus 120591
0 Note also that multi-
instanton configurations could contribute in principle pro-vided they have not more than one normalizable fermioniczero mode But as it was shown in [13] their contribution isclearly smaller with respect to radic2120576119902 and radic2120576119901 In the casewhen the SUSY potentials in 119902- and 119901-spaces have morethan two extrema 119902] and 119901120583 ] 120583 = 1 2 119873 one can putconditions on the SUSY potentials as follows
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr infin at 119902 997888rarr plusmninfin for 120595+
0
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr minusinfin at 119902 997888rarr plusmninfin for 120595minus
0
(68)
and similar to 119881(119901) that the extrema are well separated asfollows int119902]+1
119902]
119882(1199021015840)119889119902
1015840≫ 1 int119902120583+1
119901120583
119881(1199011015840)119889119901
1015840≫ 1 Around
each of the classical minima 119902] and119901120583 of the potentials1198822(119902)
and 1198812(119901) respectively one can approximate the theory
by a supersymmetric harmonic oscillator Then there are119873 ground states which have zero energy These states aredescribed by upper or lower component of the wave functiondepending on whether ] and 120583 are odd or even With thisprovision the functional integrals are calculated in [13] whichallow us consequently to write
⟨+0119902+
1003816100381610038161003816119876119902+1003816100381610038161003816 119902minus0minus⟩ = 119894
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888
⟨minus0119902minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+0+⟩ =
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888Δ119902
119888
(69)
8 ISRNMathematical Physics
and so forth Inserting this in (67) we arrive at (64)
⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= 2119894radic120576[
[
(
120576119902
120576)radic120576119902
radic119882
1015840
119888(119902+)
120587Δ119902
119888
minus (
120576119901
120576)radic120576119901
radic1198811015840
119888(119901
+)
120587Δ119901
119888]
]
(70)
and thus of (65) as its inevitable corollary This proves thatthe extended SUSY breaking has resulted from tunnelingbetween the classical vacua of the theory The correctionsto this picture are due to higher-order terms and quantum-tunneling effects
6 Spectrum Generating Algebra
An extended Hamiltonian 119867ext equation (27) can be treatedas a set of two ordinary two-dimensional partner Hamiltoni-ans [4] as follows
119867plusmn=1
2[120587
2
119902minus 120587
2
119901+ 119880
plusmn(119902 119901)] (71)
provided by partner potentials
119880plusmn(119902 119901) = 119880
119902plusmn(119902) minus 119880
119901plusmn(119901)
119880119902plusmn(119902) = 119882
2(119902 119886
119902) ∓119882
1015840
119902(119902 119886
119902)
119880119901plusmn(119901) = 119881
2(119901 119886
119901) ∓ 119881
1015840
119901(119901 119886
119901)
(72)
A subset of the SUSY potentials for which the Schrodinger-like equations are exactly solvable share an integrabilityconditions of shape-invariance [15] as follows
119880+(1198860 119902 119901) = 119880
minus(1198861 119902 119901) + 119877 (119886
0) 119886
1= 119891 (119886
0)
(73)
where 1198860and 119886
1are a set of parameters that specify phase-
space-independent properties of the potentials and thereminder 119877(119886
0) is independent of (119902 119901)
61 Algebraic Properties of Shape Invariance Using the stan-dard technique we may construct a series of Hamiltonians119867119873 119873 = 0 1 2
119867119873=1
2[120587
2
119902minus 120587
2
119901+ 119880
minus(119886119873 119902 119901) +
119873
sum
119896=1
119877 (119886119896)] (74)
where 119886119873= 119891
(119873)(119886) (119873 is the number of iterations) From
(72) and (73) we obtain then 119873 = 119899 + 119898 coupled nonlineardifferential equations which are the two recurrence relationsof Riccati-type differential equations as follows
1198822
119899+1(119902) + 119882
1015840
119902(119899+1)(119902) = 119882
2
119899(119902) minus 119882
1015840
119902119899(119902) minus 120583
119899
1198812
119898+1(119901) + 119881
1015840
119901(119898+1)(119901) = 119881
2
119898(119901) minus 119881
1015840
119901119898(119901) minus ]
119898
(75)
where we denote 119882119899(119902) equiv 119882(119902 119886
119902119899) 119881
119898(119901) equiv 119881(119901 119886
119901119898)
120583119899equiv 119877
119902(119886119902119899) and ]
119898equiv 119877
119901(119886119901119898) Here we admit that
for unbroken SUSY the eigenstates of the potentials 119880119902119901
respectively are
119864(minus)
1199020= 0 119864
(minus)
119902119899=
119899minus1
sum
119894=0
120583119894 119864
(minus)
1199010= 0 119864
(minus)
119901119898=
119898minus1
sum
119895=0
]119895
(76)
that is the ground states are at zero energies characteristic ofunbroken supersymmetryThe differential equations (75) canbe investigated to find exactly solvable potentials The shapeinvariance condition equation (73) can be expressed in termsof bosonic operators as
119861+(119909 119886
0) 119861
minus(119909 119886
0) minus 119861
minus(119909 119886
1) 119861
+(119909 119886
1)
= 119877 (1198860) = 120583
0minus ]
0
119861aelig+ (aelig 119886aelig0) 119861aeligminus (aelig 119886aelig0) minus 119861aeligminus (aelig 119886aelig1) 119861aelig+ (aelig 119886aelig1)
= (1205830or ]
0)
(77)
