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Hot and dense QCD matter APCTP-WCU Focus Program “From dense matter to campact stars in QCD and hQCD”, Pohang, May 2 4-June 4, 2010 Mei Huang IHEP, CAS TPCSF, CAS

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Page 1: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

Hot and dense QCD matter

APCTP-WCU Focus Program “From dense matter to campact stars in QCD and hQCD”, Pohang, May 24-June 4, 2010

Mei Huang IHEP, CAS

TPCSF, CAS

Page 2: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Content

I. QCD Phase structure chiral restoration & deconfinement phase transition

II. Locate CEP from viscosities shear viscosity/entropy density ratio

bulk viscosity/entropy density ratio

Page 3: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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I. QCD Phase Structure

Page 4: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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1974 ---- 1999 1999 ---- 2002

HM

QGP

CSCHM

QGP

Page 5: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Compact Star

sQGP E. Shuryak, I. Zahed

Pseudogap phase Hatsuda,Kunihiro

After 2003 High T part

Page 6: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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After 2003 High density part

Abuki-Baym-Hatsuda-Yamamoto, arXiv:1003.0408

Darmstadt and Frankfurt CSC group, Phys.Rev.D72:034004,2005

Many people contributed on the rich structure of CSC

APCTP focus program 2006

Page 7: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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After 2007: Chiral symmetric but confined phase

Quarkyonic and half-Skymion phase

L. McLerran, R. Pisarski

Phase diagram at large Nc Skymion crystal

See M. Rho’s talk

Page 8: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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HM

QGP

CSC

Can Quarkyonic phase be realized in real QCD phase diagram?

Fukushima, Hatsuda,arXiv:1005.4814

HM

QGP

CSC

Page 9: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Quarkyonic phase in PNJL model

Different choices of Polyakov potential: fixed by lattice QCD at finite T

Page 10: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

10Kenji Fukushima, arXiv:0803.3318

Page 11: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Quarkyonic phase in PLSM model

H. Mao, J. Jin, MH, arXiv:0906.1324

Page 12: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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In PNJL or PLSM model, at zero baryon density, whether chiral phase transition and deconfinement phase transition coincide or not depends much on parameters used.

In these models, there are no interplay between chiral phase transition and deconfinement phase transition.

Page 13: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Lattice results on Tc at zero mu

Chiral limit: coincide

Physical quark mass (2+1):

RBC-Bielefeld: coincide

Wuppertal-Budapest: (crossover feature)

Page 14: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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An equivalent order parameter for deconfinement phase transition:

Gattringer,PRL97(2006)032003Bilgici et.al. PRD77(2008)094007Braun, Hass,Marhauser,Pawlowski, arXiv:0908.0008

Order parameter of center symmetry

Confinement: center symmetry

Deconfinement:

center symmetry breaking

Page 15: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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The periodicity property of the quark fields change under the the gauge transformation Uz:

Dual observables:

Page 16: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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n=1: dressed Polyakov loop

Dual quark condensate:

order parameter of center symmetry

Dressed Polyakov loop in NJL model

Page 17: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Chiral limit: coincide

T.Mukherjee, H.Chen,M.Huang, arXiv:1005.2482

Page 18: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

18T.Mukherjee, H.Chen,M.Huang, arXiv:1005.2482

Physical quark mass:

crossover region

1st order:

Page 19: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Why for 1st and 2nd phase transition?

T.Mukherjee, H.Chen,M.Huang, arXiv:1005.2482

Page 20: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Why for crossover?

T.Mukherjee, H.Chen,M.Huang, arXiv:1005.2482

Page 21: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Mass effect

Nf=2+1 in NJL model is in progress

Page 22: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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II. Locate CEP by viscosities

shear viscosity/bulk viscosity

Page 23: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Relativistic Heavy Ion Collision

Discovery of “Perfect fluid” at RHIC

Hydrodynamics

???

Page 24: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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A little bit Hydrodynamics

Page 25: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Increase shear viscosity reduces elliptic flow!

P. Romatschke, U. Romatschke, nucl-th/0706.1522

Before 2003, people believed that de-confined QCD matter would be weakly coupled gas. Therefore, bulk viscosity is neglected, only consider shear viscosity corrections to the ideal hydro.

Page 26: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Discovery of sQGP at RHIC

Low shear viscosity

Page 27: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Handling strongly coupled system by using AdS/CFT

Minimum bound?

