Hadron Spectra in Au Au Collisions by STAR Experiment at RHIC

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Hadron Spectra in Au Au Collisions by STAR Experiment at RHIC

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Hadron Spectra in Au+Au Collisions by STAR Experiment at RHIC Masashi Kaneta for the STAR collaboration LBNL Introduction Study of bulk properties Macroscopic ... – PowerPoint PPT presentation

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Title: Hadron Spectra in Au Au Collisions by STAR Experiment at RHIC


1
Hadron Spectra in AuAu Collisions by STAR
Experiment at RHIC
  • Masashi Kaneta
  • for the STAR collaboration
  • LBNL

2
Introduction
  • Study of bulk properties
  • Macroscopic approach
  • Chemical freeze-out
  • Thermal freeze-out
  • Focusing on pT distribution
  • Thermal freeze-out Temperature
  • Transverse flow

Expansion Cooling
Time
3
RHIC-STAR experiment
  • Solenoidal Tracker At RHIC

40 Institutes/Universities 300 Collaborators
  • One of large experiments at RHIC
  • 2p acceptance
  • Excellent particle identification

4
STAR Event
Tracks are reconstructed by online tracking
5
Particle Identification
  • dE/dx by TPC p,K,p,d,He,
  • Kink method K
  • RICH 1-3 GeV/c for p/K, 1.5-5GeV/c for p
  • Topology L, X, W, K0s
  • Combinatrics D, L, L(1520), K, f,
  • TOF (year 2)
  • EMC (year 2)

p
K
dE/dx
p
e
p/Z GeV/c
6
pT Distribution / Kinetic Freeze-out
  • Kinetic freeze-out
  • End of elastic interactions
  • Information of momentum is frozen
  • Boltzmann distribution flow effect

Blast wave model E. Schnedermann et al.,
PRC48(1993)2462
Boosted
No Boost
7
pT distribution vs. Centrality
ltNpartgt for p 345?7 289?9 221?4 152?9 102?4
63?4 35?3 20?2 9?4 -------
ltNpartgt for K, p 345?7 280?9 235?8 180?9 135?8 100
?4 70?4 25?3
STAR Preliminary
K- (dE/dx)
K- (kink)
p
p
central peripheral
p-
K (kink)
K (dE/dx)
pT GeV/c
8
Centrality dependence of T th and ltbrgt
  • Selected similar centrality region in p and K,p

p-
K
K-
p
p
38 115 224 347 ltNpartgt
pT GeV/c
  • As a function of centrality
  • Tth 100 MeV
  • ltbrgt goes up then saturated
  • Flow profile changed?

9
Bombarding Energy Dependence
  • From SPS to RHIC
  • Increasing flow
  • Decreasing temperature
  • Longer time for cooling at RHIC?

STAR
PHENIX
10
Summary
  • The pT distributions of p, K, and p are obtained
    as a function of centrality from RHIC-STAR at
    ?sNN130GeV AuAu
  • The blast wave model describes the data over all
    of centrality
  • As a function of centrality at RHIC
  • Tth 100 MeV
  • ltbrgt goes up then saturated (0.55c)
  • Flow profile changed?
  • From SPS to RHIC
  • Increasing flow
  • Decreasing temperature
  • Indicating longer time for cooling at RHIC?

11
STAR vs. PHENIX
p-
  • PHENIX p and K show smaller yield at pTgt0.6 than
    STAR
  • upto factor of 2!!
  • Protons have coincidence

K-
K
p
p
12
Centrality
centrality bin for kink K
13
STAR Event
14
Test of Flow Profile
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