Nu Xu1/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 February 27, 2013 Status of STAR - A report to the Council Nu Xu.

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Nu Xu1/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 February 27, 2013 Status of STAR - A report to the Council Nu Xu

Nu Xu2/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 RHIC Physics Focus Polarized p+p program - Study proton intrinsic properties Forward program - Study low-x properties, initial condition, search for CGC - Study elastic and inelastic processes in pp2pp 1) At 200 GeV at RHIC - Study medium properties, EoS - pQCD in hot and dense medium 2) RHIC beam energy scan (BES) - Search for the QCD critical point - Chiral symmetry restoration eRHIC (eSTAR) eRHIC (eSTAR)

Nu Xu3/15 STAR Collaboration Meeting, BNL, February 24 – March 1, T E RHIC, SPS 3 3 Large μ B NICA, FAIR Exploring the QCD Phase Structure 1 1 T ini, T C LHC, RHIC 2 Partonic Matter Hadronic Matter LHC+RHIC sQGP properties √s NN ~ few TeV LHC+RHIC sQGP properties √s NN ~ few TeV RHIC BES-II QCD phase structure and critical point √s NN ≤ 20 GeV RHIC BES-II QCD phase structure and critical point √s NN ≤ 20 GeV NICA/FAIR QCD phase structure √s NN ≤ 12 GeV NICA/FAIR QCD phase structure √s NN ≤ 12 GeV Future eRHIC Cold nuclear matter properties e + ion collisions Future eRHIC Cold nuclear matter properties e + ion collisions Emergent properties of QCD matter

Nu Xu4/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 QCD Phase Diagram (2010) LHC RHICeRHIC (EIC) K. Fukushima and T. Hatsuda, Rept. Prog. Phys. 74, (2011); arXiv: Hot QCD Matter Cold QCD Matter - Helicity structure of proton - PDF/NPDF at small-x region

HFT TP C TO F BEMC MTD FGT EEMC η = -1 η = 0 η = 1 STAR Detector System (2014)

Nu Xu6/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 Infrastructures for HFT

Nu Xu7/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 HFT at STAR D-Tube Kinematic Mounts Sectors Pixel Support Tube (PST) Read-out

Nu Xu8/15 STAR Collaboration Meeting, BNL, February 24 – March 1, /24/20138 MTD Installation 1)~ 50% MTD has been installed 2)Trigger setup in progress

Nu Xu9/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 Particle Identification at STAR TPC TOF EMC HFT Neutral particles e, μ π K p d TPC TOF TPC Log 10 (p) Multiple-fold correlations for the identified particles! Hyperons & Hyper-nuclei Jets Heavy-flavor hadrons MTD High p T muonsJets & Correlations Charged hadrons

Nu Xu10/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 STAR Detector Configurations  STAR: Large coverage, excellent PID, fast DAQ - detects nearly all particles produced at RHIC - multiple fold correlation measurements - Probes: bulk, penetrating, and bulk-penetrating  STAR: Perfect mid-y collider experiment  STAR: Expanding into forward rapidity regions PeriodDetectorsPhysics TPCu, d, s 2010TPC + TOFu, d, s + dilepton 2013TPC + TOF + MTD u, d, s, c, b + dilepton 2014TPC + TOF + MTD + HFT

Nu Xu11/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 p/A e 0 0 EMCal iTPC Tracking PID EM/HCal Tracking HFT TP C TO F BEMC MTD EEMC GEM η = -1 η = 0 η = 1 STAR Forward Upgrade Plan (2018) HLT Built on the mid-y success: Evolution, not revolution! Built on the mid-y success: Evolution, not revolution! (1)eSTAR taskforce: E. Sichtermann and Z.B. Xu (2)STAR Upgrade/Decadal Plan: C. Gagliardi, H. Huang and F. Videbaek (1)eSTAR taskforce: E. Sichtermann and Z.B. Xu (2)STAR Upgrade/Decadal Plan: C. Gagliardi, H. Huang and F. Videbaek Be part of STAR’s forward upgrades!

Nu Xu12/15 STAR Collaboration Meeting, BNL, February 24 – March 1, ppHIpp/HIHIpppA/HIpA epep/eA Study QCD Phase Structure HFT/MTD: HF, dileptons HFT’ BES-I e-cooling&iTPC BES-II, √s NN ≤ 20GeV Upgrades at large-y & iTPC, CGC, pdf eSTAR/eRHIC CBM Experiment (QCD phase structure) LHC FAiR RHIC LHC √s NN = 5.5 TeV (sQGP properties) Spin: Δg, W ±, A N STAR Core Programs x10 x100

Nu Xu13/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 Future STAR Meetings Datenamelocationchairfocus 2/24 - 3/1CollaborationBNLJ. Dunlop 6/6-7RegionalPragueJ. Bielcik HF,HBT ?Analysis meeting? BES-I, strangeness 7/22-27SQM2013Birmingham 10/20-25CollaborationLBNL? HF, strangeness 11/4-8HP2013Stellenbosch, SA

Nu Xu14/15 STAR Collaboration Meeting, BNL, February 24 – March 1, Be part of STAR forward upgrade - iTPC: BNL, IU, KS, LBNL, SDU, SINAP, UC Davis, USTC - Forward-y: IU, LBNL, Penn State Texas A&M, UCLA Need more efforts! - Be part of STAR operation - Software efforts: - Operation efforts: detector maintain, Early summer, Operation Meeting with conveners. Of course, all are welcome! - Be part of STAR physics analysis - Trainor issue: solvable if the council put its act together Challenges in the Collaboration

Nu Xu15/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013

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