Upload
davida
View
58
Download
3
Tags:
Embed Size (px)
DESCRIPTION
1) Motivation 2) Mean Field Theory at T = 0 3) Fluctuations at T ≠ 0 4) Application to QCD: Color Superconductivity and Pion Superfluid 5) Conclusions. Relativistic BCS-BEC Crossover at Quark Level. - PowerPoint PPT Presentation
Citation preview
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 11
Relativistic BCS-BEC Crossover at Quark LevelRelativistic BCS-BEC Crossover at Quark Level Pengfei Zhuang Physics Pengfei Zhuang Physics
Department, Tsinghua University, Beijing 100084Department, Tsinghua University, Beijing 100084
1) Motivation1) Motivation
2) Mean Field Theory at T = 0 2) Mean Field Theory at T = 0
3) Fluctuations at T≠ 03) Fluctuations at T≠ 0
4) Application to QCD: 4) Application to QCD: Color Superconductivity and Pion Superfluid Color Superconductivity and Pion Superfluid
5) Conclusions5) Conclusions
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 22
1) Motivation1) Motivation
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 33
BCS-BECBCS-BEC
BCS BCS (Barden, Cooper and Schrieffer, 1957):(Barden, Cooper and Schrieffer, 1957): normal superconductivitynormal superconductivity weak coupling, large pair size, k-space pairing, overlaping Cooper weak coupling, large pair size, k-space pairing, overlaping Cooper
pairspairs BEC BEC (Bose-Einstein-Condensation, 1924/1925):(Bose-Einstein-Condensation, 1924/1925): strong coupling, small pair size, r-space pairing, ideal strong coupling, small pair size, r-space pairing, ideal gas of bosons, first realization in dilute atomic gas with bosons in gas of bosons, first realization in dilute atomic gas with bosons in
1995.1995. BCS-BEC crossoverBCS-BEC crossover (Eagles, Leggett, (Eagles, Leggett,
1969, 1980):1969, 1980): BCS wave function at T=0 can be generalized to arbitrary BCS wave function at T=0 can be generalized to arbitrary
attraction: aattraction: a smoothsmooth crossover from BCS to BEC!crossover from BCS to BEC!
BEC of moleculesBEC of molecules BCS fermionic superfluidBCS fermionic superfluid
2/12
2/1
1 kB
kBk
N
Nv
BCSBCS
0exp 2/10
kkk k ccNB
BECBEC
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 44
pairingspairings
in BCS, Tin BCS, Tcc is determined by thermal excitation of fermions, is determined by thermal excitation of fermions,
in BEC, Tin BEC, Tcc is controlled by thermal excitation of collective modes is controlled by thermal excitation of collective modes
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 55
in order to study the question of ‘vacuum’, we must turn to a different in order to study the question of ‘vacuum’, we must turn to a different direction: we should investigate some ‘bulk’ phenomena by distributing direction: we should investigate some ‘bulk’ phenomena by distributing
high energy over a relatively large volume.high energy over a relatively large volume.
BCS-BEC in QCDBCS-BEC in QCD
T. D. Lee, Rev. Mod. Phys. 47, 267(1975)T. D. Lee, Rev. Mod. Phys. 47, 267(1975)
pair dissociation line
BCSBEC
sQGP
QCD phase diagramQCD phase diagram
rich QCD phase structure at high density, natural attractive interaction rich QCD phase structure at high density, natural attractive interaction in QCD, possible BCS-BEC crossover ?in QCD, possible BCS-BEC crossover ?
