space-time evolution of bulk qcd matter at rhic

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Space-time Evolution of Space-time Evolution of Bulk QCD Matter at RHIC Bulk QCD Matter at RHIC June 7@RHIC AGS annual users’ meeting Chiho NONAKA Chiho NONAKA Nagoya University Nagoya University n collaboration with Steffen A. Bass (Duke University & RIKEN collaboration with Steffen A. Bass (Duke University & RIKEN Contents Contents Introduction Introduction Hydrodynamic models at RHIC Hydrodynamic models at RHIC Freezeout process, finite state interactions Freezeout process, finite state interactions 3D hydro+UrQMD 3D hydro+UrQMD Results Results Single particle spectra, reaction yinamics, elliptic flow Single particle spectra, reaction yinamics, elliptic flow Summary Summary

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Space-time Evolution of Bulk QCD Matter at RHIC. Chiho NONAKA Nagoya University. Contents Introduction Hydrodynamic models at RHIC Freezeout process, finite state interactions 3D hydro+UrQMD Results Single particle spectra, reaction yinamics, elliptic flow Summary. - PowerPoint PPT Presentation

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Page 1: Space-time  Evolution of  Bulk QCD Matter at RHIC

Space-time Evolution of Space-time Evolution of Bulk QCD Matter at RHICBulk QCD Matter at RHIC

June 7@RHIC AGS annual users’ meeting

Chiho NONAKAChiho NONAKANagoya UniversityNagoya University

In collaboration with Steffen A. Bass (Duke University & RIKEN BNL)In collaboration with Steffen A. Bass (Duke University & RIKEN BNL)

ContentsContents•IntroductionIntroduction

–Hydrodynamic models at RHICHydrodynamic models at RHIC–Freezeout process, finite state interactionsFreezeout process, finite state interactions

•3D hydro+UrQMD3D hydro+UrQMD•ResultsResults

–Single particle spectra, reaction yinamics, elliptic flowSingle particle spectra, reaction yinamics, elliptic flow•SummarySummary

Page 2: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Hydrodynamic Models at RHICHydrodynamic Models at RHIC Success of Perfect Hydrodynami

c Models at RHIC

– Single particle spectra Huovinen, Kolb, Heinz, Hirano, Teaney, Shuryak, Hama, Morita, …….

– Strong elliptic flow Strong coupled (correlated) QGP

at mid rapidityat mid rapidityHuovinen et.al, PLB503

Discrepancy at large : •Insufficient thermalization?•Viscosity effect?•Simple freezeout process?

•freezeoutfreezeout•viscosityviscosity

Hirano and Tsuda, PRC66

However….–Elliptic flow vs.

Page 3: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Freezeout processFreezeout process in Hydro in Hydro– Difference between chemical and   thermal freezeout

Heinz,NPA

Possible solutions:– Partial chemical equilibrium (PCE) Hirano, Kolb, Rapp– Hydro + Micro Model Bass, Dumitru, Teaney, Shuryak

1. Single freezeout temperature?

• chemical freezeoutchemical freezeout statistical modelstatistical model TTchch ~170 MeV ~170 MeV hadron ratiohadron ratio

• thermal freezeoutthermal freezeout hydro hydro TTff ~ 110~140 MeV ~ 110~140 MeV

Page 4: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Final State InteractionsFinal State Interactions

Thermal model T = 177 MeV = 29 MeV

UrQMD

2. In UrQMD final state interactions are included correctly.

Markert @QM2004

3D-Hydro +UrQMD

Page 5: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

– Hadron phase: viscosity effect– Freezeout process:

• Chemical freezeout & thermal freezeout• Final state interactions

3D-Hydro +UrQMD

Key:Bass and Dumitru, PRC61,064909(2000)Teaney et al, nucl-th/0110037

• Treatment of freezeout is determined by mean free path.• Brake up thermalization: viscosity effect

3D-Hydro + UrQMD Model3D-Hydro + UrQMD Model

Full 3-d Hydrodynamics

• EoS :1st order phase transition QGP + excluded volume model

Cooper-Fryeformula

UrQMD

t fm/c

final stateinteractions

Monte Carlo

Hadronization

TC TSWTC:critical temperature TSW: Hydro UrQMD

Page 6: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

3-D Hydrodynamic Model 3-D Hydrodynamic Model Relativistic hydrodynamic equation

– Baryon number conservation

Coordinates

Lagrangian hydrodynamics– Tracing the adiabatic path of each volume element– Effects of phase transition on observables– Computational time– Easy application to LHC

