Strongly Interacting Low Viscosity Matter Created in Heavy Ion Collisions Joe Kapusta * University...
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Transcript of Strongly Interacting Low Viscosity Matter Created in Heavy Ion Collisions Joe Kapusta * University...
Strongly Interacting Low Viscosity Matter Created in Heavy Ion Collisions
Joe Kapusta*
University of Minnesota
Quark Matter 2006, Shanghai, China
* Original work done in collaboration with Laszlo Csernai and Larry McLerran.
The phase transition is 2nd
order for 2 massless flavorsand 1st order for 3, otherwisea rapid crossover.
Karsch, Laermann, Peikert
For realistic quark massesthere may be a line of 1st
order transition terminatingat a critical point.
de Forcrand, Philipsen
Big Experimental Motivation!PHENIX data + Huovinen et al. PHENIX: First Three Years of
Operation of RHIC
.correlated are and But fT T
Assume thermalization between 0.15 and 1 fm/c.
Agreement provides strong indication for early thermalization and collective flow.
Numerical Hydrodynamics(Huovinen, Kolb, Heinz, Hirano, Teaney, Shuryak, Hama, Morita, Nonaka, Bass)
Big Theoretical Motivation!
Viscosity in Strongly Interacting Quantum Field Theories from Black Hole Physics
Kovtun, Son, Starinets PRL 94, 111601 (2005)
Using the Kubo formula )0(),(1
lim20
1tracelesstraceless
4
0
ijijti TxTexd
the low energy absorption cross section for gravitons on blackholes, and the black hole entropy formula they found that
4/1/ s and conjectured that this is a universal lower bound.
Is the RHIC data, in the formof elliptic and radial flow,telling us that the matter hasvery small viscosity, a perfect fluid ?
Atomic and Molecular Systems
vTls free~
nl
1~freeIn classical transport theory and
so that as the density and/or cross section is reduced(dilute gas limit) the ratio gets larger.
In a liquid the particles are strongly correlated. Momentumtransport can be thought of as being carried by voids insteadof by particles (Enskog) and the ratio gets larger.
2D Yukawa Systemsin the Liquid State
radius Seitz-Wigner1
17parameter coupling Coulomb
at located Minimum
2
2
na
aT
Q
Applications to dusty-plasmas andmany other 2D condensed mattersystems.
Liu & Goree
QCD• Chiral perturbation theory at low T
(Prakash et al.): grows with decreasing T.
• Quark-gluon plasma at high T (Arnold, Moore, Yaffe): grows with increasing T.
4
4
16
15
T
f
s
)/42.2ln(
12.54 ggs
TT
TT
Tgln2ln
9
4ln
8
9
)(
1222
MeV 30T
QCDLow T (Prakash et al.)using experimentaldata for 2-bodyinteractions.
High T (Yaffe et al.)using perturbativeQCD.
η/s≈1/2 just above Tc
from lattice (Nakamura, Sakai)and classical quasiparticle model (Gelman, Shuryak, Zahed)
Large Nc Limit at Low T
• Baryon masses are proportional to Nc and can be neglected, meson masses are essentially independent of Nc. Hagedorn temperature and critical temperature should not change by much. Meson-meson cross sections scale as 1/ Nc
2, therefore η/s should scale as Nc
2 in the hadronic phase.
• From Yaffe et al. η/s = A/[(g2 Nc)2 ln(Bg2 Nc)] with A and B known constants, therefore η/s has a finite limit as Nc becomes large in the plasma phase.
• Implication: There is a jump in η/s of order Nc2 in going from the
low to the high temperature phases.
Huot,Jeon,Moore
Policastro,Son,Starinets & Buchel,Liu,Starinets
SYM •SYM has no running coupling and no phase transition•SYM has many more d.o.f. as scattering targets than QCD
BBB JunJ
TuuwPgT
QuHuHuHuuT 3
2
uTuTQuuguuH ,,
TuT
sus 1
22
22
32
2 kkk
kk
kiji
jj
i uTTT
uT
uuuT
s
Relativistic Dissipative Fluid Dynamics
In the Eckart approach u is the velocity of baryon number flow.
BBB JunJ
TuuwPgT
uHuuT 32
uTuTQuuguuH ,,
BBBB
B JT
susTw
TnJ
,
2
22
22
32
2 kkk
kk
kiji
jj
i uTTT
uT
uuuT
s
Relativistic Dissipative Fluid Dynamics
In the Landau-Lifshitz approach u is the velocity of energy transport.
How is this relevant for RHIC?
For baryon-free matter: transverse waves
sound waves
02 kiDt
0222 kiDv ls
TsD
TsD lt
3/4Momentum diffusion constants:
Bulk viscosity is generally small unless internal degreesof freedom (rotation, vibration) can easily be excited incollisions.
How is this relevant for RHIC?
• Solve relativistic viscous fluid equations, with appropriate initial conditions and with a hadron cascade afterburner, over a range of beam energies and nuclei and extract η(T)/s(T) from comparison with data.
• An analogous program was successful in obtaining information on the compressibility of nuclear matter and on the momentum-dependence of the nuclear mean-field at low beam energies.
m
TmT
1
03
2
Viscous Heating of Expanding Fireballs JK, PRC 24, 2545 (1981)
Viscosity smoothesout gradients intemperature, velocity, pressure,etc.
Extracting η/s from RHIC data
• Elliptic flow (Teaney,…)
• HBT (Teaney,…)
• Momentum spectra (Teaney, Baier & Romatschke,…)
• Momentum fluctuations (Gavin & Abdel-Aziz,…)
• Fluctuations in v2 (Csernai,…)
• Photon & dilepton spectra• Jet quenching
RHIC.at 5.01.0/at suggest th studiesy Preliminar s
Work in progress…and complications
• Numerical relativistic viscous fluid dynamics (Baier & Romatschke; Heinz & Song, Chaudhuri; Muronga &
Rischke) Large gradients (Baier & Romatschke) may require second-order Israel-Stewart equations (Muronga).
• Initial conditions (Lappi & Venugopalan CGC,…)
• Hadron afterburner (Hirano, Heinz, Kharzeev, Lacey, Nora; Bass & Nonaka)
• Turbulent plasmas (Asakawa, Bass, Muller) Charged particles scatter coherently from
dynamically generated color fields leading to “anomalous” viscosity.
Conclusion
• Hadron/quark-gluon matter should have a minimum at or near the critical or crossover point in the phase diagram analogous to atomic and molecular systems.
• Sufficiently detailed calculations and experiments ought to allow us to infer the viscosity/entropy ratio. This is an interesting dimensionless measure of dissipation relative to disorder.