1 On viscosity of Quark Gluon Plasma Defu Hou CCNU, Wuhan RHIC-Star full TOF detector and related...

Preview:

Citation preview

1

On viscosity of Quark Gluon Plasma

Defu Hou

CCNU , Wuhan

RHIC-Star full TOF detector and related physics in China Hangzhou April 27-29

hou

2

Introduction and motivation Viscosity from Kubo formula Viscosity from kinetic theory (Boltzmann

Eq) Viscosity from AdS/CFT Summary

Outlines

3

QCD under extreme conditions

At very High T or density ( deconfined) High T (Early universe, heavy-ion collisions) High density matter ( in the core of neutron stars)

4

@ RHIC

Robust collective flows, well described by ideal hydro with Lattice-based EoS. This indicates very strong interaction even at early time => sQGP

sQGP seems to be the almost perfect fluid known /s>= .1-.2<<1

Motivations

Experiments aspect:

5

Study of dissipative effects on <vStudy of dissipative effects on <v22>>

How sensitive is elliptic flow to finite /s?

Z. Xu & C. Greiner, PRL 101(08)

Agreement for s=0.3 – 0.6 /s=0.15 – 0.08

Viscous Hydro Cascade (2<->2,2<->3)

P. Romatschke, PRL99 (07)

Dependence on relaxation time

II0 order expansion with green terms (D. Rischke)

6

Theoretic aspect:

• To calculate Trsp. Coefs. in FT in highly nontrivial

(nonperturbative ladder resummation) (c around 5)

• String theory method: AdS/CFT (D.Son et al 2003)

/s = 1/4

. Kinetic theory + uncertainty principle (Gyulassy)

7

Main obstacle for theory

QCD in nonperturbative regime (T~200Mev) Pertburb. Expansion of QCD is not well behaved for realistic T

For thermodyn.,one can use lattice and resummation techniques Kinetic coefficients are difficult to extract from lattice

8

y

v

A

F xx

Shear Viscosity

9

10

11

Viscosity from Kubo formula

12

Nonlinear Response

13

14

S. Jeon, PRD 52; Carrington, Hou, Kobes, PRD61

15

Carrington, Hou, Kobes, PRD64 (2001)

16

Hou, hep-ph/0501284

17

18

Viscosity from kinetics theory

19

20

21

Boltzmann Equation

Fluctuation of distribution (s: species)

Recast the Boltzmann equation

P.Arnold, G.D.Moore and G.Yaffe,

JHEP 0011(00)001

Viscosity of hot QCD at finite density

22

Shear viscosity

With a definition of inner product and expanded distribution functions,

where

23

Collision terms

Performing the integral over dk’ with the help of

Scattering amplitude

Distribution function term \chi term

24

Matrix Element

25

Variation method gives

Liu, Hou, Li EPJC 45(2006)

26

Computing transport coefficients from AdS/CFT

In the regime described by a gravity dual the correlator can be computed using AdS/CFT

27

AdS/CFT at finite temperature

Classical Supergravity on AdS-BH×S5

4dim. Large-Nc strongly coupledSU(Nc) N=4 SYM at finite temperature(in the deconfinement phase).

conjecture

=

Witten ‘98

28

Field Theory Gravity Theory=

Gauge TheoriesQCD

Quantum GravityString theory

the large N limitSupersymmetric Yang Mills

Gravitational theory in 10 dimensions

N large

Calculations Correlation functionsQuark-antiquark potential

Holography

29

AdS/CFT now being applied to RHIC physics

Viscosity, /s. EOS Jet quenching “Sound” waves Photon production Friction … Heavy quarkonium Hardron spectrum (ADS/QCD)

30

Universality of shear viscosity in the regime described by gravity duals

Graviton’s component obeys equation for a minimally coupled massless scalar. But then .

Since the entropy (density) is we get

D. Son, P. Kovtun, A.S., hep-th/0405231

31

Shear viscosity in SYM

Correction to : A.Buchel, J.Liu, A.S., hep-th/0406264

P.Arnold, G.Moore, L.Yaffe, 2001

32

A viscosity bound conjecture

P.Kovtun, D.Son, A.S., hep-th/0309213, hep-th/0405231

33

Universality of

Theorem:

For any thermal gauge theory (with zero chemicalpotential), the ratio of shear viscosity to entropy density is equal to in the regime describedby a corresponding dual gravity theory

Remark:

Gravity dual to QCD (if it exists at all) is currentlyunknown.

