UARKONIA Q EAVY H D M - uni-bielefeld.de€¦ · MOTT DISSOCIATION OF HEAVY QUARKONIA David...
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MOTT DISSOCIATION OFHEAVY QUARKONIA
David Blaschke
Institute for Theoretical Physics, University of Wroclaw, Poland
Bogoliubov Laboratory for Theoretical Physics, JINR Dubna, Russia
Outline:
• Introduction: historical remarks
•Bound states in strongly correlated plasmas
•Quantum mechanical evolution of charmonium at the QCD transition
•Mott effect for D-mesons in a hot, dense medium
EMMI Workshop “Quarkonia in Deconfined Matter”, Acitrezza, 30.09.2011
INTRODUCTION: SOME HISTORICAL REMARKS ...
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J.H.; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
INTRODUCTION: SOME HISTORICAL REMARKS ...
Ropke & group (Ahrenshoop ∼ 1987)
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J.H.; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
INTRODUCTION: SOME HISTORICAL REMARKS ...
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J.H.; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
INTRODUCTION: SOME HISTORICAL REMARKS ...
D.B. (Rostock ∼ 1988)
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J.H.; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
INTRODUCTION: SOME HISTORICAL REMARKS ...
D.B., Ropke, Schulz (Rathen 2006)
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J.H.; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
INTRODUCTION: SOME HISTORICAL REMARKS ...
Hufner, Aichelin, Werner (Heidelberg 1991)
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J. Hufner; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
INTRODUCTION: SOME HISTORICAL REMARKS ...
The Berlin Wall at Potsdamer Platz (Dec. 1989)
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J. Hufner; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
INTRODUCTION: SOME HISTORICAL REMARKS ...
Schulz, Knoll, Satz, Heinz (CERN 1990)
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J. Hufner; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
INTRODUCTION: SOME HISTORICAL REMARKS ...
Schulz, D.B., Knoll (CERN-NA38 1990)
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in National Peo-ples Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J. Hufner; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
A SNAPSHOP OF THE SQGP
The Picture: String-flip (Rearrangement) ⇐⇒ Pair correlation
1 2
Horowitz et al. PRD (1985), D.B. et al. PLB (1985),Ropke, Blaschke, Schulz, PRD (1986)
NNr r
g(r)
1
Thoma,[hep-ph/0509154]Gelman et al., PRC 74 (2006)
•Strong correlations present: hadronic spectral functions above Tc (lattice QCD)
•Finite width due to rearrangement collisions (higher order correlations)
• Liquid-like pair correlation function (nearest neighbor peak)
WHAT HAPPENS ON“H APPY ISLAND”?
"Happy Island"
quarkyonic"beach"
"cliff"
“beach” : hadron resonances −→ QGP
“cliff” :
• (unmodified) vacuum bound state energies
• fast chemical equilibration
Explanation:
Strong medium dependence of ratesfor flavor (quark) exchange processes
Reason:
• lowering of thresholds
• increase of hadron size (Pauli principle)→ geometrical overlap (percolation)
D.B., Berdermann, Cleymans, Redlich,Part. Nucl. Phys. Lett. (2011), arxiv:1102.2908;Few Body Syst. (2011) arxiv:1109.5391
HYBRID APPOACH: PNJL & MOTT-HAGEDORN RESONANCEGAS
Ptot(T, {µj}) = PPNJL(T, {µi})+∑
r=M,B
δrgr
∫ds Ar(s,mr;T )
∫d3p
(2π)3T ln
{1 + δr exp
(√p2 + s− µr
T
)}
0 100 200 300 400 500 600T [MeV]
0
3
6
9
12
P[T
4],
ε[T
4]
εQGP
= εPNJL
+ ε2
PQGP
=PPNJL
+P2
PMHRG,21
εMHRG,21
Ptot
= PMHRG,21
+ PQGP
εtot
= εMHRG,21
+ εQGP
Lattice data: Borsanyi et al. Spectral function for hadronic resonances:
Ar(s,m;T ) = NsmΓr(T )
(s−m2)2 +m2Γ2r(T )
Ansatz motivated by chemical freeze-out model:
Γr(T ) = τ−1r (T ) =
∑
h
λ < r2r >T< r2h >T nh(T )
Apparent phase transition at Tc ∼ 165 MeV
Hadron resonances present up to Tmax ∼ 250 MeV
Blaschke & Bugaev, Fizika B13, 491 (2004)
Prog. Part. Nucl. Phys. 53, 197 (2004)
Blaschke, Prorok & Turko, in preparation
T-MATRIX APPROACH TO QUARKONIA IN THE QGP
Riek & Rapp, PRC 82 (2010);arxiv:1005.0769
Open question: Wich potential to use?