where 119909(119902 119901)- is the coordinate in (119902 119901)-space aelig denotesconcisely either 119902- or 119901-representations (no summation onaelig is assumed) To classify algebras associated with the shapeinvariance following [16] we introduce an auxiliary variables120601(120601
119902 120601119901) and define the following creation and annihilation
operators
119869+= 119890
119894119896120601119861+(119909 120594 (119894120597
120601)) 119869
minus= 119861
minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601
(78)
where 119896(119896119902 119896119901) are an arbitrary real constants and 120594(120594
119902 120594119901)
are an arbitrary real functions Consequently the creationand annihilation operators in (119902 119901)-spaces can be written as
119869aelig+ = 119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig))
119869aeligminus = 119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig
(79)
The operators 119861plusmn(119909 120594(119894120597
120601)) and 119861aeligplusmn(aelig 120594aelig(119894120597120601aelig )) are the
generalization of (77) where 1198860rarr 120594(119894120597
120601) and 119886aelig0 rarr
120594aelig(119894120597120601aelig ) One can easily prove the following relations
119890119894119896120601119861+(119909 120594 (119894120597
120601)) = 119861
+(119909 120594 (119894120597
120601+ 119896)) 119890
119894119896120601
119861minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601= 119890
minus119894119896120601119861minus(119909 120594 (119894120597
120601+ 119896))
(80)
and that
119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig)) = 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119890
119894119896aelig120601aelig
119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig = 119890
minus119894119896aelig120601aelig119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) (81)
If we choose a function 120594(119894120597120601) such that 120594(119894120597
120601+ 119896) =
119891[120594(119894120597120601)] then we have identified 119886
0rarr 120594(119894120597
120601) and
1198861= 119891(119886
0) rarr 119891[120594(119894120597
120601)] = 120594(119894120597
120601+ 119896) Similar relations can
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
Submit your manuscripts athttpwwwhindawicom
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Stochastic AnalysisInternational Journal of
ISRNMathematical Physics 7
Using the matrix representations of119876119902+ 119876
119901+ and
minusand the
wave functions equation (53) one gets [13]
(120595darr
minus120595uarr) = radic
1198821015840(119902+)
120587119890minusΔ119882
Δ119902
(120601darr
minus120601uarr) = radic
1198811015840(119901
+)
120587119890minusΔ119881
Δ119901
(120595uarr 119876
119902+120595darr) = 119894radic
1198821015840(119902minus)
120587119890minusΔ119882
(120601uarr 119876
119901+120601darr) = 119894radic
1198811015840(119901
minus)
120587119890minusΔ119881
(63)
where Δ119902 = 119902+minus 119902
minusand Δ119901 = 119901
+minus 119901
minus Hence
(120594uarr 119876
+120594darr) (120594
darr
minus120594uarr)
= 2119894radic120576[
[
(
120576119902
120576)radic120576
119902radic119882
1015840(119902minus)
120587Δ119902
minus (
120576119901
120576)radic120576
119901radic1198811015840(119901
minus)
120587Δ119901]
]
(64)
⟨119865⟩ = minus2radic120576 [
[
(
120576119902
120576)radic
1198821015840(119902+)
120587119890minus2Δ119882
Δ119902
minus (
120576119901
120576)radic
1198811015840(119901)
120587119890minus2Δ119881
Δ119901]
]
(65)
Along the actual trajectories in 119902-space (65) reproduces theresults obtained in [13]
5 An Extended SUSY Breaking in theInstanton Picture
In this Section our goal is to show that the expressionsequations (64) and (65) can be obtained in the path integralformulation of the theory by calculating the matrix elementsthat is the effect of tunneling between two classical vacuaby using a one-instanton background That is the matrixelements of
plusmn 119876
119902plusmn and 119876
119901plusmncan be calculated in the
background of the classical solution 119902119888= minus119882
119888and
119888= minus119881
119888
In doing this we rewrite the matrix element equation (62) interms of eigenstates of the conjugate operator
plusmnas follows
radic120576 [⟨+0119902+119901+
1003816100381610038161003816 119890minus119894119867ext(119879minus119905)119876
+119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816
times 119890minus119894119867ext(119879minus119905)
minus119890minus119894119867ext(119879+119905) 1003816100381610038161003816 119902+119901+0+⟩]119879rarrminus119894infin
= radic120576119902 [⟨+0119902+1003816100381610038161003816 119890
minus119894119867119902(119879minus119905)119876119902+119890minus119894119867119902(119879+119905) 1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus
1003816100381610038161003816
times 119890minus119894119867119902(119879minus119905)
minus
10038161003816100381610038161003816119890minus119894119867119902(119879+119905)119902
+0+⟩]
119879rarrminus119894infin
minus radic120576119901 [⟨+0119901+1003816100381610038161003816 119890minus119894119867119901(119879minus119905)119876
119901+119890minus119894119867119901(119879+119905)
times1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus
1003816100381610038161003816 minus
10038161003816100381610038161003816119901+0+⟩ ]
119879rarrminus119894infin
(66)
in the limit 119879 rarr minus119894infin This reduces to
