su houng lee 1. quark condensate and the ’ mass 2. gluon condensate and the heavy quark system 3....
TRANSCRIPT
1
Su Houng Lee
1. Quark condensate and the h’ mass
2. Gluon condensate and the Heavy quark system
3. Summary
Medium dependence; are all hadrons alike?
2
1. Quark condensate and the h’ meson
1. Some introduction
2. Casher Banks formula
3. Lee-Hatsuda formula
4. Witten – Veneziano formula
5. At finite temperature and den-
sity
3
• Kapusta, Kharzeev, McLerran PRD 96 : Effective U(1)A restoration in medium in SPS data
Some introduction
• Rapp, Wambach, van Hees: SPS dilepton data
• RHIC dilepton puzzle
• Csorgo, Vertesi, Sziklai : Additional contribution from h’ mass reduction
• Experimental and theoretical works on h‘ in nuclear medium
• QCD symmetry: SU(N)Lx SU(N)R SU(N)V and U(1)A is always broken by Anomaly
QCD confinement
4
Finite temperature
T/Tc
/r rn
0/ TT qqqq
18.0/ 0 TT qqss
Tmmss ssT /exp
Quark condensate – Chiral order parameter
Finite density
Lattice gauge theory
Linear density approximation
2
12
1G
mcc
c
5
• Quark condensate
Casher Banks formula - Chiral symmetry breaking (m0)
0
10Tr)0,(Trlim00
0 mDdAexSqq QCDS
x
0 0001
0Tr00 022
m
m
md
mDqq
Phenomenologically need constituent quark mass
Casher Banks formula in the chiral limit
6
• Other order parameters: - s p correlator (mass difference)
),0( )0,( Tr xSxS
00, 00, 1 554 qiqxqixqqqxqxqxdV
aa
0 c 2
1 1
a5 a5
)0,0(Tr),(Tr SxxS
),0( )0,(Tr 55 xSixSi aa
Phenomenologically constituent quark mass terms survives
Generalized Casher Banks formula in the chiral limit
1 1
7
Correlation function for h ‘ (Lee, Hatsuda 96)
• h ‘- p correlator (mass difference)
00,00,1 55554 qiqxqixqqiqxqixqxedV
aaikx
),0()0,(Tr 55 xSixSi
3q
x SU(2)for const qqmq
nspermutatio 0 01
000
40000
4
ysmysydxuddxuxdV s
n=1
)0,0(Tr),(Tr 55 SixxSi
GG~
),0()0,(Tr 55 xSixSi aa
5i 5i
U(1) A symmetry will effectively be restored up to quark mass terms in SU(3)
20
T. Cohen (96)
Lee, Hatsuda (96)
8
• Contributions from glue only from low energy theorem
• When massless quarks are added
• Correlation function
h’ mass? Witten-Veneziano formula - I
0~
,~
e GGxGGdxikP ikx
000 kP
• Large Nc argument
mesons nglueballs n mk
mesonGG
mk
glueballGGkP
22
2
22
2|
~|0
|
~|0
00,e 055 kikx PkkjxjdxikP
GG~
GG~
GG~
GG~
cNOm
mk
GG 1 with
'|~
|02
'2'
2
2
2cN cN
• Need h‘ meson
2
'
2
0
'|~
|00)0(
m
GGPkP c
9
Witten-Veneziano formula – II
• h‘ meson 0
'|~
|002
'
2
Pm
GG
22
2'
2
'2
'
2
11
8
3
424
Gm
fmNNN
FF
MeV 432 11
8
3
2'
22
2'
2'
mG
NNfm F
MeV 411)547()958(' mm
Lee, Zahed (01)
10
• Large Nc counting
Witten-Veneziano formula in medium (Kwon, Morita, Wolf, Lee in prep )
m
ikx GGxGGdxikP 0~
,~
e
2cN
• LET (Novikov, Shifman, Vainshtein, Zhakarov) at finite temperature for S(k): Ellis, Kapusta, Tang (98)
2cN cN
0,e4/1
202
0
GGgxOpdxiOpgd
d ikx
d
T
d
d
TTcOpTc
bgMconstOp ''
8exp
020
2
0
0
22
20
3232
4/1 TTTOp