new phenomena in BCS-BEC crossover of QCD:new phenomena in BCS-BEC crossover of QCD: relativistic systems, anti-fermion contribution, rich inner structure relativistic systems, anti-fermion contribution, rich inner structure (color, flavor), medium dependent mass, ……(color, flavor), medium dependent mass, ……
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 66
theory of BCS-BEC crossovertheory of BCS-BEC crossover
*) Leggett mean field theory (Leggett, 1980) *) Leggett mean field theory (Leggett, 1980) *)NSR scheme (Nozieres and Schmitt-Rink, 1985) *)NSR scheme (Nozieres and Schmitt-Rink, 1985) extension of of BCS-BEC crossover theory at T=0 to T extension of of BCS-BEC crossover theory at T=0 to T≠0 (above T≠0 (above Tcc
) ) Nishida and Abuki (2006,2007) Nishida and Abuki (2006,2007) extension of non-relativistic NSR theory to relativistic systems, extension of non-relativistic NSR theory to relativistic systems, BCS-NBEC-RBEC crossover BCS-NBEC-RBEC crossover
4
0 04
1ln ( ) ,
(2 )fl
d qq G G
G
*) *) GG00G scheme (Chen, Levin et al., 1998, 2000, 2005)G scheme (Chen, Levin et al., 1998, 2000, 2005)
asymmetric pair susceptibility asymmetric pair susceptibility 0 G G extension of non-relativistic extension of non-relativistic GG00G scheme to relativistic systems (He, G scheme to relativistic systems (He,
Zhuang, 2006, 2007)Zhuang, 2006, 2007)
*) Bose-fermion model (Friedderg, Lee, 1989, 1990)*) Bose-fermion model (Friedderg, Lee, 1989, 1990) extension to relativistic systems (Deng, Wang, 2007) extension to relativistic systems (Deng, Wang, 2007) Kitazawa, Rischke, Shovkovy, 2007, NJL+phase diagram Kitazawa, Rischke, Shovkovy, 2007, NJL+phase diagram Brauner, 2008, collective excitations ……Brauner, 2008, collective excitations ……
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 77
2) 2) Leggett Leggett Mean Field Theory at T = 0Mean Field Theory at T = 0 A.J.Leggett, in Modern trends in the theory of condensed matter, A.J.Leggett, in Modern trends in the theory of condensed matter, Springer-Verlag (1980) Springer-Verlag (1980)
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 88
non-relativistic mean field theorynon-relativistic mean field theory
fermion number: fermion number: Fermi momentum: Fermi momentum:
Fermi energy:Fermi energy:
3 2, / 3F Fk n k p=
2
32tL i h gm
2 2g g
2 3 2
3(2 ) 4k kk
d kE
g
order parameterorder parameter
2 2 2, , / 2k k k k kE k mx x e m e= +D = - =
n
2 / 2F Fk me =
thermodynamics in mean field approximationthermodynamics in mean field approximation
quasi-particle energyquasi-particle energy
renormalization to avoid the integration divergence renormalization to avoid the integration divergence 3
3
1 1,
4 (2 ) 2
0 for attractive coupling, 0 for repulsive coupling
ss k
s s
m d kg a
a g
a a
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 99
universalityuniversality
0
gap equationgap equation
n
number conservationnumber conservation
( ), ( )n n
3
3
3
3
1 1
4 (2 ) 2 2
1(2 )
s k k
k
k
m d k
a E
d kn
E
2222 20
22
22 20
1ˆ / , / ,
1 1
2
ˆ21
3
F FF sk a
dxxxx
xdxx
x
universalityuniversality
ˆ ( ), ( )
effective couplingeffective coupling
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1010
BCS limit
BEC limit
non-relativistic BCS-BEC crossovernon-relativistic BCS-BEC crossover
2 /2
8ˆ, , 1e
e
2
2
( ) /
16ˆ, ,
31
, 2
1( ) 0
1
bb
s
T
ma
n pe
BCS-BEC crossover0 0,
small large ,
0 0
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1111
relativistic BCS-BEC crossoverrelativistic BCS-BEC crossover
0, m mm m- = =
( )2 2 2 2, k k kE k m
m
x x m
m
± ± ±= +D = + ±
-
2
, 02
0
b
b
m
m m
e
em m
m
<
- >- ³ - ³
®
BCS-BEC crossover around BCS-BEC crossover around
plays the role of non-relativistic chemical potentialplays the role of non-relativistic chemical potential