U = F − TdF
dTV (r;T ) = F (r;T )− F (∞, T ) or F ↔ U
Result: J/ψ good resonancebelow 1.5 Tc for F , and 2.5 Tc for U
Lattice:Kaczmarek et al. (left), Petreczky et al. (right)
Field theoretic input:Megias et al. JHEP (2006)
D00(~k) = DP00(~k) +DNP
00 (~k)
DP00(~k) =
1
~k2 +m2D
DNP00 (~k) =
m2G
(~k2 + m2D)
2
BOUND STATES IN STRONGLY COUPLED PLASMAS(I)
Bethe-Salpeter Equation and Plasma Hamiltonan
= + = + TG Gab ab abK ab
Gab = G0ab +G0
ab Kab Gab = G0ab +G0
ab Tab G0ab
= +G G0 G0
Σ Ga a a aa
Ga = G0a +G0
aΣaGa
Equivalent Schrodinger equation [Zimmermann et al. (1978)]∑
q
{[εa(p1) + εb(p2)− z] δq,0 − Vab(q)}ψab(p1+q, p2−q, z) =∑
q
Hplab(p1, p2, q, z)ψab(p1+q, p2−q, z),
with Plasma Hamiltonian
Hplab(p1, p2, q, z) = Vab(q) [Nab(p1, p2)− 1]︸ ︷︷ ︸
(i) Pauli blocking
−∑
q′Vab(q
′) [Nab(p1 + q′, p2 − q′)− 1]
︸ ︷︷ ︸(ii) Exchange self−energy
δq,0
+ ∆Vab(p1, p2, q, z)Nab(p1, p2)︸ ︷︷ ︸(iii) Dynamically screened potential
−∑
q′∆Vab(p1, p2, q
′, z)Nab(p1 + q′, p2 − q′)
︸ ︷︷ ︸(iv) Dynamical self−energy
δq,0
In-medium modification of interaction: ∆Vab(p1, p2, q, z) = Kab(p1, p2, q, z)− Vab(q)
BOUND STATES IN STRONGLY COUPLED PLASMAS(II)
2-particle wave function ψab and phase space occupation factor Nab
•Uncorrelated fermionic medium: Nab(p1, p2) = 1− fa(p1)− fb(p2)
•Correlated medium with two-particle clusters (ψab(p1, p2, EnP ))fa(p1) → fa(p1) = fa(p1) +
∑c,n,P |ψac(p1, P − p1, EnP )|2gac(EnP )
Discussion of the plasma Hamiltonian:
•Bound states localized in x-space, therefore:over a finite range Λin q-space wave function q-independent:ψab(p1 + q, p2 − q, z = EnP ) ≈ ψab(p1, p2, z = EnP ) , for q < Λ, and vanishes for q > Λ.
• flat momentum dependence of the Pauli blocking factors:Nab(p1 + q, p2 − q) ≈ Nab(p1, p2)
• approximate cancellations of:Pauli blocking term (i) by the exchange self-energy (ii), anddynamically screened potential (iii) by the dynamical self-energy (iv)result in stability of bound states against medium effects !
•Scattering states extended in x-space → no cancellations!,but shift of the continuum threshold !
SUMMARY: Mott effect for bound states possible due to cancellations of medium effects whichdo not apply for the continuum states.