radic120576 ⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= radic120576119902 ⟨+0119902+1003816100381610038161003816119876119902+
1003816100381610038161003816 119902minus0minus⟩⟨minus0119902minus1003816100381610038161003816 minus
1003816100381610038161003816 119902+0+⟩
minus radic120576119901 ⟨+0119901+1003816100381610038161003816119876119901+
1003816100381610038161003816119901minus0minus⟩⟨minus0119901minus1003816100381610038161003816 minus
1003816100381610038161003816119901+0+⟩
(67)
which in turn can be presented by path integrals definedin terms of anticommuting 119888-number operators 120577 and 120578
with Euclidean actions of the instantons in 119902- and 119901-spacesrespectively Following [13] these functional integrals includean integration over instanton time 120591
0which is due to the
problem of zero modes of the bilinear terms in Euclideanactions This arises from time-transformation of instantonsand SUSY transformations on them respectively The exis-tence of zero modes gives rise to non-Gaussian behaviour ofthe functional integral Due to it the matrix elements abovedo not receive any contributions from either no-instantonor anti-instanton configurations The zero mode problem issolved by introducing a collective coordinate 120591
0replacing the
bosonic zero mode [14] Whereas the functional integralsdepend only on the difference 120591 minus 120591
0 Note also that multi-
instanton configurations could contribute in principle pro-vided they have not more than one normalizable fermioniczero mode But as it was shown in [13] their contribution isclearly smaller with respect to radic2120576119902 and radic2120576119901 In the casewhen the SUSY potentials in 119902- and 119901-spaces have morethan two extrema 119902] and 119901120583 ] 120583 = 1 2 119873 one can putconditions on the SUSY potentials as follows
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr infin at 119902 997888rarr plusmninfin for 120595+
0
int
infin
0
119882(1199021015840) 119889119902
1015840997888rarr minusinfin at 119902 997888rarr plusmninfin for 120595minus
0
(68)
and similar to 119881(119901) that the extrema are well separated asfollows int119902]+1
119902]
119882(1199021015840)119889119902
1015840≫ 1 int119902120583+1
119901120583
119881(1199011015840)119889119901
1015840≫ 1 Around
each of the classical minima 119902] and119901120583 of the potentials1198822(119902)
and 1198812(119901) respectively one can approximate the theory
by a supersymmetric harmonic oscillator Then there are119873 ground states which have zero energy These states aredescribed by upper or lower component of the wave functiondepending on whether ] and 120583 are odd or even With thisprovision the functional integrals are calculated in [13] whichallow us consequently to write
⟨+0119902+
1003816100381610038161003816119876119902+1003816100381610038161003816 119902minus0minus⟩ = 119894
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888
⟨minus0119902minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+0+⟩ =
radic119882
1015840
119888(119902+)
120587119890minusΔ119882119888Δ119902
119888
(69)
8 ISRNMathematical Physics
and so forth Inserting this in (67) we arrive at (64)
⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= 2119894radic120576[
[
(
120576119902
120576)radic120576119902
radic119882
1015840
119888(119902+)
120587Δ119902
119888
minus (
120576119901
120576)radic120576119901
radic1198811015840
119888(119901
+)
120587Δ119901
119888]
]
(70)
and thus of (65) as its inevitable corollary This proves thatthe extended SUSY breaking has resulted from tunnelingbetween the classical vacua of the theory The correctionsto this picture are due to higher-order terms and quantum-tunneling effects
6 Spectrum Generating Algebra
An extended Hamiltonian 119867ext equation (27) can be treatedas a set of two ordinary two-dimensional partner Hamiltoni-ans [4] as follows
119867plusmn=1
2[120587
2
119902minus 120587
2
119901+ 119880
plusmn(119902 119901)] (71)
provided by partner potentials
119880plusmn(119902 119901) = 119880
119902plusmn(119902) minus 119880
119901plusmn(119901)
119880119902plusmn(119902) = 119882
2(119902 119886
119902) ∓119882
1015840
119902(119902 119886
119902)
119880119901plusmn(119901) = 119881
2(119901 119886
119901) ∓ 119881
1015840
119901(119901 119886
119901)
(72)
A subset of the SUSY potentials for which the Schrodinger-like equations are exactly solvable share an integrabilityconditions of shape-invariance [15] as follows
119880+(1198860 119902 119901) = 119880
minus(1198861 119902 119901) + 119877 (119886
0) 119886
1= 119891 (119886
0)
(73)
where 1198860and 119886
1are a set of parameters that specify phase-
space-independent properties of the potentials and thereminder 119877(119886
0) is independent of (119902 119901)
61 Algebraic Properties of Shape Invariance Using the stan-dard technique we may construct a series of Hamiltonians119867119873 119873 = 0 1 2
119867119873=1
2[120587
2
119902minus 120587
2
119901+ 119880
minus(119886119873 119902 119901) +
119873
sum
119896=1
119877 (119886119896)] (74)
where 119886119873= 119891
(119873)(119886) (119873 is the number of iterations) From
(72) and (73) we obtain then 119873 = 119899 + 119898 coupled nonlineardifferential equations which are the two recurrence relationsof Riccati-type differential equations as follows
1198822
119899+1(119902) + 119882
1015840
119902(119899+1)(119902) = 119882
2
119899(119902) minus 119882
1015840