pair binding energypair binding energy
atat fermion and anti-fermion degenerate, fermion and anti-fermion degenerate, relativistic effectrelativistic effect
0 m m
BCS BCS limitlimit
NBEC-BCS NBEC-BCS crossovercrossover
NBECNBECRBEC-NBEC RBEC-NBEC crossovercrossover
RBEC RBEC limitlimit
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1212
relativistic mean field theoryrelativistic mean field theory
5 5
0 2
4T Tg
L i m i C iC
C i
52TgiC
2 3
3(2 ) k k k k
d kE E
g
order parameterorder parameter
antifermionantifermion
extremely high T and high density: pQCD extremely high T and high density: pQCD finite T (zero density): lattice QCD finite T (zero density): lattice QCD moderate T and density: models like 4-fermion interaction (NJL)moderate T and density: models like 4-fermion interaction (NJL)
charge conjunction matrixcharge conjunction matrix
mean field thermodynamic potentialmean field thermodynamic potential
the most important thermodynamic contribution from the uncondensed the most important thermodynamic contribution from the uncondensed pairs is from the Goldstone modes, , at T=0, the fluctuation pairs is from the Goldstone modes, , at T=0, the fluctuation contribution disappears, and MF is a good approximation at T=0.contribution disappears, and MF is a good approximation at T=0.
4T
fermionfermion
He, Zhuang, 2007He, Zhuang, 2007
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1313
broken universalitybroken universality
gap equation and number equation: gap equation and number equation: 3
3
3
3
1 1 1
(2 ) 2 2
1 1(2 )
k k
k k
k k
d k
g E E
d kn
E E
22 2
0
2
0
1 1 1 1
2 2 2
21 1
3
1,
z
x x x x
zx x
x x
F
F s
dxxE E
dxxE E
k
k a m
renormalization to avoid the integration divergence renormalization to avoid the integration divergence 3
3
41 1 1 1 1,
2 (2 )s
k k
ad kU
U g m m m
the ultraviolet divergence can not be completely removed, and a the ultraviolet divergence can not be completely removed, and a momentum cutoff still exists in the theory.momentum cutoff still exists in the theory.
broken universality:broken universality:
explicit density dependence !explicit density dependence !
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1414
m m / 1Fk m
non-relativistic limit: 1) non-relativistic kinetics 2) negligible anti-fermions ●
●
1
2
( , ) ( )
( , ) 0 ( )
c
c
mmh z h z
mh z h z
= Þ
® Þ
● NBEC
● RBEC
non-relativistic limitnon-relativistic limit
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1515
density induced crossoverdensity induced crossover
atom gas
QCD
1/ F sk a In non-relativistic case, only one dimensionless variable, , changing the density of the system can not induce a BCS-BEC crossover. However, in relativistic case, the extra density dependence may induce a BCS-BEC crossover.
/Fk mz=
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1616
3) Fluctuations at T≠ 0 3) Fluctuations at T≠ 0
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1717
● ● the the Landau mean field theory Landau mean field theory is a good approximation only at T=0 is a good approximation only at T=0 where there is no thermal excitation,where there is no thermal excitation, one has to go beyond the mean one has to go beyond the mean field at finite temperature.field at finite temperature.
pair dissociation line
BCSBEC
sQGP
● ● an urgent question in relativistic heavy ion collisionsan urgent question in relativistic heavy ion collisions
introductionintroduction
tto understand the sQGP phase o understand the sQGP phase with possible bound states of with possible bound states of quarks and gluons, one has to quarks and gluons, one has to go beyond the mean field !go beyond the mean field !