Page 28: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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sQGP: Most “perfect fluid” known

• Lattice: C0.13 0.03, at T=1.65 Ts

Nakamura-Sakai(2004)

Meyer (2007)

~ 10s

• Water

10.08

4s

Policastro, Son, and Starinets;Kovton, Son and Starinets; Buchel, J. Liu; Nakamura, Sin; Maeda, Natsuume, Okamura; ……

• N=4 SYM:

0.1 0.2s

• RHIC: Teaney (2003)

Romatschke-Romatschke (2007)

Page 29: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Interesting global feature of /s

Does /s make some sense?

Page 30: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Phys.Rev.Lett.97:152303,2006

Proposal:

Sufficient precise Experimental measurement of /s to pinpoint the location of phase transitions or crossover.

Empirical observation:

Page 31: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Lacey et al., PRL 98:092301,2007

Probe CEP by /s

Page 32: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Results from real scalar model

Yagi, Hatsuda, Miake, “Quark-Gluon Plasma”

Can /s characterize phase transitions?

Page 33: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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1, Minimum at Tc, most difficult condition for momentum transportation.

2. The value of /s at phase transition decreases with increases of coupling strength

J.W Chen, MH, Y.H. Li, E. Nakano, D.L.Yang, Phys.Lett.B670:18-21,2008, arXiv: 0709.3434

/s characterizes phase transitions CJT+Boltzmann Eq

Page 34: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

Dmitri Kharzeev, Kirill Tuchin arXiv:0705.4280 [hep-ph],F.Karsch, Dmitri Kharzeev, Kirill Tuchin arXiv:0711.0914 [hep-ph],Harvey Meyer arXiv:0710.3717 [hep-ph],

However: large bulk viscosity of QCD matter near phase transition

Pure gluodynamics 2-flavor case

Page 35: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

Bulk viscosity is related to nonconformality

Several quantities measure conformality

Page 36: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

LQCD results:

trace anomaly shows a sharp peak near phase transition

BNL-Columbia-RBRC-Bielefeld, arXiv:0710.0354 Bielefeld, hep-lat/9602007

Page 37: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

BNL-Columbia-RBRC-Bielefeld arXiv:0710.0354

LQCD results:

soft EOS & small sound velocity near phase transition

Page 38: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

Gubser et al, 0804.1950

AdS/CFT

Gravity duals, nonconformal

Bulk viscosity in gravity dual models

Page 39: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

Results from scalar model: 2nd order phase transition

Trace anomaly: height is DOF dependent

Baochun Li, Mei Huang, Phys.Rev.D78:117503,2008 arXiv: 0807.0292

Page 40: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

EOS & sound velocity

Baochun Li, Mei Huang, Phys.Rev.D78:117503,2008 arXiv: 0807.0292

Page 41: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

Bulk viscosity/entropy density

Baochun Li, Mei Huang, Phys.Rev.D78:117503,2008 arXiv: 0807.0292

Page 42: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Results from a more realistic model: PLSM model

H. Mao, J. Jin, M. Huang, arXiv: 0906.1324[hep-ph]

Comparing with LQCD

Page 43: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Sound velocity square at Tc: 0.05 in PLSM, 0.07 in LQCD

H. Mao, J. Jin, M. Huang, arXiv: 0906.1324[hep-ph]

Page 44: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Comparing with LQCD: Bulk viscosity/entropy density

H. Mao, J. Jin, M. Huang, arXiv: 0906.1324[hep-ph]

Page 45: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Dependence of bulk viscosity/entropy density on the order of phase transition: large for 1st order phase transition, small for crossover. Thus, bulk viscosity/entropy density is better than shear viscosity/entropy density to probe CEP.

H. Mao, J. Jin, M. Huang, arXiv: 0906.1324[hep-ph]

Page 46: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Shear viscosity: how much entropy is produced bytransformation of shape at constant volume

Bulk viscosity: how much entropy is produced bytransformation of volume at constant shape

Physical quantities related bulk viscosity

Generated bytranslations

Generated bydilatations

Page 47: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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Conclusion and discussion

1, Interplay between chiral phase transition and

deconfinement phase transition.

2, Locate CEP by bulk viscosity/entropy density

Observables related to bulk viscosity?

Radial flow?

Page 48: Hot and dense QCD matter APCTP-WCU Focus Program “ From dense matter to campact stars in QCD and hQCD ”, Pohang, May 24-June 4, 2010 Mei Huang IHEP, CAS

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What’s the effect of large bulk viscosity near Tc?

Breakdown of hydrodynamic picture

Slow down the expansion of the system

Clustering at hadroniztion

……

G.Torrieri, B.Tomasik, I.Mishustin, arXiv:0707.4405[hep-ph]

G.Torrieri, I.Mishustin, arXiv:0805.0422[hep-ph]

R.J.Fries, B.Muller,A.Schafer, arXiv:0807.4333[hep-ph]