119902119899(119902) minus 120583
119899
1198812
119898+1(119901) + 119881
1015840
119901(119898+1)(119901) = 119881
2
119898(119901) minus 119881
1015840
119901119898(119901) minus ]
119898
(75)
where we denote 119882119899(119902) equiv 119882(119902 119886
119902119899) 119881
119898(119901) equiv 119881(119901 119886
119901119898)
120583119899equiv 119877
119902(119886119902119899) and ]
119898equiv 119877
119901(119886119901119898) Here we admit that
for unbroken SUSY the eigenstates of the potentials 119880119902119901
respectively are
119864(minus)
1199020= 0 119864
(minus)
119902119899=
119899minus1
sum
119894=0
120583119894 119864
(minus)
1199010= 0 119864
(minus)
119901119898=
119898minus1
sum
119895=0
]119895
(76)
that is the ground states are at zero energies characteristic ofunbroken supersymmetryThe differential equations (75) canbe investigated to find exactly solvable potentials The shapeinvariance condition equation (73) can be expressed in termsof bosonic operators as
119861+(119909 119886
0) 119861
minus(119909 119886
0) minus 119861
minus(119909 119886
1) 119861
+(119909 119886
1)
= 119877 (1198860) = 120583
0minus ]
0
119861aelig+ (aelig 119886aelig0) 119861aeligminus (aelig 119886aelig0) minus 119861aeligminus (aelig 119886aelig1) 119861aelig+ (aelig 119886aelig1)
= (1205830or ]
0)
(77)
where 119909(119902 119901)- is the coordinate in (119902 119901)-space aelig denotesconcisely either 119902- or 119901-representations (no summation onaelig is assumed) To classify algebras associated with the shapeinvariance following [16] we introduce an auxiliary variables120601(120601
119902 120601119901) and define the following creation and annihilation
operators
119869+= 119890
119894119896120601119861+(119909 120594 (119894120597
120601)) 119869
minus= 119861
minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601
(78)
where 119896(119896119902 119896119901) are an arbitrary real constants and 120594(120594
119902 120594119901)
are an arbitrary real functions Consequently the creationand annihilation operators in (119902 119901)-spaces can be written as
119869aelig+ = 119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig))
119869aeligminus = 119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig
(79)
The operators 119861plusmn(119909 120594(119894120597
120601)) and 119861aeligplusmn(aelig 120594aelig(119894120597120601aelig )) are the
generalization of (77) where 1198860rarr 120594(119894120597
120601) and 119886aelig0 rarr
120594aelig(119894120597120601aelig ) One can easily prove the following relations
119890119894119896120601119861+(119909 120594 (119894120597
120601)) = 119861
+(119909 120594 (119894120597
120601+ 119896)) 119890
119894119896120601
119861minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601= 119890
minus119894119896120601119861minus(119909 120594 (119894120597
120601+ 119896))
(80)
and that
119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig)) = 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119890
119894119896aelig120601aelig
119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig = 119890
minus119894119896aelig120601aelig119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) (81)
If we choose a function 120594(119894120597120601) such that 120594(119894120597
120601+ 119896) =
119891[120594(119894120597120601)] then we have identified 119886
0rarr 120594(119894120597
120601) and
1198861= 119891(119886
0) rarr 119891[120594(119894120597
120601)] = 120594(119894120597
120601+ 119896) Similar relations can
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
Submit your manuscripts athttpwwwhindawicom
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Volume 2014 Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Stochastic AnalysisInternational Journal of
8 ISRNMathematical Physics
and so forth Inserting this in (67) we arrive at (64)
⟨+0119902+119901+
1003816100381610038161003816119876+1003816100381610038161003816 119902minus119901minus0minus⟩⟨minus0119902minus119901minus
1003816100381610038161003816 minus1003816100381610038161003816 119902+119901+0+⟩
= 2119894radic120576[
[
(
120576119902
120576)radic120576119902
radic119882
1015840
119888(119902+)
120587Δ119902
119888
minus (
120576119901
120576)radic120576119901
radic1198811015840
119888(119901
+)
120587Δ119901
119888]
]
(70)
and thus of (65) as its inevitable corollary This proves thatthe extended SUSY breaking has resulted from tunnelingbetween the classical vacua of the theory The correctionsto this picture are due to higher-order terms and quantum-tunneling effects
6 Spectrum Generating Algebra
An extended Hamiltonian 119867ext equation (27) can be treatedas a set of two ordinary two-dimensional partner Hamiltoni-ans [4] as follows
119867plusmn=1
2[120587
2
119902minus 120587
2
119901+ 119880
plusmn(119902 119901)] (71)
provided by partner potentials
119880plusmn(119902 119901) = 119880
119902plusmn(119902) minus 119880
119901plusmn(119901)
119880119902plusmn(119902) = 119882
2(119902 119886
119902) ∓119882
1015840
119902(119902 119886
119902)
119880119901plusmn(119901) = 119881
2(119901 119886
119901) ∓ 119881
1015840
119901(119901 119886
119901)
(72)
A subset of the SUSY potentials for which the Schrodinger-like equations are exactly solvable share an integrabilityconditions of shape-invariance [15] as follows
119880+(1198860 119902 119901) = 119880
minus(1198861 119902 119901) + 119877 (119886
0) 119886
1= 119891 (119886