● ● going beyond mean field self-consistently is very difficultgoing beyond mean field self-consistently is very difficult
NSR Theory (GNSR Theory (G00GG00 Scheme) above T Scheme) above Tcc: Nishida and Abuki (2005),: Nishida and Abuki (2005),Bose-Fermi Model: Deng and Wang (2006),Bose-Fermi Model: Deng and Wang (2006),GG00G Scheme below TG Scheme below Tcc: He and Zhuang (2007), ……: He and Zhuang (2007), ……
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1818
10 0 0( , ) ( )G k k k m
0 0
3
03
1 ( , ) ( , ) 0, ( , ) 2
2 , , ,
(2 1) , (2 )
k k
n n
gi Tr G k G k n i Tr G k
n T bosonsd kiT k i
n T fermi
k n ons
20( ) ( , )mf k G k
5 54T Tg
L i m i C iC
fermion propagator with diagonal and off-diagonal elements in Nambu-Gorkov spacefermion propagator with diagonal and off-diagonal elements in Nambu-Gorkov space
bare propagator and bare propagator and condensate induced self-energycondensate induced self-energy
( , ) ( , )( , )
( , ) ( , )
G k F kS k
F k G k
1 10
5 0
( , ) ( , ) ( )
( , ) ( , ) ( , )
mfG k G k k
F k G k i G k
gap and number equations at finite Tgap and number equations at finite T
3
3
3
3
1 2 ( ) 1 2 ( )1
(2 ) 2 2
1 1 2 ( ) 1 1 2 ( )(2 )
k k
k k
k kk k
k k
f E f Ed k
g E E
d kn f E f E
E E
gap and number equations in terms of the fermion propagatorgap and number equations in terms of the fermion propagator
mean field fermion propagatormean field fermion propagator
Matsubara frequency summation Matsubara frequency summation
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 1919
2
( ) ( )mft q i qT
0 G Gmean field theory in schememean field theory in scheme
introducing a condensed-pair propagatorintroducing a condensed-pair propagator
0( ) ( ) ( , )mf mfq
k t q G q k
0( ) ( , ) ( , )2 k
iq Tr G k G q k
1(0) 0t
gap equation in condensed phase is determined by uncondensed pairsgap equation in condensed phase is determined by uncondensed pairs
0G
mft
( )1 ( )
igt q
g q
problem: problem: there is no feedback of the uncondensed pairs on the fermion self- there is no feedback of the uncondensed pairs on the fermion self-energy energy
defining an uncondensed pair propagatordefining an uncondensed pair propagator
the name scheme, the name scheme, G is the mean field G is the mean field fermion propagatorfermion propagator
0 G G
( , )T
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2020
2
( ) ( ) ( )
( ) ( )
( )1 ( )
mf pg
mf
pg
t q t q t q
t q i qTig
t qg q
0( ) ( , ) ( , )2 k
iq Tr G k G q k
full pair propagatorfull pair propagator
0( ) ( ) ( , )
( ) ( )
q
mf pg
k t q G q k
k k
1 10( , ) ( , ) ( )G k G k k
going beyond mean field in schemegoing beyond mean field in scheme0G G
with full susceptibility and full propagatorwith full susceptibility and full propagator
full fermion self-energyfull fermion self-energy
pgt
1 (0) 0pgt
fermions and pairs are coupled to each otherfermions and pairs are coupled to each other
new gap equationnew gap equation ( , )T a new order parameter which is a new order parameter which is different from the mean field onedifferent from the mean field one
all the formulas look the same as the mean field ones, all the formulas look the same as the mean field ones, but we do not know the expression of the full fermion propagator G.but we do not know the expression of the full fermion propagator G.
