AGS/RHIC User’s Meeting May 12 James Dunlop 1 Brookhaven National Laboratory for the STAR Collaboration Highlights from STAR.

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AGS/RHIC User’s Meeting May 12 James Dunlop 1 Brookhaven National Laboratory for the STAR Collaboration Highlights from STAR

AGS/RHIC User’s Meeting May 12 James Dunlop 2 The STAR Detector MagnetCoilsCentralTriggerBarrel(CTB)ZCalTimeProjectionChamber(TPC) Year 2000 Barrel EM Cal (BEMC) Silicon Vertex Tracker (SVT) Silicon Strip Detector (SSD) FTPC Endcap EM Cal FPD TOFp, TOFr Year DAQ: currently running at ~100x design rate for TPC

AGS/RHIC User’s Meeting May 12 James Dunlop 3 Au+X Datasets  This year: extremely successful run, all BUR goals substantially met  Greater than order of magnitude increase in dataset  Significant new challenge for data processing

AGS/RHIC User’s Meeting May 12 James Dunlop 4 pQCD calculations consistent with measured large-    cross sections Large transverse single-spin effects observed for  s = 200 GeV pp collisions Collins effect  transversity Sivers effect  orbital angular momentum Additional measurements required to disentangle contributions STAR collaboration PRL 92, (2004) Spin: Forward  0

AGS/RHIC User’s Meeting May 12 James Dunlop 5 A LL for at  s = 200 GeV  sensitivity to gluon polarization x  G(x,Q 2 ) x STAR Di-jet event in STAR barrel EMC E T of Jet [GeV] Projections for 2003 Data Achieved in 2003: ● Ave Polarization / Beam ~ 0.25 ● RHIC Delivered Integrated L ~ 0.4 pb -1 Goal for 2005 ● Ave Polarization / Beam ~ 0.40 ● RHIC Delivered Integrated Luminosity ~ 5 pb -1 GRSV maximum x  G(x,Q 2 )  A LL ~ 0.06 for jet production

AGS/RHIC User’s Meeting May 12 James Dunlop 6 e + e - pairs accompanied by nuclear breakup Strong fields: Z  EM ~ 0.6 –Higher order corrections? Full lowest-order QED necessary Limits set on higher order corrections Further topic: exotic meson spectroscopy Preliminary Pair P t (GeVc) Pair Mass (GeV) STAR Preliminary STAR Preliminary UPC collisions: QED J. Adams et al., nucl-ex/ , submitted to PRL

AGS/RHIC User’s Meeting May 12 James Dunlop 7 Jet Quenching  Au + Au, R AA 1  p+p, away side jet exists  Au + Au, away-side correlation suppressed  d+Au, away-side correlation exists  jet quenching ? J. Adams et al., Phys. Rev. Lett. 91, (2003). Pedestal&flow subtracted

AGS/RHIC User’s Meeting May 12 James Dunlop 8 Inclusive hadrons: Evolution with √s Dominant feature: order of magnitude increase at high p T

AGS/RHIC User’s Meeting May 12 James Dunlop 9 Inclusive hadron suppression 2  bins, driven by p+p –  = 0: p T <~6 GeV –  = 0.7: p T <~10 GeV Significant suppression seen at 62 and 200 GeV 1/3 of dataset: quantitative treatment awaits full analysis 200 GeV |  | < GeV |  | < GeV 0.5 < |  | < 0.9

AGS/RHIC User’s Meeting May 12 James Dunlop 10 R CP : Centrality dependence Significant suppression using peripheral as reference relative to both binary and participant scaling 62 GeV |  | < GeV 0.5 < |  | < GeV |  | < 0.5 R CP

AGS/RHIC User’s Meeting May 12 James Dunlop 11 Geometry of away-side suppression  Au+Au: Away-side suppression is larger in the out-of- plane direction compared to in-plane  Geometry of dense medium imprints itself on correlations STAR Preliminary ?

AGS/RHIC User’s Meeting May 12 James Dunlop parton modification in expanding color medium: elongation on   narrowing on   soft partons probe color medium properties peak widths Au-Au p-p reference Au-Au collisions central peripheral 0.15 < p t < 0.5 GeV/c0.5 < p t < 2.0 GeV/c 0.15 < p t < 2.0 GeV/c STAR preliminary Number Correlations at Lower p T

AGS/RHIC User’s Meeting May 12 James Dunlop single point statistical reference data 2D scale inversion  p t  fluctuation inversion minijet dissipation & velocity/temperature structure: elongation on   necking on   200 GeV Au-Au data fluctuation scale dependence  two- particle correlations STAR preliminary soft partons as extended objects peripheral central   Fluctuations → Correlations

