Starting the Energy Scan - First Results from 62

Slides:



Advertisements
Similar presentations
Quark Matter 2006 ( ) Excitation functions of baryon anomaly and freeze-out properties at RHIC-PHENIX Tatsuya Chujo (University of Tsukuba) for.
Advertisements

Identified particle transverse momentum distributions in 200 GeV Au+Au collisions at RHIC 刘海东 中国科技大学.
ICPAQGP, Kolkata, February 2-6, 2015 Itzhak Tserruya PHENIX highlights.
Centrality-dependent pt spectra of Direct photons at RHIC F.M. Liu 刘复明 Central China Normal University, China T. Hirano University of Tokyo, Japan K.Werner.
5-12 April 2008 Winter Workshop on Nuclear Dynamics STAR Particle production at RHIC Aneta Iordanova for the STAR collaboration.
Helen Caines Yale University SQM – L.A.– March 2006 Using strange hadron yields as probes of dense matter. Outline Can we use thermal models to describe.
Identified and Inclusive Charged Hadron Spectra from PHENIX Carla M Vale Iowa State University for the PHENIX Collaboration WWND, March
12-17 February 2007 Winter Workshop on Nuclear Dynamics STAR identified particle measurements at large transverse momenta in Cu+Cu collisions at RHIC Richard.
Strange and Charm Probes of Hadronization of Bulk Matter at RHIC International Symposium on Multi-Particle Dynamics Aug 9-15, 2005 Huan Zhong Huang University.
Identified Particle Ratios at large p T in Au+Au collisions at  s NN = 200 GeV Matthew A. C. Lamont for the STAR Collaboration - Talk Outline - Physics.
QM2006 Shanghai, China 1 High-p T Identified Hadron Production in Au+Au and Cu+Cu Collisions at RHIC-PHENIX Masahiro Konno (Univ. of Tsukuba) for the PHENIX.
Spectra Physics at RHIC : Highlights from 200 GeV data Manuel Calderón de la Barca Sánchez ISMD ‘02, Alushta, Ukraine Sep 9, 2002.
QM’05 Budapest, HungaryHiroshi Masui (Univ. of Tsukuba) 1 Anisotropic Flow in  s NN = 200 GeV Cu+Cu and Au+Au collisions at RHIC - PHENIX Hiroshi Masui.
1 Nov. 15 QM2006 Shanghai J.H. Lee (BNL) Nuclear Induced Particle Suppression at Large-x F at RHIC J.H. Lee Physics Department Brookhaven National Laboratory.
Hard vs. Soft Physics at RHIC - Insights from PHENIX l Why hard vs. soft? l Soft physics: thermal, flow effects l Hard processes at RHIC l Conclusion Barbara.
20 Nov 2006, Quark Matter, Shanghai, ChinaShinIchi Esumi, Univ. of Tsukuba1 Rapporteur 3 Bulk Properties and Collective Phenomena ShinIchi Esumi Univ.
Charged Hadron Nuclear Modification Factors in the Beam Energy Scan data from STAR Stephen Horvat for the STAR collaboration Yale University Stephen HorvatCPOD.
1 Jeffery T. Mitchell – Quark Matter /17/12 The RHIC Beam Energy Scan Program: Results from the PHENIX Experiment Jeffery T. Mitchell Brookhaven.
Energy Scan of Hadron (  0 ) Suppression and Flow in Au+Au Collisions at PHENIX Norbert Novitzky for PHENIX collaboration University of Jyväskylä, Finland.
Hadron Collider Physics 2012, 12/Nov/2012, KyotoShinIchi Esumi, Univ. of Tsukuba1 Heavy Ion results from RHIC-BNL ShinIchi Esumi Univ. of Tsukuba Contents.
Presentation for NFR - October 19, Trine S.Tveter Recent results from RHIC Systems studied so far at RHIC: - s NN 1/2 = 
Masashi Kaneta, First joint Meeting of the Nuclear Physics Divisions of APS and JPS 1 / Masashi Kaneta LBNL
Robert Pak (BNL) 2012 RHIC & AGS Annual Users' Meeting 0 Energy Ro Robert Pak for PHENIX Collaboration.
1 Fukutaro Kajihara (CNS, University of Tokyo) for the PHENIX Collaboration Heavy Quark Measurement by Single Electrons in the PHENIX Experiment.