TTd
bOp
TTd
bOp
gd
d
11
• LET at finite temperature for P(k) : Lee, Zahed (01)
•
22
11
2
3
40 G
TTdkP
'|~
|0 GG
00,00,
2 55
2
4 qiqxqixqqiqxqixqN
Nxedkk
F
ikx
0 phase restored sym chiral
...0|
~|0
0~
,~
2'
2
24
4
mk
GGkGGxGGxedkP ikx
Therefore, 0'|~
|0 GG
12
• W-V formula at finite temperature:
22
11
2
3
4G
TTd
0
2442 GTagG
0'|
~|0
02'
2
Pm
GG
2'
2
m
0
22
22
11
2
3
4
11
2
3
4GdG
TTd
Smoothes out temperature change because if
Therefore , : Observable consequences ?qqm '
13
3. Heavy quark system
1. Charmonium system
2. Panda
14
rr
rrV s )(
3
4)(
)(GeV 2
small
r
b decdec /)0()( TTTT
dec/TT
T/Tc
sString Tension: QCD order pa-rameter
Early work on J/y at finite T (Hashimoto, Miyamura, Hirose, Kanki)
15
J/y suppression in RHIC
• Matsui and Satz: J/y will dissolve at Tc due to color screening
• Lattice MEM : Asakawa, Hatsuda, Karsch, Petreczky , Bielefield, Nonaka….
J/y will survive Tc and dissolve at 2 Tc .. Still not settled at QM2011
• Potential models (Wong …) : .
• Refined Potential models with lattice (Mocsy, Petreczky…)
: J/y will dissolve slightly above Tc
• Lattice after zero mode subtraction (WHOT-QCD)
: J/y wave function hardly changes at 2.3 Tc
• AdS/QCD (Kim, Lee, Fukushima, Stephanov…. ..) • NRQCD: UK group+ S.Y. Kim
• QCD sum rule (Morita, Lee) , QCD sum rule+ MEM (Gluber, Oka, Morita)
• Perturbative approaches: Blaizot et al… Imaginary potential• pNRQCD: N. Brambial et al.
Recent works on J/y in QGP
16
AdS/QCD (Y.Kim, J.P.Lee, SHLee 07)
J/y
y’
Deconfinement
Thermal effect?
Mass (GeV)
17
mqqS
1)( where,...........)()()()( qSGqSqSqSG
Perturbative treatment are possible
because
0for even qqm QCD
q
Heavy quark propagator
18
..)12(4
),(...)(
2222
21
0
n
n Gqxqm
xqFdxq
Perturbative treatment are possible when
222 4 QCDqm
2q
Two Heavy quark propagator
19
q2 process expansion parameter
example
0 Photo-production of open charm
m2J/ y
> 0 Bound state properties
Formalism by Peskin (79)
J/y dissociation: NLOJ/y mass shift: LO
-Q2 < 0 QCD sum rules for heavy quarks
Predicted mhc <mJ/y before experiment
Perturbative treatment are possible when 222 4 QCDqm
2
2
4mQCD
22
2
4 QmQCD
2/
2
2
4 J
QCD
mm
0/
2
2
J
QCD
mm
20
• At finite temperature: from
02 GG
• Two independent operators
Twist-2 Gluon
Gluon condensate
24
1GguuGGs
or
2E
2Bs
<a/p B2
>T
<a/p E2 >T
G0
G2
pGpG 20 ,3
9
8
400 MeV 18984
9B
GTG c
Lowest dimensional - Gluon operators
21
W(ST)=exp(-s ST)
Time
Space
Space
SW(S-T) = 1- <a/p E2> (ST)2 +
…
W(S-S) = 1- <a/p B2> (SS)2 +…
OPE for Wilson lines: Shifman NPB73 (80)
<E2>, <B2> vs confinement potential
• Local vs non local behavior
W(SS)= exp(-s SS)
T
• Behavior at T>Tc
W(SS)= exp(-s SS)
W(ST)= exp(- g(1/S) S)
<a/p B2
>T
<a/p E2 >T
22
NN
NN
N
mxdxxGmG
mGm
0.9 ),(2
MeV 750 N|(Chiral)T|N ,N|Op|N2
Op Op
22
000
• Linear density approximation
• Condensate at finite density
n.m.0
000 0.061-1
9
8
GmGG N
Tc
2
0
2
5
2 0.7 ..