AGS/RHIC User’s Meeting May 12 James Dunlop 14 P T is balanced by many gluons “Mono-jet” Dilute parton system (deuteron) Dense gluon field (Au)  E  > 25 GeV     4   Beam View Top View Statistical errors only 25<E  <35GeV 35<E  <45GeV STAR Preliminary dAu Correlations: probing low x Fixed  as E & p T grows Large   0 +h ± correlations Suppressed at small, Consistent with CGC picture Consistent in d+Au and p+p at larger and as expected by HIJING

AGS/RHIC User’s Meeting May 12 James Dunlop 15 Baryon Enhancement  Simple fragmentation picture fails for p T less than ~6 GeV/c  p+pbar/h enhancement in Au + Au not fully explained by Cronin effect  Strong baryon/meson modification in Au + Au also in  /K 0 s ratio J. Adams et al., nucl-ex/ PHENIX STAR preliminary

AGS/RHIC User’s Meeting May 12 James Dunlop 16 R CP of Strange Hadrons  Two groups (2<p t <6GeV/c): - K 0 s, K , K*,   mesons - , ,   baryons  dependence on number of valence quarks  limited to p t <6GeV/c ?  hadron production from quark recombination/ coalescence ?

AGS/RHIC User’s Meeting May 12 James Dunlop 17  Meson – baryon Effect ?  Exp. data consistent with quark recombination/coalescence scenario S.A. Voloshin, Nucl. Phys. A715, 379 (2003). Z. Lin et al., Phys. Rev. Lett., 89, (2002). R. Fries et al., nucl-th/ D. Molnar and S.A. Voloshin, PRL 91, (2003).  Further tests: ,  0, K*, … v 2 : Scaling

AGS/RHIC User’s Meeting May 12 James Dunlop 18 First D Measurement at RHIC  D 0, D , D* spectra from d+Au  Cover range 0.2 < p T < 11 GeV/c  Necessary baseline for Au+Au

AGS/RHIC User’s Meeting May 12 James Dunlop 19 Heavy Flavor D,B  e + X  (e + + e - )/2 spectrum, background subtracted  e-PID by TOF, dE/dx and EMC, measurements consistent  Consistent with measured D meson yield  PYTHIA:c  e, dominates at p T ~ 2-4 GeV/c b  e, dominates at p T > 4-5 GeV/c

AGS/RHIC User’s Meeting May 12 James Dunlop 20 PRELIMINARY 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  HBT 62 GeV

AGS/RHIC User’s Meeting May 12 James Dunlop % events, fully consistent Coulomb treatment No sign of qualitatively different expansion dynamics at 62 GeV PRELIMINARY Systematics of central 0-5% events Fully consistent Coulomb treatment in k T dependence No sign of qualitatively different expansion dynamics at 62 GeV Continues to be a severe challenge HBT from SPS to RHIC

AGS/RHIC User’s Meeting May 12 James Dunlop 22 Outlook Wealth of results from STAR –Critical assessment QGP whitepaper: June Current dataset: qualitative increase in statistical power –Extend p T reach well into perturbative regime Extensive correlation analyses –Charm identification and suppression (or lack) –Extend particle intermediate p T Test v 2 and R CP : where does it scale, and where not? –Extend systematics with 62 GeV Are there any qualitative differences? Can quantitative differences be explained?

AGS/RHIC User’s Meeting May 12 James Dunlop 23 England: University of Birmingham France: Institut de Recherches Subatomiques Strasbourg, SUBATECH - Nantes Germany: Max Planck Institute – Munich University of Frankfurt India: Bhubaneswar, Jammu, IIT-Mumbai, Panjab, Rajasthan, VECC Netherlands: NIKHEF Poland: Warsaw University of Technology Russia: MEPHI – Moscow, LPP/LHE JINR – Dubna, IHEP – Protvino Switzerland: University of Bern U.S. Labs: Argonne, Lawrence Berkeley, and Brookhaven National Labs U.S. Universities: UC Berkeley, UC Davis, UCLA, Caltech, Carnegie Mellon, Creighton, Indiana, Kent State, MIT, MSU, CCNY, Ohio State, Penn State, Purdue, Rice, Texas A&M, UT Austin, Washington, Wayne State, Valparaiso, Yale Brazil: Universidade de Sao Paolo China: IHEP - Beijing, IPP - Wuhan, USTC, Tsinghua, SINR, IMP Lanzhou Croatia: Zagreb University Czech Republic: Nuclear Physics Institute The STAR Collaboration: 51 Institutions, ~ 500 People

AGS/RHIC User’s Meeting May 12 James Dunlop 24 Charged hadron 62 GeV p+p reference from ISRAu+Au from STAR Both p+p reference and Au+Au spectra out to ~12 GeV/c 1/3 of the Au+Au dataset analyzed