He, Zhuang, 2007He, Zhuang, 2007
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2121
approximation in condensed phaseapproximation in condensed phase
1) peaks at 1 (0) 0pgt ( )pgt q
20 0 0
0 0
2
0
( ) ( ) ( , ) ( ) ( , ) ( , )
( )
pg pg pg pgq q
pg pgq
k t q G q k t q G k G k
t q
0q
2 20( ) ( ) ( ) ( , )mf pg pgk k k G k
1 (0) 0pgt
0 0
2 2 21 0 2 0
2 2
1 2 22 20 0 00 0
( )1 ( ) ( ) (0)
1 1, ,
2 2
pg
qq q
ig i it q
g q q Z q Z q q
Z Zq q q
0q
2 2
32
32
mean field gap equation with
( ) ( )1
(2 ) 2
pg
b q b qpg
q
f v f vd q
Z
v
2 2 21 2 q 2/ 2 , /Z Z q Z v
, , ,pgT T
the pseudogap is related to the uncondensed the pseudogap is related to the uncondensed pairs and does not change the symmetry !pairs and does not change the symmetry !
full self-energy
2) expansion around
1 (0) 0pgt gap equation mean field gap equation withgap equation mean field gap equation with 2 2
pg
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2222
thermodynamicsthermodynamics
2
2 3
3
3
3
3/ 2
1 23
3
3
1ln 1 1
(2 )
1ln 1 ( ) ln 1 1
(2 )
1ln 1 Z ,
(2 )
2ln 1
(2 )
k k
q q
B
mf fl
E Emf k k k k
flq
q m
d kE E e e
g
d qg q e e
d qe Z non relativistic boson gas
d qe
2 1 Z , cq Z relativistic boson gas
3
2 2132 (2 )
mf flB k k pg B B
n d kn f f Z n n
number of bosonsnumber of bosons
21
/ 2 / 2
mfB
c
n ZP
n n
fraction of condensed pairsfraction of condensed pairs
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2323
BCS-NBEC-RBEC crossoverBCS-NBEC-RBEC crossover
*
*
: critical temperature
: 0, condensed phase
: 0, normal or pseudogap phase
: pair dissociation temperature
: 0, pseudogap phase
c
c
c
c pg
T
T T
T T
T
T T T
* : 0 normal phasepgT T
BCS: no pairs BCS: no pairs
NBEC: heavy pairs, no anti-pairsNBEC: heavy pairs, no anti-pairs
RBEC: light pairs, almost the same RBEC: light pairs, almost the same number of pairs and anti-pairsnumber of pairs and anti-pairs
0, m 0 / , 0<Fm k m
/ , 0Fm k
●●
●●
/( / 2)B Br n n
1F Br r
number fractions at Tnumber fractions at Tc c , ,
in RBEC, Tin RBEC, Tcc is large enough and is large enough and
there is a strong competition there is a strong competition between condensation and between condensation and dissociation.dissociation.
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2424
discussion on discussion on 0G G
10 51
15 0
( , ) ( , )( )
( , ) ( , )pg
pg
G k k iS k
i G k k
can the symmetry be restored in the pseudogap phase? can the symmetry be restored in the pseudogap phase?
fermion propagator including fluctuations (to the order of ) :fermion propagator including fluctuations (to the order of ) :2 2/
the pseudogap appears in the diagonal elements of the propagator the pseudogap appears in the diagonal elements of the propagator and does not break the symmetry of the system. and does not break the symmetry of the system.
Kandanoff and Martin: Kandanoff and Martin: the scheme can not give a correct symmetry restoration the scheme can not give a correct symmetry restoration picture and the specific heat is wrong. picture and the specific heat is wrong.
GG 2
VC T
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2525
BCS-BEC in Bose-fermion modelBCS-BEC in Bose-fermion modelDeng, Wang, 2007Deng, Wang, 2007
mean field thermodynamicsmean field thermodynamics
fluctuation changes the phase fluctuation changes the phase transition to be first-order.transition to be first-order.
