overview of hot and dense qcd matter

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Overview of hot and dense QCD matter Jean-Paul Blaizot, IPhT- Saclay Strongly Interacting Matter under Extreme Conditions Hirschegg January 18, 2010

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Page 1: Overview of hot and dense QCD matter

Overview of hot and dense QCD matter

Jean-Paul Blaizot, IPhT- Saclay

Strongly Interacting Matterunder Extreme Conditions

Hirschegg

January 18, 2010

Page 2: Overview of hot and dense QCD matter

T

µB

Hadronic matter

Quark-Gluon Plasma

Color superconductor

The QCD phase diagram (« low resolution »)

Page 3: Overview of hot and dense QCD matter

The Ideal baryonlessQuark-Gluon Plasma

Page 4: Overview of hot and dense QCD matter

Asymptotic freedom

Matter is « simple » at high temperature:

- an ideal gas of quarks and gluons

- the dominant effect of interactions is to turn

(massless) quarks and gluons into weakly interacting (massive) quasiparticles.

! s =g2

4"#

2"

b0ln µ / $QCD( )

µ ! 2"T( )

Page 5: Overview of hot and dense QCD matter

Phase transition(s)(crossover)

(from Z. Fodor,

arXiv:0711.0336)

(from M. Bazavov et al, arXiv:0903.4379)

Page 6: Overview of hot and dense QCD matter

(SU(3) lattice gauge calculation from Karsch et al, hep-lat/0106019)

At T>3Tc Resummed Pert. Theory accounts for lattice results

Resummed Pert. Th.SB

Pressure

(resummed pert. th. from J.-P. B., E. Iancu, A. Rebhan: Nucl.Phys.A698:404-407,2002)

Page 7: Overview of hot and dense QCD matter

Pressure for SU(3) YM theory at (very) high temperature

(from G. Endrodi et al, arXiv: 0710.4197)

Page 8: Overview of hot and dense QCD matter

Conserved charge susceptibilities

(from M. Cheng et al, arXiv: 0811.1006)

Page 9: Overview of hot and dense QCD matter

From the « ideal gas »

to the « perfect liquid »

Lessons from RHIC

Page 10: Overview of hot and dense QCD matter

(STAR: Phys.Rev.Lett.91:072304,2003)

Matter is opaque to the propagation of jets

Page 11: Overview of hot and dense QCD matter

(from Akiba et al, NPA 774 (2006) 403)

pp

AuAubinaryAuAu

AAYield

NYieldR

/ !"=

Page 12: Overview of hot and dense QCD matter

Initial momentumdistribution isotropic

Without interactions, the particleswould escape isotropically, irrespectiveof the shape of the interaction zone

Strong interactions induce pressure gradients. The expansion becomes anisotropic, and the momentum distribution reflects the anisotropy of the initial interaction region

Matter flows like a fluid

Page 13: Overview of hot and dense QCD matter

Elliptic flow

(Quark-Matter 02)

(Quark Matter 09)

Page 14: Overview of hot and dense QCD matter

(M. Luzum and P. Romatschke, arXiv: 0804.4015)

The low viscosity of the quark-gluon plasma

Page 15: Overview of hot and dense QCD matter

Low viscosity, phase transition and strong coupling

(from L. Csernai et al, nucl-th/0604032)

(from Z. Donko et al, arXiv: 0710.5229)

QGP Helium

Strongly correlated plasma

Also, cold fermionic gasat unitarity

Page 16: Overview of hot and dense QCD matter

Viscosity at weak and strong coupling

Page 17: Overview of hot and dense QCD matter

The Ideal strongly coupledQuark-Gluon Plasma

A new ‘reference’ system

Page 18: Overview of hot and dense QCD matter

New techniques (borrowed from string theory) allow calculationsin (some) strongly coupled gauge theories .

A theoretical breakthroughAdS/CFT Duality

Rely on a mapping between a strongly coupled gauge theory and a weakly coupled (i.e. classical) gravity theory.

New reference state: the strongly coupled quark-gluonplasma (instead of the weakly coupled one).New ideal system, allowing for many explicit calculations.

Page 19: Overview of hot and dense QCD matter

Some strong coupling results

Simple limit of the entropydensity at strong coupling

S

S0

=3

4+45

32!(3)

1

"3 / 2 ! " g2N

c( )

!

s=1

4"

Simple result for the viscosity

QCD

AdS/CFT

(G. Policastro et al, PRL87 (2001))

Page 20: Overview of hot and dense QCD matter

Weakly or stronglycoupled ?

A puzzling situation

Page 21: Overview of hot and dense QCD matter

Weakly AND strongly coupled …

In the qgp coexist degrees of freedom withdifferent wavelengths. Whether these degrees offreedom are weakly or strongly coupled dependson their wavelength.

Non perturbative features arise from the cooperation of many degrees of freedom, or strong classical fields. An example: the colorglass condensate.

Page 22: Overview of hot and dense QCD matter

High density partonic systems

Large occupation numbers

=> classical fields

Page 23: Overview of hot and dense QCD matter

Exploring the (µ,T) plane

Page 24: Overview of hot and dense QCD matter

T

µB

Hadronic matter

Quark-Gluon Plasma

Color superconductor

The QCD phase diagram(« low resolution »)

Page 25: Overview of hot and dense QCD matter

(from Ruester et al, PRD72 (2005))

A better resolution phase diagram (model dependent)

Speculation about new phases at high density

(from M. Stephanov)

Much uncertainty about theexistence and location of the critical point

(from R. Pisarski and L. McLerran)

Page 26: Overview of hot and dense QCD matter

(from J. Cleymans et al, hep-ph/0511094)

Matter at « freeze-out »

(from P. Braun-Munzinger et al)

well described by statistical picture

Page 27: Overview of hot and dense QCD matter

Conclusions

- ultra-relatvistic heavy ion collisions allow us to study fundamental questions concerning the phase diagram of hotand dense matter, or the nuclear wave functions at very high energy.

-exciting developments in recent years, many open questions/puzzles : phase diagram ? strongly/weakly coupled plasma ? detailed mechanisms leading tothermalisation and collective flow ? What can we learn from heavy quarks ?