34

Possible Mechanisms for Low viscosity Large cross-section, strong coupling

Anomalous viscosity: turbulence

M. Asakawa, S.A. Bass, B.M., hep-ph/0603092, PRLSee Abe & Niu (1980) for effect in EM plasmas

35

Take moments of

with pz2( ) ( , , )r p p

p

pD p f r p t C f

t E

2

23

4

2

12

3

11

110

1 ln 1mc

c A C

g gO

T

g BNO

N sT

M. Asakawa, S.A. Bass, B.M., hep-ph/0603092

See Abe & Niu (1980) for effect in EM plasmas

36

Low viscosity due to Anderson Local. AL effect renders infinite reduces viscosity

significantly even at weak coupling

Mechanism:coherent backscattering (CBS) effect

Ginaaki, Hou , Ren PRD 77(2008)

37

Summary

Kubo formula: via correlation functions of currents

Transport theory: Boltzmann Eqs. (for weak scattering)

ADS/CFT(strongly coupled) Lattice calculation (noisy)

Approches to calculate viscosity

38

Thanks

39

Renormalized diffusion

40

Weak Localization (WL)

Anderson proposed (‘58) that electronic diffusion can vanish in a random potential (AL)

Experiments detected ( Ishimaru 1984,Wolf Maret 1985) Mechanism:coherent backscattering (CBS) effect

after a wave is multiply scattered many times , its phase coherence is preserved in the backscattering direction , the probability of back scattering is enhenced via constructive interference

41

Viscosity with random mediumSystem: quasi-particles in random potential

Candidate disorder in sQGP ?1. The islands of heavy state; bound states

(Shuryak); 2. The reminiscent of confinement vaccum,

say the domain structure of 't Hooft's monopole condensation;

3. The disoriented chiral condensate (DCC);4. CGC

42

43

Response function

44

BS Eq. In Diagrams

45

Localization length

Itinerant states ---- Localized States

46

II Some applications to N=4 SUSY YM Plasma:

Equation of state in strong coupling: Plasma temperature = Hawking temperature

22

222

22

2

14

1 )1(

xdz

dtz

dds

zz

hh

h

Near Schwarzschild horizon

Continuating to Euclidean time, it

hhh zd

zd

zdds

2 , scoordinatepolar 2d

14 22

222

22 x

To avoid a conic singularity at 0 , the period of hz

Recalling the Matsubara formulation

hzT

1

47

Free energy = temperature X (the gravity action without metric fluctuations) E. Witten, Adv. Theor. Math. Phys. 2, 505 (1998), hep-th/9803131.

Consider a 4D Euclidean space of spatial volume V_3 atThe EH action of AdS-Schwarzschild:

z

44

5

3

053

5

11

8)1220(

16

10

h

z

EH zG

V

z

dzdtV

GI

h

The EH action of plain AdS

4

5

3

053

5

)0( 1

8)1220(

16

10

G

V

z

dzdtV

GI EH

----- To eliminate the conic singularity,----- To match the proper length in Euclidean time

nz

00 2

1 )0(4

4

GHGHh

IIz

f

Plasma free energy:

342

2

45

3)0(

0 81600lim

1VTN

zG

VIIF c

hEHEH

Plasma entropy:

332

2

23

VTNT

FS c

V

48

Bekenstein-Hawking entropy:

8

areahorizon

4

1unitsPlanck in measured area)(horizon

4

1

PBH l

S

8

1

length Planck d10 where GlP

------ The metric on the horizon :

3365

33

25

22

2

) of angle solid the( areahorizon The

1

VTSz

V

ddz

ds

h

h

x

------ The gravitational constant of the dual: 2

48

10 2 cP N

lG

plasmacBH SVTNS 3322

2

1

agree with the entropy extraced from the gravity action.

Gubser, Klebanov & Pest, PRD54, 3915 (1996)

49

The ratio 3/4:

The plasma entropy density at and cN322

3 2

1/ TNVSs c

The free field limit:

322322

30

7

240

78 TNTN cc

the contents of N=4 SUSY YM number entropy density

gauge potential 1

real scalars 6

Weyl spinors 4

322322

5

1

30

16 TNTN cc

322

30

1TN c

222)0(

3

2TNs c

The lattice QCD yields

75.04

3)0(

s

s

.8.00

s

s

50

Shear viscosity in strong coupling:

Kubo formula

Policastro, Son and Starinets, JHEP09, 043 (2002)

where

)0(),()(),(

)0,(Im1

lim

,

,0

xyxyxitiR

xyxy

Rxyxy

TxTtedtdG

G

qxq

51

Gravity dual: the coefficient of term of the gravity action

2xyh

22

2222

2

4

1du

fudfdt

u

Tds x

10 1 22

2

uufz

zu

h

52

The metric fluctuation

Substituting into Einstein equation

04 gR and linearize

The Laplace equation of a scalar field

dxdxuzthdu

fudfdt

u

Tds ),,(

4

1 22

2222

2 x

xyxy h

T

uh

xg

xg 22 where 0

1

53

Calculation details:

zyxjiuuf

f

f

f

ufTuT

ijiuj

tut

uuuij

uij

utt

,,, 2

1

1

2

1

2

2

1 2 12 22422

------ Nonzero components of the Christofel (up to symmetris):

fuR

u

TRf

u

TR uuijijtt 2

2222 1

4

4

------ Nonzero components of the Ricci tensor:

uyxu

xyuz

yxz

xyz

yxt

xyt

uuxyz

zxy

txy ufT

f

,2

1 ,

2

1

2

1

,2 ,2

1

2

1

:)symmetries to(up components nonzero with

22

Linear expansion:

4,2,2

1

component nonzeroonly the with

32

uzzyx

u

f

uuu

f

u

Tr

rRR

x

ggxgu

f

uuu

f

u

Thr uzzy

xy

x

2

1,2,

2

14 3

2

54

The solution:

Heun equation (Fucks equation of 4 canonical singularities)------trivial when energy and momentum equatl to zero;------low energy-momentum solution can be obtained perturbatively.

The boundary condition at horizon: 1u

correlator advanced waveoutgoing )-(1

correlator retarded waveincoming )1(~),,(

)(ˆ

2

)(ˆ

2

tqzii

tqzii

eu

euuzt

The incoming solution at low energy and zero momentum:

tii

eOu

iuuzt

)ˆ(

2

1ln

2

ˆ1)1(),,( 2

ˆ2

T

qq

Teuuuuzt tqzi

i

2ˆ where)()1()1(),,( )(

ˆ2

2

04

ˆˆ

2

1ˆˆˆ11ˆ)1(1)1(

2222

2

22

uii

qdu

duiui

du

duu

55

32, 8

)0,( TNi

G cR

xyxy

32

8

1TN c

Viscosity ratio: 08.04

1

s

Elliptic flow of RHIC:

Lattice QCD: noisy

1.0s

V_4 = 4d spacetime volume

)0,(2

1

16

lim8

1

8

1

)()( of termquadratic The

,432

4

0422

4

1

0

24422

Rxyxyc

ucc

GHEH

GVTNVi

uu

fTNV

uu

fxdduTN

II

56

III. Remarks:N=4 SYM is not QCD, since1). It is supersymmetric2). It is conformal ( no confinement )3). No fundamental quarks---- 1) and 2) may not be serious issues since sQGP is in the deconfined phase at a nonzero temperature. The supersymmetry of N=4 SYM is broken at a nonzero T.---- 3) may be improved, since heavy fundamental quarks may be introduced by adding D7 branes. ( Krach & Katz)

Introducing an infrared cutoff ---- AdS/QCD:

2222

2

2

4

5

1

fielddilaton thewhere

1216

1

dzddtz

ds

cz

RegxddzG

I EH

x

----- Regge behavior of meson spectrum ---- confinement;----- Rho messon mass gives ----- Lack of string theory support.

MeV; 338c

Karch, Katz, Son & Stephenov

57

Deconfinement phase transition: Herzog, PRL98, 091601 (2007)

Hadronic phase:

Plasma phase:

2222

2

4

5hadronic

1with

1216

1 2

dzddtz

ds

RegxddzG

I czEH

x

dzzTddtzTz

ds

RegxddzG

I czEH

1444224442

2

4

5plasma

111

with

1216

1 2

x

Hawking-Page transition:

---- First order transition with entropy jump

MeV1914917.0

plasmahadronic

cT

II

c

EHEH

2cN

---- Consistent with large N_c QCD because of the liberation of quark-gluon degrees of freedom.

58

59

60

61

Epilogue

AdS/CFT gives insights into physics of thermal gauge theories in the nonperturbative regime

Generic hydrodynamic predictions can be used to check validity of AdS/CFT

General algorithm exists to compute transport coefficients and the speed of sound in any gravity dual

Model-independent statements can presumably be checked experimentally

62

63

64

Mechanisms for Low viscosity Large cross-section, strong coupling

Anomalous viscosity: turbulence

Soft color fields generate anomalous transport coefficients, which may give the medium the character of a nearly perfect fluid even at moderately weak coupling

M. Asakawa, S.A. Bass, B.M., hep-ph/0603092, PRLSee Abe & Niu (1980) for effect in EM plasmas

Recommended