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2626
4) Application to QCD: 4) Application to QCD: Color Superconductivity and Pion SuperfluidColor Superconductivity and Pion Superfluid
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2727
motivationmotivation
* QCD phase transitions like chiral symmetry restoration, color * QCD phase transitions like chiral symmetry restoration, color superconductivity, and pion superfluid happen in non-perturbative superconductivity, and pion superfluid happen in non-perturbative temperature and density region, the coupling is strong. temperature and density region, the coupling is strong.
* relativistic BCS-BEC crossover is controlled by , the BEC-BCS * relativistic BCS-BEC crossover is controlled by , the BEC-BCS crossover would happen when the light quark mass changes in the crossover would happen when the light quark mass changes in the QCD medium. QCD medium.
* effective models at hadron level can only describe BEC state, they * effective models at hadron level can only describe BEC state, they can not describe BEC-BCS crossover. One of the models that enables can not describe BEC-BCS crossover. One of the models that enables us to describe both quarks and mesons and diquarks is the NJL model us to describe both quarks and mesons and diquarks is the NJL model at quark level.at quark level.
disadvantage: no confinementdisadvantage: no confinement
* there is no problem to do lattice simulation for real QCD at finite * there is no problem to do lattice simulation for real QCD at finite
isospin densityisospin density
m
2 2
0 0 5 5 5C ij ij C
NJL S i D i j i jL i m G i G i i
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2828
1 2 2 1 1 2 2 1 3 3 3 3 C C C C C Cu d d u d u u d u u d d 1
2
2
1
1
2
2
1
3
3
3
3
u
Cd
d
Cu
d
Cu
u
Cd
u
Cu
d
Cd
3 3
5C iji ji
order parameters of spontaneous chiral and color symmetry breakingorder parameters of spontaneous chiral and color symmetry breaking
quark propagator in 12D Nambu-Gorkov spacequark propagator in 12D Nambu-Gorkov space
A
B
C
D
E
F
S
S
SS
S
S
S
I II
I I
GS
G
0 2q SM m G
, , , , ,I A B C D E F
2 2
2 22
k q
k D
E k M
E E G
color superconductivitycolor superconductivity
color breaking from SU(3) to SU(2)
diquark & meson polarizationsdiquark & meson polarizations
M D
diquark & meson propagators at RPAdiquark & meson propagators at RPA
leading order of 1/Nleading order of 1/Ncc for quarks, and next to leading order for mesons & diquarks for quarks, and next to leading order for mesons & diquarks
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 2929
BCS-BEC and color neutralityBCS-BEC and color neutrality
gap equations for chiral and diquark condensates at T=0gap equations for chiral and diquark condensates at T=0
3
0 3
3
3
/ 3 / 318 / 3
(2 )
1 18
(2 )
k B k Bs k B
p
d
E Ed km m G m E
E E E
d kG
E E
/ 3 /B d sm m G G
●● ●●
there exists a BCS-BEC crossoverthere exists a BCS-BEC crossover
to guarantee color neutrality, we introduce to guarantee color neutrality, we introduce color chemical potential: color chemical potential:
8 8/ 3 / 3, / 3 2 / 3r g B b B
color neutrality speeds up the chiral color neutrality speeds up the chiral restoration and reduces the BEC regionrestoration and reduces the BEC region
●● ●●
r m
He, Zhuang, 2007He, Zhuang, 2007
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3030
vector meson coupling and magnetic instabilityvector meson coupling and magnetic instability
vector-meson couplingvector-meson coupling 2 2
5V VL G
gap equationgap equation
02V VG
vector meson coupling slows down vector meson coupling slows down the chiral symmetry restoration and the chiral symmetry restoration and enlarges the BEC region. enlarges the BEC region.
vector condensatevector condensate
3
3
/ 3 / 38 / 3
(2 )k B k B
V V k B
E Ed kG E
E E
1
Meissner masses of some gluons Meissner masses of some gluons are negative for the BCS Gapless are negative for the BCS Gapless CSC, CSC, but the magnetic instability but the magnetic instability is cured in BEC region.is cured in BEC region.