Algorithm– Focusing on the conservation law

Flux of fluid

nucleus nucleus

energy momentum tensor

Lagrangian hydrodynamics

Page 7: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

ParametersParameters Initial Conditions

– Energy density

– Baryon number density

– Parameters

– Flow

Switching temperature

ε(x,y,η ) =εmaxW (x,y;b)H(η )

nB (x,y,η ) = nBmaxW (x,y;b)H(η )

TSW=150 [MeV]

vT=0vL= Bjorken’s solution);

Different from Pure Hydro !0=0.5 =1.5εmax=40 GeV/fm3, nBmax=0.15 fm-3

0=0.6 fm/c

hydro Hydro+UrQMD

0(fm) 0.6 0.6

εmax(GeV/fm3) 55 40

nBmax(fm-3) 0.15 0.15

0, 0.5, 1.5 0.5, 1.5

•longitudinal directionlongitudinal direction •transverse planetransverse plane

Page 8: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

PPTT spectra spectra PT spectra at central collisions

Page 9: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

PPTT Spectra (Pure Hydro) Spectra (Pure Hydro)

Tf=110 MeVnormalization of p:ratio at TchemHeinz and Kolb, hep-ph/0204061

Page 10: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Rapidity DistributionRapidity Distribution Impact parameter dependence of rapidity distributions

Page 11: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Centrality DependenceCentrality Dependence Impact parameter dependence of PT

Page 12: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

PPT T Spectra for Strange ParticlesSpectra for Strange Particles

Normalization is perfect!Normalization is perfect!

Page 13: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Reaction Dynamics Reaction Dynamics At mid rapidity

decaydecay

•Slope becomes steeper

Page 14: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Final State Interactions Final State Interactions

p, : flatter, pion wind: small cross section

Page 15: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

<P<PTT> vs mass> vs mass At mid rapidity

Hydrodynamic expansionHydrodynamic expansionfinal state interactionfinal state interaction

Page 16: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Distribution of # of CollisionsDistribution of # of Collisions

•p, broad p ~ 10 times, ~ 7 times small cross section

Page 17: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Distribution of # of Collisions Distribution of # of Collisions

•plateau -3 < < 3•flavor difference

Page 18: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

ff Distribution Distribution

, K: peak ~ 19 fm• p, : peak ~ 22 fm• Multistrange particles small

•Species dependence•Broad distribution

Page 19: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

f f Distribution of MDistribution of M

•Final state interactions Duration of freezeout process

Page 20: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

ff Distribution of B Distribution of B

•Final state interactions Duration of freezeout process

Page 21: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Collision RateCollision Rate

•MM is dominant.

Page 22: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

vv22 in hadron phase ? in hadron phase ? Quark number scaling of v2

⎟⎠⎞⎜⎝

⎛≈ TTh P

nnP 1)( 22 vv

vv22: early stage : early stage of expansionof expansion

Page 23: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Reaction Dynamics in vReaction Dynamics in v2 2 II

Page 24: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

Reaction Dynamics in vReaction Dynamics in v22 II II

•Hydro+decayHydro+decay ~ Hydro@~ Hydro@TTSWSW

•vv22 grows in hadron grows in hadron phase a bit.phase a bit.•vv22 builds up in QGP builds up in QGP phase.phase.

Page 25: Space-time  Evolution of  Bulk QCD Matter at RHIC

Chiho NONAKA

RHIC & AGS annual users’ meeting

SummarySummary We present the 3-D hydrodynamic +cascade model 3-D Hydrodynamic Model

– Single particle distribution• Centrality dependence

– Elliptic flow– Low Tf : single spectra, elliptic flow, hadron ratios Necessity of improvement of freezeout process in Hydro

3-D Hydro + UrQMD – Single particle distribution

• Centrality dependence – Elliptic flow– Different initial conditions from pure Hydro– Hadron ratios Switching temperature from Hydro to UrQMD– Reaction dynamics in UrQMD

,small cross section, v2:improvement at forward/backward Work in progress

– EoS dependence: ex. lattice QCD– Switching temperature dependence