BOUND STATES IN STRONGLY COUPLED PLASMAS(III)
Application to heavy quarkonia in medium, where heavy quarks are rare
•Nab ≈ 1: Pauli blocking (i) and exchange selfenergy (ii) negligible
•medium effects due to dynamically screened potential (iii) and dynamical selfenergy (iv);from coupling of two-particle state to collective excitations (plasmons)
Screened potential (VS) approximation to interaction kernel K
V Sab(p1p2, q, z) = V S
ab(q, z)δP,p1+p2δ2q,p1−p2
V Sab(q, z) = Vab(q) + Vab(q)Πab(q, z)V
Sab(q, z) = Vab(q)[1− Πab(q, z)Vab(q)]
−1
Example: Heavy quarkonia in a relativistic quark plasma
ΠRPAab (q, z) = 2δab
∫d3p
(2π)3fa(E
ap)− fa(E
ap−q)
Eap − Ea
p−q − z.
Relativistic quark plasma described by a Polyakov-loop NJL model; evaluate the RPA polariza-tion function for Nc ×Nf massless quarks (Ea
p = |p|) in static (ω = 0), long wavelength (q → 0)case:
ΠRPAab (q → 0, 0) = 2δab
∫d3p
(2π)3dfa(E
ap)
dEap
= −2δab
∫ ∞
0
dp p
π2fΦ(p) = − δab
6π2I(Φ)T 2 ,
where I(Φ) = (12/π2)∫∞0 dxxfΦ(x) and fΦ(x) = [Φ(1+2e−x)e−x+e−3x]/[1+3Φ(1+e−x)e−x+e−3x]
is the generalized quark distribution function (Hansen et al 2006).
BOUND STATES IN STRONGLY COUPLED PLASMAS(IV)
If bare potential a color singlet one-gluon exchange V (q) = −4πα/q2, α = g2/(3π),then Fourier transform of screened potential is a Debye potential V S(r) = −α exp(−mD(T )r)/r
with Debye mass mD(T ) = 4παI(Φ)T 2.Add a screened confinement potential V S
conf(r) = (σ/mD)(1 − exp(−mDr)), calculate Hartreeselfenergies [Rapp, DB, Crochet, arxiv:0807.2470] and solve the effective Schrodinger equa-tion for
VQQ(r;T ) = −αrexp(−mD(T )r)− αmD +
σ
mD[1− exp(−mDr)]
Here σ =const, mD = mD; see Riek/Rapp, PRC 82, 035201 (2010) for σ = σ(T ) and mD 6= mD
0.1 0.2 0.3 0.4T [GeV]
0
0.3
0.6
0.9
1.2
1.5
mD
[GeV
]
with Polyakov loopwithout Polyakov loop
0 0.5 1 1.5 2r [fm]
-1
0
1
VQ
barQ
[GeV
]
T=370 MeVT=303 MeVT=240 MeVT=206 MeVT=151 MeVT=70 MeV
Temperature dependent Debye mass (left) with PL-suppressed screening and correspondingstatically screened Cornell potential (right) [Jankowski, DB, Proceedings CPOD-2010].
BOUND STATES IN STRONGLY COUPLED PLASMAS(V)
If bare potential a color singlet one-gluon exchange V (q) = −4πα/q2, α = g2/(3π),then Fourier transform of screened potential is a Debye potential V S(r) = −α exp(−µD(T )r)/rwith Debye mass µD(T ) = 4παI(Φ)T 2.Add a screened confinement potential V S
conf(r) = (σ/µD)(1−exp(−µDr)), calculate Hartree self-energies [Rapp, DB, Crochet, arxiv:0807.2470] and solve the effective Schrodinger equation
Hpl(r;T )φnl(r;T ) = Enl(T )φnl(r;T )
for the plasma Hamiltonian Hpl(r;T ) = 2mQ − αµD(T )− ~∇2/mQ + VQQ(r;T )
2.4
2.7
3
3.3
3.6
3.9
Enl
[GeV
]
0.1860.192
0.256
charmonium
J/ψχ
cψ’continuum edge
0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4T [GeV]
-0.6
-0.3
0
EB [G
eV]
-Eth= -T
EB = E
nl - (σ/µ − µ α + 2 m
c)
Tc = 0.202 GeV
9.0
9.3
9.6
9.9
10.2
10.5
Enl
[GeV
]
0.2290.244
0.469
bottomonium
Υχ
bΥ’continuum edge
0 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 0.45 0.5T [GeV]
-0.6
-0.3
0
EB [G
eV]
-Eth= -T
EB
= Enl - (σ/µ − µ α + 2 m
b)
Tc = 0.202 GeV
Two-particle energies of charmonia (left) and bottomonia (right) in a statically screened Cornellpotential, [Jankowski, DB, Grigorian, Acta Phys. Pol. B (PS) 3, 747 (2010)].
