space time evolution of qcd matter

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Space time evolution of QCD matter Parton cascade with stochastic algorithm Transport rates and momentum isotropization Thermalization of gluons due to Results: bottom-up scenario, jet-quenching, elliptic flow, viscosity,… viscous hydro, I. Bouras, A. El, O. Fochler, F. Reining, Z. Xu, CG Johann Wolfgang Goethe-Universität Frankfurt Institut für Theoretische Physik Focus week, HIC at the LHC, CERN , may 2007

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Johann Wolfgang Goethe-Universität Frankfurt Institut für Theoretische Physik. Space time evolution of QCD matter. I. Bouras, A. El, O. Fochler, F. Reining, Z. Xu, CG. Focus week, HIC at the LHC, CERN , may 2007. Parton cascade with stochastic algorithm - PowerPoint PPT Presentation

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Page 1: Space time evolution of QCD matter

Space time evolution of QCD matter

• Parton cascade with stochastic algorithm

• Transport rates and momentum isotropization

• Thermalization of gluons due to

• Results: bottom-up scenario, jet-quenching,

elliptic flow, viscosity,… viscous hydro, …

I. Bouras, A. El, O. Fochler, F. Reining, Z. Xu, CG

Johann Wolfgang Goethe-Universität Frankfurt

Institut für Theoretische Physik

Focus week, HIC at the LHC, CERN , may 2007

Page 2: Space time evolution of QCD matter

Relativistic Quantum Transport for URHIC

• microscopic transport calculations of partonic degrees of freedom

RHIC, LHC

),(),(),( pxCpxCpxfp ggggggggg

new development

Z. Xu and C. Greiner, PRC 71, 064901 (2005)

Boltzmann Approach of MultiParton Scatterings (BAMPS)

LPM

DDggggg

mqkk

qg

mq

sgM

222

22

222

242

)(

12

)(2

9

3x

23321

3232

32323

32222

)(823

32

22

x

t

EEE

IPfor

x

tvPfor

x

tvPfor

rel

rel

collision probability

particle in cell method

Page 3: Space time evolution of QCD matter

LPM

DDggggg

Dgggg

mqkk

qg

mq

sgM

mq

sgM

222

22

222

242

222

242

)(

12

)(2

9

,)(2

9

J.F.Gunion, G.F.Bertsch, Phys. Rev. D 25, 746(1982)

parton scatterings in leading order pQCD

),3(16 1)2(

23

3

qfgppd

sD fnfm

screening mass:

LPM suppression: the formation time

)cosh( yk g

gk y

cosh1

)/ln()233(12

QCDf sns

Page 4: Space time evolution of QCD matter

MeVTfmgs 400~5.0~3.0~ fugacity ~ 0.5

Example

Page 5: Space time evolution of QCD matter

Important scales for kinetic transport & simulations

Simulations solve Boltzmann equation:→ test particles and other schemes

Semiclassical kinetic theory:

(Quantum mechanics: )

Page 6: Space time evolution of QCD matter

Initial production of partons

dt

dpxfxpxfxK

dydydp

d cdab

tbtadcbat

jet

),(),( 2

222

11,;,21

2

minijets

string matter

CGC

Page 7: Space time evolution of QCD matter

central

elliptic flow in noncentral Au+Au collisions at RHIC:

)(exp)()( 0

2

2

02

2

2

2

2

2

t

tt

E

pt

E

p

E

pt

E

peq

ZZeq

ZZ

fast isotropization and thermalisation

hydrodynamical evolution of momentum spectrum,… micr. determination of transport parameter …

Z. Xu and C. Greiner, hep-ph/0703233 Z. Xu and C. Greiner,

NPA 774, 787 (2006)

Page 8: Space time evolution of QCD matter

3+1dim. full cascade: comparison with RHIC data

Page 9: Space time evolution of QCD matter

5.

22

.32

.23 tr

trtr

R

RR

The drift term is large.

.

.32

.23

.22

trdrift

tr

tr

tr

R

R

R

R

ggggg interactions are essential for kinetic equilibration!

Z. Xu and C. Greiner, arXiv:hep-ph/0703233

trz

z

Rfvpd

fvEpdn

1

)(

)(

5

12

313

2313

Page 10: Space time evolution of QCD matter

transverse energy at y=0 in Au+Au central collision

Page 11: Space time evolution of QCD matter

Initial condition with Color Glass Condensate

: [-0.05:0.05] and xt < 1.5 fm

Page 12: Space time evolution of QCD matter

bottom-up scenario of thermalization

R.Baier, A.H.Mueller, D.Schiff and D.T.Son, PLB502(2001)51

• Qs-1 << t << -3/2 Qs

-1 Hard gluons with momenta about Qs are freedand phase space occupation becomes of order 1.

• -3/2 Qs-1 << t << -5/2 Qs

-1 (h+h h+h+s)Hard gluons still outnumber soft ones, but soft gluons give most of theDebye screening.

