HIGHLIGHTS IN 2011 AT STAR & ALICE In-Kwon Yoo. Outline  STAR BES Results  BES runs and STAR general  Charged Meson   and   Freeze-out Conditions.

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Presentation transcript:

HIGHLIGHTS IN 2011 AT STAR & ALICE In-Kwon Yoo

Outline  STAR BES Results  BES runs and STAR general  Charged Meson   and   Freeze-out Conditions    Flow  E-by-E  ALICE Recent Results  ALICE general  Particle Production  RHIC vs. LHC  Freeze-out Volume  Particle Ratios  Flow  Jet Quenching  Miscellaneous.. 2 IKYoo for HIM

STAR BES  Beam Energy Scan  Signature of Onset  Critical Point  T-mB scan  Looking for  anomalies  testing theories  RHIC vs. LHC 3 IKYoo for HIM

4

PID at STAR 5 IKYoo for HIM

K/ , ,  vs. E CM 6  Excellent agreement with SPS results IKYoo for HIM

Freeze-Out Conditions 7  Statistical model fit to , K, p  Excellent agreements with pub.data  Clear centrality dependence of T IKYoo for HIM

  KK 8  R CP in E CM dependence   /K ratio vs. theories IKYoo for HIM

Flow (v 2 ) of Charged Hadrons 9 IKYoo for HIM

Integrated v 2 vs. E CM 10  BES results fill gap between NA49 and 200GeV/u IKYoo for HIM

Particle – Antiparticle v2 11 IKYoo for HIM

Particle – Antiparticle v2 12 IKYoo for HIM

v 2 /ncq scaling 13  ncq-scaling for all particles holds up to 7.7 GeV   -meson results deviates from others at 11.5 GeV IKYoo for HIM

K(p)/  E-by-E fluctuations 14   (p/  ): monotonic increase  s(K/p): almost constant ; disagree with NA49 IKYoo for HIM

15

16 IKYoo for HIM

ALICE Data 17 IKYoo for HIM

Particle Production in pp/PbPb 18 IKYoo for HIM

RHIC vs. LHC 19  The same experiment under vastly different conditions IKYoo for HIM

System-size dependence vs. Theories 20  identical variation of particle production with system-size at RHIC and LHC  Global features of the system : independent on collision Energy IKYoo for HIM

Freeze-out Volume : Source-size 21 IKYoo for HIM

Identified particle spectra 22  much harder spectra  inv.slope parameter  expanding T IKYoo for HIM

Particle Ratios vs. Thermal model 23 Similar temperature as at RHIC, T CH ~ 164MeV IKYoo for HIM

Elliptic flows 24 mass dependence due to the radial flow viscous hydro predictions describe the data similar to RHIC : hydro+UrQMD (rescattering) for antiproton IKYoo for HIM

Jet quenching 25 IKYoo for HIM

RAA in- vs. out-of-plane 26 IKYoo for HIM

Flavor dependence 27 IKYoo for HIM

Flavor dependence 28 IKYoo for HIM

J/Psi RAA 29 Contribution from B is not substracted ; Cold nuclear matter effect at RHIC vs. LHC ; needed IKYoo for HIM

UPC with ALICE 30 IKYoo for HIM

UPC with ALICE 31 IKYoo for HIM

UPC with ALICE 32 IKYoo for HIM

Anti-Alpha with ALICE 33 IKYoo for HIM

Conclusions and Outlook 34  Excellent agreements of STAR BES results with NA49  Scanning and Filling up the gap between SPS and RHIC  Even more strongly interacting matter at LHC than RHIC?  Rich data with high precisions and PID to be continued  pA program at LHC?  What to be expected at 5.5TeV in 2014? IKYoo for HIM