0)
(73)
where 1198860and 119886
1are a set of parameters that specify phase-
space-independent properties of the potentials and thereminder 119877(119886
0) is independent of (119902 119901)
61 Algebraic Properties of Shape Invariance Using the stan-dard technique we may construct a series of Hamiltonians119867119873 119873 = 0 1 2
119867119873=1
2[120587
2
119902minus 120587
2
119901+ 119880
minus(119886119873 119902 119901) +
119873
sum
119896=1
119877 (119886119896)] (74)
where 119886119873= 119891
(119873)(119886) (119873 is the number of iterations) From
(72) and (73) we obtain then 119873 = 119899 + 119898 coupled nonlineardifferential equations which are the two recurrence relationsof Riccati-type differential equations as follows
1198822
119899+1(119902) + 119882
1015840
119902(119899+1)(119902) = 119882
2
119899(119902) minus 119882
1015840
119902119899(119902) minus 120583
119899
1198812
119898+1(119901) + 119881
1015840
119901(119898+1)(119901) = 119881
2
119898(119901) minus 119881
1015840
119901119898(119901) minus ]
119898
(75)
where we denote 119882119899(119902) equiv 119882(119902 119886
119902119899) 119881
119898(119901) equiv 119881(119901 119886
119901119898)
120583119899equiv 119877
119902(119886119902119899) and ]
119898equiv 119877
119901(119886119901119898) Here we admit that
for unbroken SUSY the eigenstates of the potentials 119880119902119901
respectively are
119864(minus)
1199020= 0 119864
(minus)
119902119899=
119899minus1
sum
119894=0
120583119894 119864
(minus)
1199010= 0 119864
(minus)
119901119898=
119898minus1
sum
119895=0
]119895
(76)
that is the ground states are at zero energies characteristic ofunbroken supersymmetryThe differential equations (75) canbe investigated to find exactly solvable potentials The shapeinvariance condition equation (73) can be expressed in termsof bosonic operators as
119861+(119909 119886
0) 119861
minus(119909 119886
0) minus 119861
minus(119909 119886
1) 119861
+(119909 119886
1)
= 119877 (1198860) = 120583
0minus ]
0
119861aelig+ (aelig 119886aelig0) 119861aeligminus (aelig 119886aelig0) minus 119861aeligminus (aelig 119886aelig1) 119861aelig+ (aelig 119886aelig1)
= (1205830or ]
0)
(77)
where 119909(119902 119901)- is the coordinate in (119902 119901)-space aelig denotesconcisely either 119902- or 119901-representations (no summation onaelig is assumed) To classify algebras associated with the shapeinvariance following [16] we introduce an auxiliary variables120601(120601
119902 120601119901) and define the following creation and annihilation
operators
119869+= 119890
119894119896120601119861+(119909 120594 (119894120597
120601)) 119869
minus= 119861
minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601
(78)
where 119896(119896119902 119896119901) are an arbitrary real constants and 120594(120594
119902 120594119901)
are an arbitrary real functions Consequently the creationand annihilation operators in (119902 119901)-spaces can be written as
119869aelig+ = 119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig))
119869aeligminus = 119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig
(79)
The operators 119861plusmn(119909 120594(119894120597
120601)) and 119861aeligplusmn(aelig 120594aelig(119894120597120601aelig )) are the
generalization of (77) where 1198860rarr 120594(119894120597
120601) and 119886aelig0 rarr
120594aelig(119894120597120601aelig ) One can easily prove the following relations
119890119894119896120601119861+(119909 120594 (119894120597
120601)) = 119861
+(119909 120594 (119894120597
120601+ 119896)) 119890
119894119896120601
119861minus(119909 120594 (119894120597
120601)) 119890
minus119894119896120601= 119890
minus119894119896120601119861minus(119909 120594 (119894120597
120601+ 119896))
(80)
and that
119890119894119896aelig120601aelig119861aelig+ (aelig 120594aelig (119894120597120601aelig)) = 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119890
119894119896aelig120601aelig
119861aeligminus (aelig 120594aelig (119894120597120601aelig)) 119890minus119894119896aelig120601aelig = 119890
minus119894119896aelig120601aelig119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) (81)
If we choose a function 120594(119894120597120601) such that 120594(119894120597
120601+ 119896) =
119891[120594(119894120597120601)] then we have identified 119886
0rarr 120594(119894120597
120601) and
1198861= 119891(119886
0) rarr 119891[120594(119894120597
120601)] = 120594(119894120597
120601+ 119896) Similar relations can
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
Submit your manuscripts athttpwwwhindawicom
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Mathematical Problems in Engineering
Hindawi Publishing Corporationhttpwwwhindawicom
Differential EquationsInternational Journal of
Volume 2014
Applied MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Probability and StatisticsHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Mathematical PhysicsAdvances in
Complex AnalysisJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
OptimizationJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
CombinatoricsHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
International Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Operations ResearchAdvances in
Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Function Spaces
Abstract and Applied AnalysisHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
International Journal of Mathematics and Mathematical Sciences