Roy A. Lacey, Stony Brook, ISMD, Kromĕříž, Roy A. Lacey What do we learn from Correlation measurements at RHIC.
Christina Markert Hot Quarks, Sardinia, Mai Christina Markert Kent State University Motivation Resonance in hadronic phase Time R AA and R dAu Elliptic.
24 Nov 2006 Kentaro MIKI University of Tsukuba “electron / photon flow” Elliptic flow measurement of direct photon in √s NN =200GeV Au+Au collisions at.
Systematic Study of Elliptic Flow at RHIC Maya SHIMOMURA University of Tsukuba ATHIC 2008 University of Tsukuba, Japan October 13-15, 2008.
Measurement of Azimuthal Anisotropy for High p T Charged Hadrons at RHIC-PHENIX The azimuthal anisotropy of particle production in non-central collisions.
Kirill Filimonov, ISMD 2002, Alushta 1 Kirill Filimonov Lawrence Berkeley National Laboratory Anisotropy and high p T hadrons in Au+Au collisions at RHIC.
Japanese Physics Society meeting, Hokkaido Univ. 23/Sep/2007, JPS meeting, Sapporo, JapanShinIchi Esumi, Inst. of Physics, Univ. of Tsukuba1 Collective.
Intermediate pT results in STAR Camelia Mironov Kent State University 2004 RHIC & AGS Annual Users' Meeting Workshop on Strangeness and Exotica at RHIC.
Hadron Spectra and Yields Experimental Overview Julia Velkovska INT/RHIC Winter Workshop, Dec 13-15, 2002.
Hard vs. Soft Physics at RHIC - Insights from PHENIX l Why hard vs. soft? l Soft physics: thermal, flow effects l Hard processes at RHIC l Conclusion Barbara.
Experiment Review in small system collectivity and thermalization in pp, pA/dA/HeA collisions Shengli Huang.
Proving Quark Gluon Plasma via Baryon Production at RHIC
A few observations on strangeness production at SPS and RHIC
High-pT Identified Hadron Production in Au+Au and Cu+Cu Collisions
Strangeness Production in Heavy-Ion Collisions at STAR
Bulk Properties and Collective Phenomena
Collective Dynamics at RHIC
Maya SHIMOMURA University of Tsukuba for the PHENIX Collaboration
Experimental Studies of Quark Gluon Plasma at RHIC
Tatsuya Chujo for the PHENIX collaboration
Outline First of all, there’s too much data!! BRAHMS PHOBOS PHENIX
Yields & elliptic flow of and in Au+Au collisions at
ISMD ‘02, Alushta, Ukraine Sep 9, 2002
Hadron Suppression and Nuclear kT Enhancement Studied with Neutral Pions from p+C, p+Pb, and Pb+Pb Collisions at sNN = 17.3 GeV Quark Matter 2006.
Tatsuya Chujo University of Tsukuba (for the PHENIX Collaboration)
Many Thanks to Organizers!
Xiaobin Wang (for the STAR Collaboration)
Scaling Properties of Identified Hadron Transverse Momentum Spectra
Flow Measurement in PHENIX
High-pT Identified Charged Hadrons in √sNN = 200 GeV Au+Au Collisions
Identified Charged Hadron
Cronin Effect of  K p from d+Au Collisions at 200 GeV
System Size and Energy Dependence of -meson Production at RHIC
Search for the onset of baryon anomaly at RHIC-PHENIX
Identified Charged Hadron Production
ShinIchi Esumi, Univ. of Tsukuba
Hiroshi Masui for the PHENIX collaboration August 5, 2005
Identified Charged Hadron Production at High pT
First Hints for Jet Quenching at RHIC
ShinIchi Esumi, Univ. of Tsukuba
What have we learned from Anisotropic Flow at RHIC ?
Masahiro Konno (Univ. of Tsukuba) for the PHENIX Collaboration Contact
Identified Particle Production at High Transverse Momentum at RHIC
Hiroshi Masui / Univ. of Tsukuba
QGP Formation Signals and Quark Recombination Model
Volume effects on strangeness production
Presentation transcript:

Starting the Energy Scan - First Results from 62 Starting the Energy Scan - First Results from 62.4 GeV Au+Au Collisions Introduction. High pT. Bulk matter observations. Collective motion. Summary

The story so far. We have discovered a strongly interacting medium with extremely high energy density which cannot be described in terms of simple hadronic degrees of freedom. Phobos

Nuclear modification factor at 200 GeV Charged Hadrons d2N/dpTd (Au+Au) RAA = NColld2N/dpTd (p+p) High pT suppression and loss of back-to-back signal in Au+Au but not in d+Au showed that effect due to Jet Quenching in final state NOT initial state parton saturation (GCG). BRAHMS Can we turn this effect off? Observed by all 4 experiments

Need for an energy scan Varying the beam energy changes: Initial state: sNN, Nbin/Npart, Qs(?) System: , mB, Nch Partonic: xT, dE/dx Varying the beam energy changes: Provide constraints on jet quenching models. Study the excitation function of baryon transport. Constrain models for hadron production at intermediate pT. Why 62.4 GeV? Located (on log scale) mid-way between SPS and RHIC top energies. Many reference data from ISR.

At 62.4 GeV Ncoll very different to 200 GeV Ncoll definition Glauber Monte Carlo Au+Au b ~ 10.5 fm Npart “Participants” Npart/2 ~ A L~A1/3 Ncoll= # of NN collisions: ~A4/3 At 62.4 GeV Ncoll very different to 200 GeV “Collisions”

First immediate result… Paddle Counter Signal top 50% of cross-section 200 GeV PHOBOS Preliminary 62.4 GeV Significant decrease in maximal multiplicity

Charged hadron spectra and yields PHOBOS TO BE SEEN Expect 62.4 GeV fit into √s systematics

Jet quenching predictions at 62.4 GeV I. Vitev nucl-th/0404052 Adil & Gyulassy nucl-th/0405036 RAA (p0) ~ 0.5 - 0.3 at pT = 4 GeV

RAA charged particles Maximum significantly higher than at 200 GeV. same results from all 4 experiments BRAHMS Preliminary Maximum significantly higher than at 200 GeV. There is a suppression for most central data Similar shape evolution with centrality

Universal centrality evolution? PHOBOS 62.4 GeV 200 GeV But, varying the beam energy changes: Initial state: sNN, Ncoll/Npart System : , mB, Nch, Partonic : xT, dE/dx Energy-independent Weak function of Npart, pT . Use central A+A as denominator Scale with 1/<Npart> Allows comparison between different experiments nucl-ex/0405003

PID spectra BRAHMS Phenix preliminary p0 p STAR Preliminary W- X-

RAA for p0 for central data Predictions 0.3 - 0.5 at 4 GeV/c Again maximum > 200 GeV STAR Preliminary Charged ISR reference used for p0 Still discrepancy between charged and p0 Large baryon contribution up to at least 4 GeV/c

Rcp of baryons and mesons Stat. Errors Only STAR preliminary STAR Preliminary (stat. errors only) The RCP(baryon) > RCP(meson) at intermediate pT. Problem with limited statistics.

Baryon/meson ratios Again, large proton contribution at intermediate pT Small difference as function of centrality (not very peripheral 30-60%) STAR Preliminary Lessp in central collisions at 62.4 GeV Ratios factor 2-3 higher than in p+p at pT= 2-4 GeV

Ratios at mid-rapidity Clear systematic trend with collision energy Minbias (0-80%) 62.4 GeV STAR Preliminary Stat. Errors Only STAR Preliminary L/L -/ +: 1.017±0.002 K-/K+: 0.835±0.006 p/p: 0.458±0.005 confirm varying y same effect as varying √s. Ratios flat as function of pT

Statistical model results STAR preliminary Au+Au at √sNN=200GeV and 62 GeV TLQCD~160-170MeV TLQCD~160-170MeV Close to chem. equilibrium ! Close to net-baryon free Tch flat with centrality ● p, K,p ● p, K,p, L, X ● p, K,p ● p, K,p, L, X Energy dependence but small Nch dependence…

but in such a way as to ensure yields stay ~constant (In)dependence of mid-rapidity yields Preliminary Preliminary T, µB, and V all vary with energy, but in such a way as to ensure yields stay ~constant Preliminary