• -5/2 Qs-1 << t << -13/5 Qs

-1 (h+h h+h+s; s+s s+s; h+s sh+sh+s)Soft gluons strongly outnumber hard gluons.Hard gluons loose their entire energy to the thermal bath.

• After -13/5 Qs-1 the system is thermalized: T ~ t-1/3, T0 ~ 2/5 Qs

Page 13: Space time evolution of QCD matter

→ Particle number decreases in the very first moment→ No net soft gluon production at early times!

evolution of particle number in bottom-up scenario in 1+1 dim. geometry

Not the full Bottom-Up story...

LHC …

RHIC

Page 14: Space time evolution of QCD matter

Evolution of temperature and spectrum … Andrej El

Page 15: Space time evolution of QCD matter

extracting the viscosity

preliminary

Bjorken geometry:

Page 16: Space time evolution of QCD matter

Jet-Quenching in a central Au Au collision at RHIC

Oliver Fochler

RAA higher?

RAA ~ 0.04–0.05

old:

new:preliminary

quarks not yet included …

Page 17: Space time evolution of QCD matter

Summary

• A new parton cascade including inelastic multiparton scatterings gg↔ggg

• Explains thermalization and hydrodynamical expansion at RHIC

• PQCD inspired gg↔ggg are important for the thermalization.

• PQCD gg↔ggg generate the elliptic flow in noncentral collisions.

• Not full bottom-up thermalization scenario with CGC

• 3~4 too much jet-quenching

Outlook

• viscosity

• including quarks, heavy quark production

• Test for initial conditions (boundaries)

Page 18: Space time evolution of QCD matter

possible Chromo/Weibel instabilities

B.Schenke, A. Dumitru, Y. Nara, M. Strickland

Page 19: Space time evolution of QCD matter

Initial conditions: minijets production with pt > p0

dcba

cdab

TbTa

T

jet

td

dpxfxpxfxK

dydydp

d

,;,

2

22

2

11

21

2 ˆ),(),(

ppjetAA

AAjet bTN )0(2 binary approximation

830gN for a central Au+Au collision at RHICat 200 AGeV using p0=2 GeV

Page 20: Space time evolution of QCD matter

rapidity distributionResults

Page 21: Space time evolution of QCD matter

the central region:: [-0.5:0.5] and xt < 1.5 fm

thermalization and hydrodynamical behavior

NO thermalization and free streaming

including ggggg without ggggg

Page 22: Space time evolution of QCD matter

cmt d 2sin

transport cross section:

Why fast thermalization?

gg gg

gg ggg

2

gggg

gggggBUT! This is not the whole story...

… transport rates !

Page 23: Space time evolution of QCD matter

0

2

2

02

2

2

2

2

2

exp)()(tt

E

pt

E

p

E

pt

E

peq

ZZeq

ZZ

(t) gives the timescale of kinetic equilibration.

,/ 22 EPQ Z

),,(

),,(

3

3

3

3

)2(

)2(

txpf

QtxpfQ

pd

pd

t

fpdtfpd tQ

nQ

ntQ 3

3

3

3

)2()2()(

11)(

322322 IIIfE

P

t

f

322322)( CCCCtQ drift

,1 .

32.

23.

22. trtrtrtr

drift RRRR

)(

)(

tQQ

tQ

eq

Page 24: Space time evolution of QCD matter

special case )()(),( EpEppxf ZZ

.23

.23

.22

.22 2

3

2

3,

2

3 trrel

trtrrel

tr vnRvnR

for isotropic distribution of collision angle

32.

3223.

2322.

22 3

2,

2

3, RRRRRR trtrtr

cmt d 2sin

Page 25: Space time evolution of QCD matter

momentum isotropization and kinetic equilibration

Initial condition: Minijets p0=1.4 GeV

Page 26: Space time evolution of QCD matter

Important scales for kinetic transport & simulations

Simulations solve Boltzmann equation:→ test particles and other schemes

Semiclassical kinetic theory:

(Quantum mechanics: )

Page 27: Space time evolution of QCD matter

E

dmfp

... kinetic transport still valid

Page 28: Space time evolution of QCD matter

Thermalization times: comparison with bottom-up prediction

• 1/Qs behavior seems to be correct.

• instead -13/5 behavior but -x with x < 13/5

Page 29: Space time evolution of QCD matter

Jet-Quenching Box calculation: T=400MeV

Oliver Fochler

dominant process is 2->3

Page 30: Space time evolution of QCD matter

LPM

DDggggg

mqkk

qg

mq

sgM

222

22

222

242

)(

12

)(2

9

Bremsstrahlung processes

LPM suppression: the formation time

)cosh( yk gLPM

gk y

cosh1

Bethe-Heitler regime

varying the cut-off for kT: )cosh( yAk gLPM

Page 31: Space time evolution of QCD matter
Page 32: Space time evolution of QCD matter