BOUND STATES IN STRONGLY COUPLED PLASMAS(VI)
Two(three-)-particle states in the medium: cluster expansion
XX
XX
T
X
X
X
X
T
=K + +X
X
X
X
Σ
T
= +X
X XX
X X
X X X
X X
X X
X X
X
= + Π= +
Π
T2L
T2L
= + + ...
Diagram expansion for 1st and2nd Born order cluster-clusterinteractions
X
X X
X
T
T
T
X
X X
X
T
T
T
’
"
Resulting plasma Hamiltonian [Ebeling, DB, et al., arxiv:0810.3336 [physics.plasm-ph]]:
Hpl = HHartree +HFock +HPauli +HMW +HDebye +Hpp +HvdW + . . . ,
QUANTUM EVOLUTION OF THE cc STATE: MATSUI’ S MODEL
Harmonic oscillator Hamiltonian
Hcc = 2mc +p2
mc+mc
4ω2x2
Time evolution operator
Uc(r, t0) =
(mcω
4πi sin(ωt0)exp
[imcω
4cot(ωt0)
])
Supression ratio (survival probability)
Rψ(t0) =|〈cc, ψ|Uc(t0)H2g→cc|2g, k0〉|2
|〈cc, ψ|H2g→cc|2g, k0〉|2
Result for pseudoscalar state
Rηc(t0, ω) =[cos2(ωt0) + (ω/ωψ)
2 sin2(ωt0)]−3/2
→ (ω2ψt
20)
−3/2 ; ω = 0, complete deconfinement
T. Matsui, Ann. Phys. 196 (1989) 182
QUANTUM EVOLUTION OF THE cc STATE: MATSUI’ S MODEL
Harmonic oscillator Hamiltonian
Hcc = 2mc +p2
mc+mc
4ω2x2
Time evolution operator
Uc(r, t0) =
(mcω
4πi sin(ωt0)
)3/2
exp
[imcω
4cot(ωt0)
]
Supression ratio (survival probability)
Rψ(t0) =|〈cc, ψ|Uc(t0)H2g→cc|2g, k0〉|2
|〈cc, ψ|H2g→cc|2g, k0〉|2
Result for pseudoscalar state
Rηc(t0, ω) =[cos2(ωt0) + (ω/ωψ)
2 sin2(ωt0)]−3/2
→ (ω2ψt
20)
−3/2 ; ω = 0, complete deconfinement
Lower Fig.: ω 6= 0, r =√
2/(mcω) = 0.6 fm
T. Matsui, Ann. Phys. 196 (1989) 182
EXTENDING THE cc OSCILLATOR MODEL TO COMPLEX
FREQUENCIES
Imaginary part in the potential (optical potential = disso-ciation) studied byCugnon/Gossiaux, ZPC 58 (1993) 77, 94Koudela/Volpe, PRC 69 (2004) 054904Harmonic oscillator with complex frequency ω2 = ω2
R+iω2I
Hcc = 2mc +p2
mc+mc
4ω2x2
Time evolution operator for infinitesimal time intervals ∆t
Uc(r,∆t) =
(mcω
4πi sin(ω∆t)
)3/2
exp
[imcω
4cot(ω∆t)
]
Supression ratio (survival probability) can oscillate ...Reasonable assumptions for time dependencies:
t ≤ t0 : ωR = ωψ; ωI = 0
t > t0 : ωR = ωR(t) : ωI = ωI(t)
→ results for the survival probability P (t), see Figureω2I = (ω0
I)2γ, γ = 1/
√1− v2rel (Lorentz factor)