r m
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3131
beyond men fieldbeyond men field
0 100 200 MeV 300 500 MeVq 0 ( 0)T is determined by the coupling and chemical potentialis determined by the coupling and chemical potential
● going beyond mean field reduces the critical temperature of color going beyond mean field reduces the critical temperature of color superconductivitysuperconductivity ● ● pairing effect is important around the critical temperature and dominates the pairing effect is important around the critical temperature and dominates the symmetry restored phasesymmetry restored phase
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3232
NJL with isospin symmetry breakingNJL with isospin symmetry breaking
2 2 1
2 2 2 2
2 2 2 2
( ) Tr Ln
0, 0, 0, 0, 0, 0, 0, 0u u d d
TG S
V
q q
2 2
0 0 5NJL iL i m G i
, , u d u duu dd chiral and pion condensates with finite pair momentumchiral and pion condensates with finite pair momentum
quark propagator in MFquark propagator in MF 0 51
5 0
2( , )
2u
d
p q m iGS p q
iG k q m
0 2m m G
2 25 52 , 2
2 2iq x iq xui d e di u e
quark chemical potentialsquark chemical potentials
0 / 3 / 2 0
0 0 / 3 / 2u B I
d B I
thermodynamic potential and gap equations:thermodynamic potential and gap equations:
pion superfluidpion superfluid
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3333
5
5
3 5 0
1,
,
,
,
m
m
i m
i m
i m
4
*4
( ) Tr ( ) ( )(2 )mn m n
d pk i S p k S p
meson polarization functionsmeson polarization functions
meson propagator at RPAmeson propagator at RPA
pole of the propagator determines meson masses pole of the propagator determines meson masses
mixing among normal in pion superfluid phase, mixing among normal in pion superfluid phase,
the new eigen modes are linear combinations of the new eigen modes are linear combinations of
considering all possible channels in the bubble summationconsidering all possible channels in the bubble summation
0
0
0
0 0 0 0 00 , 0
1 2 ( ) 2 ( ) 2 ( ) 2 ( )
2 ( ) 1 2 ( ) 2 ( ) 2 ( )det
2 ( ) 2 ( ) 1 2 ( ) 2 ( )
2 ( ) 2 ( ) 2 ( ) 1 2 ( )mk M k
G k G k G k G k
G k G k G k G k
G k G k G k G k
G k G k G k G k
0
, ,
mM
, ,
D
mesons in RPAmesons in RPA
, ,
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3434
I B
chiral and pion condensates at chiral and pion condensates at in NJL, Linear Sigma Model and Chiral in NJL, Linear Sigma Model and Chiral Perturbation Theory, there is no remarkable Perturbation Theory, there is no remarkable difference around the critical point.difference around the critical point.