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
The Scientific World JournalHindawi Publishing Corporation httpwwwhindawicom Volume 2014
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Algebra
Discrete Dynamics in Nature and Society
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Decision SciencesAdvances in
Discrete MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom
Volume 2014 Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Stochastic AnalysisInternational Journal of
ISRNMathematical Physics 9
be obtained for the aelig-representations From (77) we obtainthen
119861+(119909 120594 (119894120597
120601)) 119861
minus(119909 120594 (119894120597
120601))
minus 119861minus(119909 120594 (119894120597
120601+ 119896)) 119861
+(119909 120594 (119894120597
120601+ 119896)) = 119877 [120594 (119894120597
120601)]
119861aelig+ (aelig 120594aelig (119894120597120601aelig)) 119861aeligminus (aelig 120594 (119894120597120601aelig))
minus 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig)) 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
= 119877aelig [120594aelig (119894120597120601aelig)]
(82)
Introducing the operators 1198693= minus(119894119896)120597
120601and 119869aelig3 = minus(119894119896aelig)120597120601aelig
and combining (79) and (82) wemay arrive at a deformed Liealgebras as follows
[119869+ 119869minus] = [119869
119902+ 119869119902minus] minus [119869
119901+ 119869119901minus]
= 120585 (1198693) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
[1198693 119869plusmn] = plusmn119869
plusmn [119869aelig+ 119869aeligminus] = 120585aelig (119869aelig3)
[119869aelig3 119869aeligplusmn] = plusmn119869aeligplusmn
(83)
where 120585(1198693) equiv 119877[120594(119894120597
120601)] and 120585aelig(119869aelig3) equiv 119877aelig[120594aelig(119894120597120601aelig )] define
the deformations Different 120594 functions in (82) define differ-ent reparametrizations corresponding to several models Forexample
(1) the translational models (1198861= 119886
0+ 119896) correspond to
120594(119911) = 119911 If 119877 is a linear function of 1198693 the algebra
becomes SO(21) or SO(3) Similar in many respectsprediction is made in somewhat different method byBalantekin [17]
(2) the scaling models (1198861= 119890
1198961198860) correspond to 120594(119911) =
119890119911 and so forth
62 The Unitary Representations of the Deformed Lie AlgebraIn order to find the energy spectrum of the partner SUSYHamiltonians
2119867minus(119909 120594 (119894120597
120601)) = 119861
minus(119909 120594 (119894120597
120601+ 119896))
times 119861+(119909 120594 (119894120597
120601+ 119896))
2119867aeligminus (aelig 120594aelig (119894120597120601aelig)) = 119861aeligminus (aelig 120594aelig (119894120597120601aelig + 119896aelig))
times 119861aelig+ (aelig 120594aelig (119894120597120601aelig + 119896aelig))
(84)
one must construct the unitary representations of deformedLie algebra defined by (83) [16 18] Using the standardtechnique one defines up to additive constants the functions119892(119869
3) and 119892aelig(119869aelig3) as follows
120585 (1198693) = 119892 (119869
3) minus 119892 (119869
3minus 1)
120585aelig (119869aelig3) = 119892aelig (119869aelig3) minus 119892aelig (119869aelig3 minus 1) (85)
The Casimirs of this algebra can be written as 1198622= 119869
minus119869++
119892(1198693) and accordingly 119862aelig2 = 119869aeligminus119869aelig+ + 119892aelig(119869aelig3) In a basis
in which 1198693and 119862
2are diagonal 119869
minusand 119869
+are lowering
and raising operators (the same holds for aelig-representations)Operating on an arbitrary state |ℎgt they yield
1198693 | ℎ⟩ = ℎ |ℎ⟩ 119869
minus | ℎ⟩ = 119886 (ℎ) |ℎ minus 1⟩
119869+ | ℎ⟩ = 119886
lowast(ℎ + 1) |ℎ + 1⟩
(86)
where
|119886 (ℎ)|2minus |119886 (ℎ + 1)|
2= 119892 (ℎ) minus 119892 (ℎ minus 1) (87)
Similar arguments can be used for the operators 119869(119901119902)3
119862aelig2 and 119869aeligplusmn which yield similar relations for the statesℎaelig The profile of 119892(ℎ) (and thus of 119892aelig(ℎaelig)) determinesthe dimension of the unitary representation Having therepresentation of the algebra associated with a characteristicmodel consequently we obtain the complete spectrum of thesystem For example without ever referring to underlyingdifferential equation we may obtain analytic expressions forthe entire energy spectrum of extended Hamiltonian withself-similar potential A scaling change of parameters is givenas 119886
1= 119876119886
0 119886aelig1 = 119876aelig119886aelig0 at the simple choice119877(119886
0) = minus119903
11198860
where 1199031is a constant That is
120585 (1198693) equiv minus119903
1exp (minus119896119869
3) = 120585
119902(1198691199023) minus 120585
119901(1198691199013)
= minus1199031199021exp (minus119896
1199021198691199023) + 119903
1199011exp (minus119896
1199011198691199013)
(88)
which yields
[119869+ 119869minus] = 120585 (119869
3) = minus119903
1exp (minus119896119869
3) [119869
3 119869plusmn] = plusmn119869
plusmn (89)
This is a deformation of the standard SO(21) Lie algebra andtherefore one gets
119892 (ℎ) =1199031
119890119896 minus 1119890minus119896ℎ
= minus1199031
1 minus 119876119876minusℎ 119876 = 119890
119896
119892aelig (ℎaelig) =119903aelig1
119890119896aelig minus 1119890minus119896aeligℎaelig = minus
119903aelig11 minus 119876aelig
119876minusℎaeligaelig
119876aelig = 119890119896aelig