K. Martins, PhD Thesis (1996), unpublished.
TIME-DEPENDENCE OF COMPLEX FREQUENCY: T-EVOLUTION
0 200 400 600 800 1000T [MeV]
0
5
10
15
20
p[T
4 ], ε
[T4 ],
cs2 , s
[T3 ]
p/T4
ε/T4
s/T3
fit formula
Lattice data: Borsanyi et al., arxiv:1007.2580
2 4 6 8 10 12 14τ [fm/c]
0.15
0.2
0.25
0.3
T [G
eV]
PHENIX AuAu, T0= 311 MeV
PHENIX AuAu, T0= 199 MeV
NA60 PbPb, T0= 224 MeV
NA60 PbPb, T0= 190 MeV
S = const = s(T (t))V (t)
T (t) from V (t) - Bjorken scaling
Harmonic oscillator with time-dependent complex fre-quency ω(t)
H(t) = 4µ +p2
2µ+µ
2ω2(t)r2
Linear combination of two solutions
r(t) = ρ(t) exp(±iφ(t)) , φ(t) =
∫ t
ti
dt′
ρ2(t′).
ρ(t) fulfills Ermakov equation (exact solutions exist)
ρ(t) + ω2(t) ρ(t)− 1
ρ3(t)= 0 .
Time evolution operator
U(tf ; ti) =
[µ ρf ρ
−1i φf
2πi sin(φf − φi)
]3/2eiScl ,
Supression ratio (survival probability)
RAA
RCNMAA
=∣∣∣ ρf/ρi
cos(φf) +(
ρf
ρf φf+ i
ωψ
φf
)sin(φf)
∣∣∣3
COMBINED DESCRIPTION OFRHIC AND SPSCENTRALITY
DEPENDENCE
0 0.1 0.2 0.3T [GeV]
0
0.5
1
1.5
2
ωR ,
ωI [ω
ψ]
ωI, γ = 2.0
ωI, γ = 1.0
ωI, γ = 0.5ωR
Td = 1.4 Tc
ωI=γ (1−ωR/ωψ)
0 100 200 300 400 500 600 700 800dN/dη|η = 0
0.4
0.6
0.8
1
1.2
RA
A /
RA
A(C
NM
)
PHENIX Au-Au, y=0NA60 In-InNA50 Pb=Pbγ = 0.0γ = 1.0γ = 2.0
EKS98 CNM baseline
Td = 1.4 Tc
D.B., C. Pena, Nucl. Phys. Proc. Suppl. 214 (2011) 137; arxiv:1106.2519
THE NA60 IN-IN “D IP” - A HINT FOR SUBTLE CORRELATIONS?
0.1 0.15 0.2 0.25T [GeV]
0
0.5
1
1.5
2
ωR ,
ωI [ω
ψ]
ωR=ωa+ωbωaωb
ωI, γ=0.22
ωI, γ=0.40
Td = 1.4 Tc
0 100 200 300 400 500 600 700 800dN/dη|η = 0
0.2
0.4
0.6
0.8
1
1.2
RA
A /
RA
A(C
NM
)
γ=0.4γ=0.22, no feedingγ=0.22PHENIX Au-Au, y=0NA60 In-InNA50 Pb=Pb
EKS98 CNM baseline
Td = 1.4 Tc
D.B., C. Pena, Nucl. Phys. Proc. Suppl. 214 (2011) 137; arxiv:1106.2519
THE NA60 IN-IN “D IP” - A CONJECTURE...
Close to Tc a resonant J/ψ - ρ interaction gives a contribution to the plasma Hamiltonian whichcould lead to a “pocket” in the effective interaction potential ...
J/ψ J/ψ J/ψ J/ψ J/ψJ/ψ J/ψ
UflipT TUflipρ ρ ρ ρ ρ ρ ρ
X X
J/ψ J/ψ J/ψ J/ψ
UflipM M*_
ρ D,D*
D,_* D
ρ ρ ρ X
X X
X
T
T
T
’
"+. . . =
X X
T
TX
X X
High density of ρ-like states in the medium is required for this contribution to be sizeable.
C. Pena, D.B., in preparation.
EXTENSION TO THELHC CASE ...
