Presentation is loading. Please wait.

Presentation is loading. Please wait.

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.

Published byAvis Hicks Modified over 8 years ago

Similar presentations

Presentation on theme: "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."— Presentation transcript:

1 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

2 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 2020 - eRHIC (eSTAR) 2020 - eRHIC (eSTAR)

3 Nu Xu3/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 2 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

4 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, 014001(2011); arXiv: 1005.4814 Hot QCD Matter Cold QCD Matter - Helicity structure of proton - PDF/NPDF at small-x region

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

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

7 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

8 Nu Xu8/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 2/24/20138 MTD Installation 1)~ 50% MTD has been installed 2)Trigger setup in progress

9 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

10 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 2001-2010TPCu, d, s 2010TPC + TOFu, d, s + dilepton 2013TPC + TOF + MTD u, d, s, c, b + dilepton 2014TPC + TOF + MTD + HFT

11 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!

12 Nu Xu12/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 2012201320142015201620172018201920202021202220232024 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

13 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

14 Nu Xu14/15 STAR Collaboration Meeting, BNL, February 24 – March 1, 2013 - 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

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

Download ppt "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."

Similar presentations

Explore QCD Emerging Property

Explore QCD Emerging Property
The Physics of HFT the Heavy Flavor Tracker at STAR Spiros Margetis Kent State University, USA Excited QCD 2010.

The Physics of HFT the Heavy Flavor Tracker at STAR Spiros Margetis Kent State University, USA Excited QCD 2010.
The Heavy Flavor Tracker (HFT) The Silicon Vertex Upgrade of RHIC Spiros Margetis Kent State University, USA Excited QCD 2010, Slovakia.

The Heavy Flavor Tracker (HFT) The Silicon Vertex Upgrade of RHIC Spiros Margetis Kent State University, USA Excited QCD 2010, Slovakia.
The STAR Upgrade Program Flemming Videbæk Brookhaven National Laboratory For the STAR collaboration Winter Workshop on Nuclear Dynamics, Feb 2013.

The STAR Upgrade Program Flemming Videbæk Brookhaven National Laboratory For the STAR collaboration Winter Workshop on Nuclear Dynamics, Feb 2013.
Jet probes of nuclear collisions: From RHIC to LHC Dan Magestro, The Ohio State University Midwest Critical Mass October 21-22, 2005.

Jet probes of nuclear collisions: From RHIC to LHC Dan Magestro, The Ohio State University Midwest Critical Mass October 21-22, 2005.
The RHIC Physics Program 1 A versitile facility making it possible to study many aspects of the strong force: condensed QCD matter and its phase structure.

The RHIC Physics Program 1 A versitile facility making it possible to study many aspects of the strong force: condensed QCD matter and its phase structure.
Nu Xu1/32“Critical Point and Onset of De-confinement”, 23-29 August, 2010, JINR, Dubna High-Energy Nuclear Collisions and the QCD Phase Structure Nu Xu.

Nu Xu1/32“Critical Point and Onset of De-confinement”, August, 2010, JINR, Dubna High-Energy Nuclear Collisions and the QCD Phase Structure Nu Xu.
Heavy Ion Physics in Future -- Dense Matter Physics & Critical Point Search Nu Xu Nuclear Science Division Lawrence Berkeley National Laboratory Many Thanks.

Heavy Ion Physics in Future -- Dense Matter Physics & Critical Point Search Nu Xu Nuclear Science Division Lawrence Berkeley National Laboratory Many Thanks.
04/11/2008Lijuan Ruan (WWND2008)1 Prototype Performance of Novel Muon Telescope Detector at STAR Outline: Motivation Simulation Intrinsic timing and spatial.

04/11/2008Lijuan Ruan (WWND2008)1 Prototype Performance of Novel Muon Telescope Detector at STAR Outline: Motivation Simulation Intrinsic timing and spatial.
Nu Xu1/17STAR Regional Meeting, Warsaw University of Technology, November 5 th, 2012, Warsaw STAR November 5, 2012 Status of STAR Experiment at RHIC Study.