(90)
For scaling problems [16] one has 0 lt 119902 lt 1 whichleads to 119896 lt 0 The unitary representation of this algebrafor monotonically decreasing profile of the function 119892(ℎ) isinfinite dimensional Let the lowest weight state of the 119869
3be
ℎmin and then 119886(ℎmin) = 0 One can choose the coefficients119886(ℎ) to be real From (87) for an arbitrary ℎ = ℎmin + 119899119899 = 0 1 2 we obtain
119886(ℎ)2= 119892 (ℎ minus 119899 minus 1) minus 119892 (ℎ minus 1) = 1199031
119876119899minus 1
119876 minus 11198761minusℎ (91)
The spectrum of the extended Hamiltonian119867minus(119909 119886
1) reads
119867minus | ℎ⟩ = 119886(ℎ)
2| ℎ⟩ = 1199031
119876119899minus 1
119876 minus 11198761minusℎ| ℎ⟩ (92)
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
Submit your manuscripts athttpwwwhindawicom
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Mathematical Problems in Engineering
Hindawi Publishing Corporationhttpwwwhindawicom
Differential EquationsInternational Journal of
Volume 2014
Applied MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Probability and StatisticsHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Mathematical PhysicsAdvances in
Complex AnalysisJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
OptimizationJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
CombinatoricsHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
International Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Operations ResearchAdvances in
Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Function Spaces
Abstract and Applied AnalysisHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
International Journal of Mathematics and Mathematical Sciences
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
The Scientific World JournalHindawi Publishing Corporation httpwwwhindawicom Volume 2014
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Algebra
Discrete Dynamics in Nature and Society
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Decision SciencesAdvances in
Discrete MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom
Volume 2014 Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Stochastic AnalysisInternational Journal of
10 ISRNMathematical Physics
with the eigenenergies
119864119899 (ℎ) = 1199031120572 (ℎ)
119876119899minus 1
119876 minus 1 120572 (ℎ) equiv 119876
1minusℎ (93)
Similar expressions can be obtained for the119867aeligminus and eigenen-ergies 119864
1199021198991and 119864
1199011198992(119899 equiv (119899
1 1198992) 119899
12= 0 1 2 ) as
119867119902minus
10038161003816100381610038161003816ℎ119902⟩ = 119886
119902(ℎ
119902)2 10038161003816100381610038161003816ℎ119902⟩ = 119903
1199021
1198761198991119902minus 1
119876119902minus 1
1198761minusℎ119902
119902
10038161003816100381610038161003816ℎ119902⟩
119867119901minus
10038161003816100381610038161003816ℎ119901⟩ = 119886
119901(ℎ
119901)2 10038161003816100381610038161003816ℎ119901⟩ = 119903
1199011
1198761198992119901minus 1
119876119901minus 1
1198761minusℎ119901
119901
10038161003816100381610038161003816ℎ119901⟩
(94)
and that
1198641199021198991(ℎ
119902) = 119903
1199021120572119902(ℎ
119902)
1198761198991119902minus 1
119876119902minus 1
120572119902(ℎ
119902) equiv 119876
1minusℎ119902
119902
1198641199011198992(ℎ
119901) = 119903
1199011120572119901(ℎ
119901)
1198761198992119901minus 1
119876119901minus 1
120572119901(ℎ
119901) equiv 119876
1minusℎ119901
119901
(95)
Hence
119864119899 (ℎ) = 1198641199021198991
(ℎ119902) minus 119864
1199011198992(ℎ
119901) (96)
7 Conclusions
Weaddressed the classical analog of the extended phase spacequantummechanics of particle which have both bosonic andfermionic degrees of freedom that is the particle with odddegrees of freedom which gives rise to (119873 = 2)-realizationof the supersymmetry algebra We obtain the integrals ofmotion We use the iterative scheme to find the approximateground state solutions to the extended Schrodinger-likeequation and calculate the parameters which measure thebreaking of extended SUSY such as the ground state energyThe approximation which went into the derivation of solu-tions of (44) meets our interest that the ground state energy120576 is supposedly smallThis gives direct evidence for the SUSYbreaking However we calculate a more practical measure forthe SUSY breaking in particular in field theories which is theexpectation value of an auxiliary field We analyze in detailthe nonperturbative mechanism for extended phase spaceSUSY breaking in the instanton picture and show that thishas resulted from tunneling between the classical vacua ofthe theory Finally we present an analysis on the independentgroup theoretical methods with nonlinear extensions of Liealgebras from the extended phase space SUSY quantummechanics Using the factorization procedure we explorethe algebraic property of shape invariance and spectrumgenerating algebra Most of these Hamiltonians possess thisfeature and hence are solvable by an independent grouptheoretical methodWe construct the unitary representationsof the deformed Lie algebra
Acknowledgments
The author would like to thank Y Sobouti for drawinghis attention to the extended phase space formulation ofquantum mechanics The knowledgable comments from theanonymous referees are much appreciated
References
[1] Y Sobouti and S Nasiri ldquoA phase space formulation of quantumstate functionsrdquo International Journal of Modern Physics B vol7 no 18 pp 3255ndash3272 1993