0.1 0.15 0.2 0.25T [GeV]
0
0.5
1
ωR ,
ωI [ω
ψ]
ωaωb
ωI, γ=0.44
ωR, δ=1.0
ωR, δ=1.2
ωR, δ=0.44
Td = 1.4 Tc
0 200 400 600 800 1000 1200 1400 1600dN/dη|η = 0
0.2
0.4
0.6
0.8
1
1.2
RA
A /
RA
A(C
NM
)
PHENIX Au-Au, y=0NA60 In-InNA50 Pb=PbALICE Pb-Pb0.441.01.2
EKS98 CNM baseline
Td = 1.4 Tc
Where does the real part of the oscillator strength at high temperature come from?High density of D, D∗-meson like states in the medium would feed the X-state which con-tributes to the cc plasma Hamiltonian.
C. Pena, D.B., in preparation (2011)
QUANTUM KINETIC APPROACH TO J/ψ BREAKUP (µB ≈ 0)
Gqq
GqQ
GQq
Uex Uex
GQQGQQ
J/ψJ/ψ_*D, D
_
D*M*
π, ρ
D,M
τ−1(p) = Γ(p) = Σ>(p)∓ Σ<(p)
Σ>
<(p, ω) =
∫
p′
∫
p1
∫
p2
(2π)4δp,p′;p1,p2 |M|2G<
>π (p
′) G>
<D1(p1) G
>
<D2(p2)
G>h (p) = [1± fh(p)]Ah(p) and G<
h (p) = fh(p)Ah(p)
low density approximation for the final states
fD(p) ≈ 0 ⇒ Σ<(p) ≈ 0
τ−1(p) =
∫
p′
∫
p2
∫
p2
(2π)4δp,p′;p1,p2 |M|2 fπ(p′) Aπ(p′) AD1
(p1) AD2(p2)
dσ
dt=
1
16π
|M(s, t)|2λ(s,M2
ψ, s′),
τ−1(p) =
∫d3p′
(2π)3
∫ds′ fπ(p
′, s′) Aπ(s′)vrel σ
∗(s)
In-medium breakup cross section
σ∗(s) =
∫ds1 ds2 AD1
(s1) AD2(s2) σ(s; s1, s2)
Medium effects in spectral functions Ah and σ(s; s1, s2)
MOTT EFFECT: NJL MODEL PRIMER
0 50 100 150 200 250T [MeV]
0
100
200
300
Con
stite
nt q
uark
mas
s m
and
the
pion
con
stan
t Fπ
m
m (m0=0)
Fπ
Tc
0.5Mπ
0 50 100 150 200 250T [MeV]
0
100
200
300
Dec
ay w
idth
s [M
eV]
Γσ−>ππ
Γρ−>ππ
Γρ−>qq
Γπ−>qq
Γσ−>qq
Tc
Meson propagator: RPA-type resummation,
Dh(P ) ∼ [1−GΠh(P )]−1,
e.g. Pion Pseudoscalar polarization fuction (mq = mq = m)
Ππ(Mπ,~0) = − Nc
8π2
{2A(m)− (Mπ − iΓπ/2)
2 B(Mπ,~0;m,m)}
Finite temperature (Matsubara)
A(m) = −4
∫
Λ
dpp2√E(p)
tanh(E(p)/2T ) real
B(P0,~0;m,m) = 8
∫
Λ
dpp2 tanh(E(p)/2T )
E(p)[4E2(p)− P 20 ]
real for T < Tc
Complex polarization function⇒ Breit-Wigner type spectral function
⇐= Blaschke, Burau, Volkov, Yudichev: EPJA 11 (2001) 319
Charm meson sector, seeGottfried, Klevansky, PLB 286 (1992) 221
Blaschke, Burau, Kalinovsky, Yudichev,Prog. Theor. Phys. Suppl. 149 (2003) 182
MOTT EFFECT: HEAVY MESON GENERALIZATION
ΠD(P2;T ) = 4IΛ1 (mu;T ) + 4IΛ1 (mc;T ) + 4
(P 2 − (mu −mc)
2)I(λP ,Λ)2 (P 2,mu,mc;T ),
I(λM ,Λ)2 (M,mu,mc;T ) =
Nc
8π2M
Λ∫
λP
dp p2
[Euc tanh(Eu/2T )
Eu(E2u − E2
uc)+Ecu tanh(Ec/2T )
Ec(E2c − E2
cu)
],
0 100 200 300T [MeV]
0
0.5
1
1.5
2
2.5
[Ge
V]
thresholdmasswidth
TMott
= 186 MeV
NJL with IR cutoff
K D D*
Eij = (m2i −m2
j +M2)/2M ,
Infrared cutoff (Mπ(Tc) = 2mu(Tc) = 2mcru )
λP = [mcru θ(mu −mcr
u ) +mu θ(mcru −mu)]
×θ(P 2 − 4(mcru )
2)√P 2/(2 mcr
u )2 − 1,
Meson spectral properties (mass M, width Γ)
G ReΠ(P 2 =M 2; T ) = 1
Γ(T ) = ImΠ(M2; T )/[M(T ) ReΠ′(M2; T )]
⇐= Blaschke, Burau, Kalinovsky, Yudichev,Prog. Theor. Phys. Suppl. 149 (2003) 182.