Nu Xu1/17STAR Regional Meeting, Warsaw University of Technology, November 5 th, 2012, Warsaw STAR November 5, 2012 Status of STAR Experiment at RHIC Study.
STAR Physics Program at RHIC Nu Xu Nuclear Science Division Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA.

STAR Physics Program at RHIC Nu Xu Nuclear Science Division Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA.
QCD Phase Boundary and the Critical Point B. Mohanty (1), X.F. Luo (2,3), H.G. Ritter (3) and N. Xu (3) (1)VECC, Kolkata, 700064, India (2)Modern Physics.

QCD Phase Boundary and the Critical Point B. Mohanty (1), X.F. Luo (2,3), H.G. Ritter (3) and N. Xu (3) (1)VECC, Kolkata, , India (2)Modern Physics.
ICPAQGP 2010, Goa, India High-Energy Nuclear Collisions and QCD Phase Structure Nu Xu (1) Nuclear Science Division, Lawrence Berkeley National Laboratory,

ICPAQGP 2010, Goa, India High-Energy Nuclear Collisions and QCD Phase Structure Nu Xu (1) Nuclear Science Division, Lawrence Berkeley National Laboratory,
Nu Xu1/17 24 th CBM Collaboration Meeting, Krakow, Poland, September 8 – 12, 2014 Study the QCD Phase Structure at the High Baryon Density Nu Xu (1,2)

Nu Xu1/17 24 th CBM Collaboration Meeting, Krakow, Poland, September 8 – 12, 2014 Study the QCD Phase Structure at the High Baryon Density Nu Xu (1,2)
STAR and meRHIC James Dunlop 1. Heavy Flavor Tracker (2013) Tracking: TPC Forward Gem Tracker (2011) Electromagnetic Calorimetry: BEMC+EEMC+FMS (-1 ≤

STAR and meRHIC James Dunlop 1. Heavy Flavor Tracker (2013) Tracking: TPC Forward Gem Tracker (2011) Electromagnetic Calorimetry: BEMC+EEMC+FMS (-1 ≤
Nu Xu1/28VIII International Workshop on Relativistic Aspects of Nuclear Physics, Rio de Janeiro, Brazil, 3-6, November, 2008 Explore the QCD Phase Diagram.

Nu Xu1/28VIII International Workshop on Relativistic Aspects of Nuclear Physics, Rio de Janeiro, Brazil, 3-6, November, 2008 Explore the QCD Phase Diagram.
Status Update on STAR Upgrades Huan Zhong Huang Department of Physics and Astronomy University of California at Los Angeles For the STAR Collaboration.

Status Update on STAR Upgrades Huan Zhong Huang Department of Physics and Astronomy University of California at Los Angeles For the STAR Collaboration.
Nu Xu1/12 ”DNP“, Newport Beach, California, December 24 - 27, 2012 Energy Dependence of the High Moments from Transport Model Simulations Xiaofeng Luo.

Nu Xu1/12 ”DNP“, Newport Beach, California, December , 2012 Energy Dependence of the High Moments from Transport Model Simulations Xiaofeng Luo.
12/12/2010 LHC First Data 2010 – Ann Arbor, USA J.L. Klay 1 A first glimpse down the rabbit hole: status of ALICE after one year Jennifer Klay California.

12/12/2010 LHC First Data 2010 – Ann Arbor, USA J.L. Klay 1 A first glimpse down the rabbit hole: status of ALICE after one year Jennifer Klay California.
Relativistic Nuclear Collisions (RNC) Group Nuclear Science Division (NSD), Lawrence Berkeley National Lab The Relativistic Nuclear Collisions (RNC) group.

Relativistic Nuclear Collisions (RNC) Group Nuclear Science Division (NSD), Lawrence Berkeley National Lab The Relativistic Nuclear Collisions (RNC) group.

Similar presentations

Ads by Google