analytic result: analytic result: critical isospin chemical potential for pion critical isospin chemical potential for pion superfluidity is exactly the pion mass in the superfluidity is exactly the pion mass in the vacuum: vacuum:
0BT q
cI m
( )B BnI
pion superfluidity phase diagram in pion superfluidity phase diagram in plane at T=0plane at T=0
: average Fermi surface: average Fermi surface
: Fermi surface mismatch : Fermi surface mismatch
homogeneous (Sarma, ) and homogeneous (Sarma, ) and inhomogeneous pion superfluid (LOFF, )inhomogeneous pion superfluid (LOFF, )
magnetic instability of Sarma state at high magnetic instability of Sarma state at high average Fermi surface leads to the LOFF stateaverage Fermi surface leads to the LOFF state
0q 0q
phase diagram of pion superfluidphase diagram of pion superfluid
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3535
BCS-BEC crossover of pion superfluidBCS-BEC crossover of pion superfluid
( , ) 2 Im ( , )k D k meson spectra functionmeson spectra function
meson mass, Goldstone modemeson mass, Goldstone mode
phase diagramphase diagram
BEC BCS
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3636
BCS-BEC crossover in asymmetric nuclear matterBCS-BEC crossover in asymmetric nuclear matter
Mao, Huang, Zhuang, 2008Mao, Huang, Zhuang, 2008
★ ★ transition from BCS pairing to BEC in low-density asymmetric nuclear matter, transition from BCS pairing to BEC in low-density asymmetric nuclear matter, U. Lombardo, P. Nozières:PRC64, 064314 (2001)U. Lombardo, P. Nozières:PRC64, 064314 (2001)
★ ★ spatial structure of neutron Cooper pair in low density uniform matter, spatial structure of neutron Cooper pair in low density uniform matter, Masayuki Matsuo:PRC73, 044309 (2006)Masayuki Matsuo:PRC73, 044309 (2006)
★ ★ BCS-BEC crossover of neutron pairs in symmetric and asymmetric nuclear BCS-BEC crossover of neutron pairs in symmetric and asymmetric nuclear matters, matters, J. Margueron: arXiv:0710.4241J. Margueron: arXiv:0710.4241
asymmetric nuclear matter with both asymmetric nuclear matter with both npnp and and nnnn and and pp pp pairingspairings
considering density dependent Paris potential and considering density dependent Paris potential and nucleon massnucleon mass
there exists a strong there exists a strong Friedel oscillation in BCS Friedel oscillation in BCS region, and it is washed region, and it is washed away in BEC region. away in BEC region.
3
32
ip rd pr e p
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3737
near side correlation as a signature of sQGPnear side correlation as a signature of sQGPDD
we take drag coefficient to we take drag coefficient to be a parameter charactering be a parameter charactering the coupling strength the coupling strength
* * c quark motion in QGP:c quark motion in QGP:
* * QGP evolution: QGP evolution: ideal hydrodynamicsideal hydrodynamics
for strongly interacting quark-gluon plasma: for strongly interacting quark-gluon plasma: ● ● at RHIC, the back-to-back correlation is washed out.at RHIC, the back-to-back correlation is washed out.● ● at LHC, c quarks are fast thermalized, the strong at LHC, c quarks are fast thermalized, the strong flow push the D and Dbar to the near side!flow push the D and Dbar to the near side!
Zhu, Xu, Zhuang, PRL100, 152301(2008)Zhu, Xu, Zhuang, PRL100, 152301(2008)
large drag parameter is confirmed by R_AA and v_2 of large drag parameter is confirmed by R_AA and v_2 of non-photonic electrons non-photonic electrons (PHENEX, (PHENEX, 2007; Moore and Teaney, 2005; Horowitz, Gyulassy, 2007).2007; Moore and Teaney, 2005; Horowitz, Gyulassy, 2007).
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3838
conclusionsconclusions
* * BCS-BEC crossover is a general phenomena from cold atom gas BCS-BEC crossover is a general phenomena from cold atom gas to quark matter.to quark matter.
* * BCS-BEC crossover is closely related to QCD key problems: BCS-BEC crossover is closely related to QCD key problems: vacuum, color symmetry, chiral symmetry, isospin symmetry ……vacuum, color symmetry, chiral symmetry, isospin symmetry ……
* BCS-BEC crossover of color superconductivity and pion * BCS-BEC crossover of color superconductivity and pion superfluid is not induced by simply increasing the coupling superfluid is not induced by simply increasing the coupling constant of the attractive interaction but by changing the constant of the attractive interaction but by changing the corresponding charge number.corresponding charge number.
* * There are potential applications in heavy ion collisions (at There are potential applications in heavy ion collisions (at CSR/Lanzhou, FAIR/GSI and RHIC/BNL) and compact stars.CSR/Lanzhou, FAIR/GSI and RHIC/BNL) and compact stars.
thanks for your patience thanks for your patience
July, 2008 Summer School on Dense Matter and HI DubnaJuly, 2008 Summer School on Dense Matter and HI Dubna 3939