[2] S Nasiri Y Sobouti and F Taati ldquoPhase space quantummechanicsmdashdirectrdquo Journal ofMathematical Physics vol 47 no9 Article ID 092106 15 pages 2006
[3] G T Ter-Kazarian and Y Sobouti ldquoAn extended phase-spacestochastic quantization of constrained Hamiltonian systemsrdquoJournal of Physics A vol 41 no 31 Article ID 315303 8 pages2008
[4] G Ter-Kazarian ldquoAn extended phase-space SUSY quantummechanicsrdquo Journal of Physics A vol 42 no 5 Article ID055302 12 pages 2009
[5] H Nicolai ldquoSupersymmetry and spin systemsrdquo Journal ofPhysics A vol 9 no 9 pp 1497ndash1506 1976
[6] E Witten ldquoDynamical breaking of supersymmetryrdquo NuclearPhysics B vol 188 no 3 pp 513ndash554 1981
[7] E Witten ldquoConstraints on supersymmetry breakingrdquo NuclearPhysics B vol 202 no 2 pp 253ndash316 1982
[8] A Inomata and G Junker ldquoQuasiclassical path-integralapproach to supersymmetric quantum mechanicsrdquo PhysicalReview A vol 50 no 5 pp 3638ndash3649 1994
[9] A Inomata H Kuratsuji and C C Gerry Path Integrals andCoherent States of SU(2) and SU(11) Singapore 1992
[10] J Gamboa andMPlyushchay ldquoClassical anomalies for spinningparticlesrdquoNuclear Physics B vol 512 no 1-2 pp 485ndash504 1998
[11] G Grignani M Plyushchay and P Sodano ldquoA pseudoclassicalmodel for 119875 119879-invariant planar fermionsrdquo Nuclear Physics Bvol 464 no 1-2 pp 189ndash212 1996
[12] J L Cortes M S Plyushchay and L Velazquez ldquoA pseudo-classical model for the massive Dirac particle in 119889 dimensionsrdquoPhysics Letters B vol 306 no 1-2 pp 34ndash40 1993
[13] P Salomonson and J W van Holten ldquoFermionic coordinatesand supersymmetry in quantummechanicsrdquoNuclear Physics Bvol 196 no 3 pp 509ndash531 1982
[14] A M Polyakov ldquoQuark confinement and topology of gaugetheoriesrdquo Nuclear Physics B vol 120 no 3 pp 429ndash458 1977
[15] L Gendenshtein ldquoDerivation of exact spectra of the Schrdingerequation by means of supersymmetryrdquo Pisma Zhurnal Eksperi-mental noi i Teoreticheskoi Fiziki vol 38 pp 299ndash302 1983
[16] A Gangopadhyaya J Mallow and U P Sukhatme ldquoShapeinvariance and its connection to potential algebrardquo in Supersym-metry and IntegrableModels vol 502 of Lecture Notes in Physicspp 341ndash350 Springer 1998
[17] A B Balantekin ldquoAlgebraic approach to shape invariancerdquoPhysical Review A vol 57 no 6 pp 4188ndash4191 1998
[18] F Cooper A Khare and U Sukhatme ldquoSupersymmetry andquantummechanicsrdquo Physics Reports vol 251 no 5-6 pp 267ndash385 1995
Submit your manuscripts athttpwwwhindawicom
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Mathematical Problems in Engineering
Hindawi Publishing Corporationhttpwwwhindawicom
Differential EquationsInternational Journal of
Volume 2014
Applied MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Probability and StatisticsHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Mathematical PhysicsAdvances in
Complex AnalysisJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
OptimizationJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
CombinatoricsHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
International Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Operations ResearchAdvances in
Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Function Spaces
Abstract and Applied AnalysisHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
International Journal of Mathematics and Mathematical Sciences
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
The Scientific World JournalHindawi Publishing Corporation httpwwwhindawicom Volume 2014
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Algebra
Discrete Dynamics in Nature and Society
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Decision SciencesAdvances in
Discrete MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom
Volume 2014 Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Stochastic AnalysisInternational Journal of
Submit your manuscripts athttpwwwhindawicom
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Mathematical Problems in Engineering
Hindawi Publishing Corporationhttpwwwhindawicom
Differential EquationsInternational Journal of
Volume 2014
Applied MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Probability and StatisticsHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Mathematical PhysicsAdvances in
Complex AnalysisJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
OptimizationJournal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
CombinatoricsHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
International Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Operations ResearchAdvances in
Journal of
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Function Spaces
Abstract and Applied AnalysisHindawi Publishing Corporationhttpwwwhindawicom Volume 2014
International Journal of Mathematics and Mathematical Sciences
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
The Scientific World JournalHindawi Publishing Corporation httpwwwhindawicom Volume 2014
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Algebra
Discrete Dynamics in Nature and Society
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Decision SciencesAdvances in
Discrete MathematicsJournal of
Hindawi Publishing Corporationhttpwwwhindawicom
Volume 2014 Hindawi Publishing Corporationhttpwwwhindawicom Volume 2014
Stochastic AnalysisInternational Journal of