J/ψ DISSOCIATION RATE IN A π/ρ RESONANCE GAS
60 80 100 120 140 160 180 200 220 240T [MeV]
10-4
10-3
10-2
10-1
100
<σv
> [m
b]
with Mott effect without Mott effect
J/ψ + π → D* + D (+ h.c.)
NJL with IR cutoff
TMott
=186 MeV
60 80 100 120 140 160 180 200 220 240T [MeV]
10-2
10-1
100
101
<σv
> [m
b]
with Mott effectwithout Mott effect
J/ψ + ρ → D* + D* (+ h.c.)
NJL with IR cutoff
TMott
=186 MeV
Dissociation rate for a J/ψ at rest in a hot resonance gas(h = π, ρ)
τ−1(T ) = τ−1π (T ) + τ−1
ρ (T )
τ−1h (T ) =
∫d3p
(2π)3
∫ds′Ah(s
′; T )fh(p, s′; T )jh(p, s
′)σ∗h(s; T )
= 〈σ∗hvrel〉nh(T ) ,
fh(p, s; T ) = gh{exp[(√p2 + s− µ)/T ]− 1}−1
s(p, s′) = s′ +M2ψ + 2Mψ
√p2 + s′
• Masses slightly rising below TMott
⇒ reduction of breakup rate
• Mott-effect for intermediate states at TMott
⇒ breakup enhancement - “subthreshold” process
• Structure in the breakup rate at T = TMott
• Additional J/ψ absorption channel opens⇒ “anomalous” suppression
CHARM AND CHARMONIUM PRODUCTION @ RHIC
0 1 2 3 4 5p
T [GeV]
0
0.5
1
1.5
2
RA
A
c+b resoc+b pQCDc resoPHENIX prel.