Radial flow Same flow as at 200 GeV Blastwave fit Shape of the mT spectrum depends on mass: Tch Radial flow! p K STAR Preliminary STAR Preliminary STAR Preliminary Same flow as at 200 GeV

Kaon Slopes Top 5% central collisions

 interferometry HBT probes space-time evolution of system and system size at freeze-out. Studies at √s=130, 200 GeV yielded similar HBT radii to SPS energies (“HBT puzzle”). Severe challenge to hydrodynamic calculations. At an intermediate energy, a larger expansion time might point to a long-lived mixed phase. Systematics of central 0-5% Fully consistent Coulomb treatment in kT dependence PRELIMINARY same results from PHOBOS

HBT from SPS to RHIC No sign of qualitatively different expansion dynamics at 62 GeV. Continues to be a severe challenge submitted to Phys. Rev. C Rapid Communications Same results from STAR

Charged particle correlations PHENIX PRELIMINARY PHENIX PRELIMINARY pT Substantial signals attributable to elliptic flow (v2 = <cos(2f)>) v2 apparently saturates and is the same as at 200 GeV Jets are going to be a challenge

Longitudinal elliptic flow h’=|h|-ybeam Longitudinal scaling of v2 nucl-ex/0406021

Identified Elliptic Flow v2 pT [GeV/c] PHENIX preliminary sNN = 62.4 GeV Au+Au centrality : 0-84% stat. error only sys. error <20% v2 pT [GeV/c] Charged p,K,p : PRL91, 182301 (2003) p0 : work in progress sNN = 200 GeV Au+Au centrality : 0-92% stat. error only sys. error <15% 00:03:40 (60s) This is elliptic flow of identified hadron in 62.4 GeV gold on gold collisions. When we compare the results with 200GeV, we can see the pT dependence is similar. The data is limited, therefore once we have much more statistics, we can do centrality dependence and of more particle species. Although statistics not great again resembles 200 GeV

Coalescence at intermediate pT leads to: Quark coalescence? Coalescence at intermediate pT leads to: stat. error only sys. error <20% (62GeV) 15% (200GeV) 62.4 GeV Au+Au: PHENIX preliminary 200 GeV Au+Au, charged p,K,p : from PRL p0 : work in progress The scaling works as for 200 GeV Au+Au v2 /nquark Seems to be slightly lower than 200 GeV for pT/nquark<1 GeV/c 00:04:40 (60s) One of interest results is a scaling of number of quarks in v2. in approximation, both v2 and pT is scaled to number of constituent quark. The plot shows results from 200 GeV gold on gold. 62.4GeV result is like this. We can see the scaling looks working in 62GeV. Also it seems to be slightly lower than 200 GeV. pT /nquark [GeV/c]

Summary Many of the results indicate environment similar at 62.4 GeV to 200 GeV but it’s not identical Initial energy density lower Evidence of jet quenching Cronin effect is stronger HBT radii at ~6 fm Chemical freeze-out conditions similar to 200 GeV (fn Nch) Baryon chemical potential much higher Radial flow as strong as at 200 GeV (fn Nch) Elliptic flow as strong as at 200 GeV (fn centrality) Consistent with Nquark scaling Elliptic flow appears universal at forward rapidities Jet contribution much weaker than at 200 GeV As yet un-answered questions: Are the gluon densities the same in both systems? Do they spend the same amount of time in each stage? i.e. do they reach the same freeze-out conditions in the same manner?

back up

Why an energy scan? Varying the beam energy changes: Initial state: sNN, Ncoll/Npart, Qs(?) System: , mB, Nch Partonic: xT, dE/dx Varying the beam energy changes: Varying the geometry (A,b): jet quenching vary overall path length vary asymmetry Elliptic (and directed) flow Study A dependence at fixed eccentricity. Npart eccentricity

p+p references p0 reference p0 reference charged reference +/-25% uncertainty p0 reference p0 reference charged reference