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Plateau transition in Hall effect: Matrix model for this ...
Transcript of Plateau transition in Hall effect: Matrix model for this ...
Plateau transition in Hall effect: Matrix model for this class of
problems
A. Sedrakyan
Yerevan Physics Institute
Cologne-2015
1. Random Networks and their connection to gravity
a) Plateau transition in Hall effect b) Integrable models on random surfaces: Non-critical strings c) Sign-factor in 3D Ising model
3. Matrix Models for random networks
For any random network consisting of different n-channel S-matrices (n-incoming and n-outgoing waves)
Definen
Khachatryan, Sedrakyan, Sorba- Nucl.Phys. B 825 (2009) 444Khachatryan , Schrader, Sedrakyan -J. Phys. A 42 (2009)304019
and plug into network
S1
1
nn
,
Rψ1 ψ2
'
ψ1
'ψ2=e
ψi
' S ij ψj+ψ2
'ψ1
' S0 ψ1 ψ2
Rψ1 ψ2
'
ψ1
'ψ2 =
ψ1'ψ2
'
ψ2ψ1
R R
R
RRR
R R
R
RR
RRR
R
R
R
R
R
R
R
R
R
R
ML
Feynman diagrams of the gauge field
)(Nsuaa
A
Z=∫∏rdψr ∏
plaquetts
Rψ1ψ2
'
ψ1
'ψ2
∫∏rdψr e
∑r ,μ
ψr
' S r ,r+μψr+μ+ ∑
plaquettes
ψ2
'ψr+μ x
' S0 ψr+μ x+μ yψr+μ y=
This can be done for all quantum spin chain models with fixed R-matrix. All chain models with local Hamiltonian have R-matrix.
What we will have if network is random?
Exp{-S( , , )}
Putting into partition function Z we get full action of the fermionic part
=
=
=
e
n
nnn
niα
nnniα
nn ψψ+)e,ψ,S(ψ=e,,ψS }{
eiα
XXR
Example: XX-model with phases, equivalent to CC model
The coordinate systems on randomML and regular ML can be connectedvia tetrads
S [ Aa ,F ]=i2
ψσa [∂a−∂a+Aa ]−ψ(m+F σ3) ψ
aadxedx
curved regular
aa e
S [ ψ , Aa ,F ]=∫d ξ ei2
ψσa eαa [∂α−∂α+Aα ]−ψ(e m+F σ3)ψ
We got fermions interacting with U(1) gauge fieldand gravity
For the averaging over U(1) disorder in supersymmetricapproach (Efetov) we need to introduce two fermionic fields,and interacting with U(1) gauge field with opposite charges together with two complex bosonic fields , which have the same action as fermions
ψ↑
ψ↓
ϕ↓ ,↑
S [ ψ↓ ,↑ ,ϕ↓ ,↑ , Aα , F ]total S [ ψ↑ ,−Aα ,−F ]S [ ψ↓ , Aα ,F ]
S [ϕ↑ ,−Aα ,−F ]S [ϕ↓ , Aα , F ]
=
++
+
W. Nudding, I. Gruzberg, A. Kluemper, A. S.-article in preparation
3D Ising model, fermionic string representation. Polyakov-1979
Sign factor exhibits Pauli principle for strings. Fermionic string
Z=∑x⃗(ξ )eα Area
Φ[ x⃗ (ξ)]
Sign-factor in 3D Ising model Kavalov, Sedrakyan—Preprint ERPHI-695(10)-1984 Nucl. Phys. B285[FS19](1987)
S=∑n,μ
ψ nΩn,n+μψ n+μ tn,n+μ
Ωn,n+μ∈SU (2 )
Φ[ x⃗ (ξ) ,ψ]=∫ dψe−S=∏CΩn ,n+μ=(−1)N N= # of fluxes
Μatrix Model for Random Network
Action
)2( NSUMconsiderj
''';'
;
'';''
;
j
j
i
i
ji
ji RRmatrixR
][][][;'';''
;'';'' MMMRMn
n
n
n
jiji
jijiTrTrMS
eMS
DMZ
FunctionPartition][
J. Ambjorn, A. Sedrakyan - Nucl.Phys.B874, 877(2013)J. Ambjorn, Sh.Khachatryan, A.Sedrakyan - PRD92, 026002(2015)
M=U mU+.
Consider adjoined representation
τa∈su((2 s+1)N )
Action become
S [m ,Λ]=mbΛb
aRacΛc
umu−∑aV (ma)
Λ=Tr [ τaU τbU ]
Action is quadratic. Gaussian integration may be used if is parametrized byfree coordinates
Λba
DM=DU dm=DΛ dm
Λ∈F (1,1,...1)=U ((2 s+1)N )
U (1)(2 s+1)N ≃∏1
(2 s+1)NCPi
Flag Manifold
DΛ=∏k=1
(2 s+1 )N−1D [CPk
]=∏k=1
(2 s+1)N−1D [
Sk
S1 ]
.≃∏k=1
(2 s+1 )N−1D [ Sk
]
¿
D [ Sk]=δ(∑1
k|z i|
2−1)∏ dz i
Z=∫∏ dmad λa e−W (ma , λa )
Summary
Random network problems and strings in real space have the same physical background.They contain matter and gauge fields interacting with gravity
Random network