GGGmn
• At r = 5 x r n.m.
167.0 2.0
167.0 2.0
2
2
s
s
B
E
9.02
sG
Operators in at finite density and hadronic phase
23
• Hatsuda, Adami, Brown.. (90)
....440
2 TagTGG
• Lattice calculation (Lee 89)
Non zero above Tc
Non-perturbative Gluon condensate ;
06.0 00 TGTG
<a/p B2
>T
<a/p E2 >T
Gluon condensate – Non perturbative
• Morita, Lee (08)
24
• In terms of density of eigenvalues
Gluon condensate – Non perturbative
dmm
md
mDhh m 1
0001
0Tr0022
2
12
1G
mm
25
• Morita and Lee (08 present)
In Vacuum
In medium
Heavy quark system – QCD sum rule constraints
,,,/ ccJ
4430,3872 ZX
26
qc
c
OPE for bound state: m infinity
)( || ),( 16/ 24220 mgOkmgOgNm c
Mass shift: QCD 2nd order Stark Effect : Peskin 79 e > L qcd
Medium
220
6
2/3
0
20
2
2
/
1
)1(9
128E
maxx
xdx
a
EE
nzEim
n niJ
Attractive for ground state
)1( ))()((
)(2244
3242 O
mgmgmg
mgmgg
c
c
c
c
=
<a/p B2
>T<a/p E2 >T
27
Summary of analysis • Due to the sudden change of condensate near Tc
<a/p B2
>T
<a/p E2 >T
G0
G2
• Abrupt changes for mass and width near Tc
(GeV)/Jm
28
0 50 100 150 200 250 300 350 4000
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
No. of participants
RAANuclear absorption &Thermal decay in QGP & HG
Recombination
Total
With g=1.85
Melting of y’ cc
Slope: GJ/yMelting T
of J/y
Height: mass of J/y
RAA from RHIC (√s=200 GeV y=0 , 2-comp model (Rapp) Song, Park, Lee 10)
29
Quantum numbers
QCD 2nd Stark eff.
Potential model
QCD sum rules
Effects of DD loop
hc0-+ –8 MeV –5 MeV
(Klingl, SHL ,Weise,
Morita)
No effect
J/y 1-- –8 MeV(Peskin, Luke)
-10 MeV(Brodsky et al).
–7 MeV(Klingl,
SHL ,Weise, Morita)
<2 MeV(SHL, Ko)
cc0,1,2++ -20 MeV -15 MeV
(Morita, Lee)
No effect on cc1
y(3686)
1-- -100 MeV(SHL, Ko)
< 30 MeV
y(3770)
1-- -140 MeV(SHL, Ko)
< 30 MeV
Other approaches for mass shift in nuclear matter
30
Anti pro-ton
4 to 6 GeV/ck
Heavy nuclei
3 2
11.2
0.17 5fm
fm fm
e
e
Observation of Dm through p-A reaction
Expected luminosity at GSI 2x 1032cm-2s-1
Can be done at J-PARC
31
1. h’ mass is related to quark condensate and thus should reduce in medium
a) Could serve as signature of chiral symmetry restoration
b) Dilepton in Heavy Ion collision
c) Measurements from nuclear targets
2. Heavy quark system - related to confinement phenomena
a) Refined measurements in Heavy Ion collisions
b) Measurements from nuclear target
Summary
32
• Other order parameters: - s p correlator (mass difference)
xmDmD
x1
001
Tr
00, 00, 1 554 qiqxqixqqqxqxqxdV
aa
0 c 2
a a
a5 a5
01
0Tr1
Tr mD
xmD
x
1
001
Tr 55
xmD
imD
xi aa