Au-Au (√s=200 GeV)
0 1 2 3 4 5p
T [GeV]
0
5
10
15
20
25
-5
v 2 [%]
c+b resoc+b pQCDc reso
STAR prel.PHENIX
Au-Au (√s=200 GeV)
0 50 100 150 200 250 300 350N
part
0
0.2
0.4
0.6
0.8
1
1.2
1.4
R AA
PHENIXdirectregenerationsumτ
c
eq~5fm/c
Tdiss
=1.25Tc
Au-Au (200 A GeV)
Recombination of open charm (regeneration of ψ)
dNψ/dt = −Γψ[Nψ −N eqψ (T )]
Hees, Mannarelli, Greco, Rapp, PRL 100, 192301(2008)Nuclear modification factor RAA and elliptic flow v2 ofsemileptonic D− and B− meson decay-electrons inb = 7 fm Au-Au (
√s = 200 GeV) collisions at RHIC
⇐= Hees, Greco, Rapp, PRC 73, 034913 (2006)
CHARM AND CHARMONIUM PRODUCTION @ FAIR-CBM
__ _GQq
Uex Uex
GQQ
GqqQ
Gqqq
GQQ
J/ψ dissociation process in dense baryonic matterat FAIR-CBM: spectral functions for open charmhadrons (D-meson, Λc) are essential inputs!⇐=
D-meson spectral function in cold dense nuclearmatter from a G-matrix approach ↓
1600 1700 1800 1900ωD (MeV)
0
1
2
3
4
5
6
7
8
S D(kD=0
,ω) (G
eV−2
)
ρ=0.5ρ0
ρ=ρ0
ρ=1.5ρ0
1600 1700 1800 1900 2000ωD (MeV)
Tolos et al., EPJC (2005); nucl-th/0501151
QUANTUM KINETICS OF J/ψ DISSOCIATION @ CBM (µB 6= 0)
__ _GQq
Uex Uex
GQQ
GqqQ
Gqqq
GQQ
J/ψJ/ψ
M*
D_
Λ cM
N
Charmonium lifetime in a dense nuclear medium (fD ≈ 0)
τ−1(p) =
∫
p′
∫
p2
∫
p2
(2π)4δp,p′;p1,p2 |M|2 fN(p′) AN(p′) AΛ(p1) AD(p2)
Medium effects in hadronic spectral functions Ah and σ(s; s1, s2)D-meson spectral function in cold dense nuclear matter from a G-matrix approach ↓ (N, Λc similar)
1600 1700 1800 1900ωD (MeV)
0
1
2
3
4
5
6
7
8
S D(k D=0,ω)
(GeV
−2)
ρ=0.5ρ0
ρ=ρ0
ρ=1.5ρ0
1600 1700 1800 1900 2000ωD (MeV)
Tolos et al., EPJC (2005); PRC 80, 065202 (2009)
QUANTUM KINETICS OF J/ψ DISSOCIATION @ CBM (µB 6= 0)
__ _GQq
Uex Uex
GQQ
GqqQ
Gqqq
GQQ
J/ψJ/ψ
M*
D_
Λ cM
N
Charmonium lifetime in a dense nuclear medium (fD ≈ 0)
τ−1(p) =
∫
p′
∫
p2
∫
p2
(2π)4δp,p′;p1,p2 |M|2 fN(p′) AN(p′) AΛ(p1) AD(p2)
Medium effects in hadronic spectral functions Ah and σ(s; s1, s2)D-meson spectral function in hot, dense quark matter from a NJLmodel approach ↓ (N, Λc similar)
1850
1900
1950
2000
2050
2100
mas
s [M
eV]
0 1 2 3 4 5 6density n [n
0]
0100200300400500
widt
h [M
eV]
T = µ/3
D+
D-
D-
D+
Mu(d)
+Mc
D.B., P. Costa, Yu. Kalinovsky, arxiv:1107.2913
SUMMARY
•Diagram expansions in strongly correlated quark plasma guided by plasma physics
•Microscopic formulation of the hadronic Mott effect within a chiral quark model
•Mesonic (hadronic) correlations important for T > Tc
•Step-like enhancement of threshold processes due to Mott effect
•Reaction kinetics for strong correlations in plasmas applicable @ SPS and RHIC
•Prospects for CBM: Anomalous suppression expected, eventually (more) steplike!
PLANS FOR THE FUTURE
•Bridge Lattice QCD and Phenomenology: spectral functions
•Calculate J/ψ breakup with baryon impact =⇒ CBM @ FAIR GSI
•Mott effect in dense baryonic matter: nucleon dissociation!
•EoS for hot, dense matter with Mott-effect, encoded in hadronic spectral functions
CONCLUSION: MOTT DISSOCIATION STILL INTERESTING...
• 1983: Mott effect and color deconfinement
• 1984: Mott effect and hadron-to-quark mattertransition
• 1986: Matsui-Satz; (Blaschke in N. P. Army)
• 1987: Mott dissociation; NA38 data
• 1989: Meeting H.S., J. Hufner; Wall breakup
• 1990: 1st Visit at CERN - NA38
• ...
• 2011: EMMI workshop Acitrezza
THANKS FOR YOUR INSPIRING WORK, HELMUT !
INVITATION : V ISIT WROCŁAW & U NIVERSITY