star physics program with the tof nu xu for the star collaboration nuclear science division

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Nu Xu 1/20 STAR-DOE TOF Review, BNL, August 10-11, 2009 STAR STAR Physics Program with the TOF Nu Xu for the STAR Collaboration Nuclear Science Division Lawrence Berkeley National Laboratory

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STAR Physics Program with the TOF Nu Xu for the STAR Collaboration Nuclear Science Division Lawrence Berkeley National Laboratory. 1) At 200 GeV top energy - Study medium properties, EoS - pQCD in hot and dense medium 2) RHIC beam energy scan - PowerPoint PPT Presentation

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Page 1: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

STAR Physics Programwith the TOF

Nu Xufor the STAR Collaboration

Nuclear Science DivisionLawrence Berkeley National Laboratory

Page 2: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 2/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARSTAR Physics Focus

1) At 200 GeV top energy - Study medium properties, EoS - pQCD in hot and dense medium

2) RHIC beam energy scan - Search for the QCD critical point - Chiral symmetry restoration

Polarized spin program - Study proton intrinsic properties

Forward program - Study low-x properties, search for CGC - Study elastic (inelastic) processes (pp2pp) - Investigate gluonic exchanges

Page 3: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 3/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARSTAR Detector

MRPC TOF barrel100% ready for run 10

BBC

PMD

FPD

FMS

EMC barrelEMC End Cap

DAQ1000

FGT

Completed

Ongoing

MTD

R&DHFT

TPC

FHC

HLT

Page 4: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 4/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARSTAR: Physics with TOF

1) Significant improvement in PID. With TPC, PID will be extended to pT ~ 15 GeV/c

2) Correlations with PID hadrons; resonances (up to Ω); trigger with high pT hadrons …

3) Beam energy scan program: event-by-event K/π analysis and net-proton Kurtosis

4) 2π electron and di-electron analysis; heavy flavor program …

STAR TOFSTAR TPC+TOF

Log10(p)

Page 5: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 5/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STAR

red: with STAR TOFblack: without STAR TOF

Acceptance: 10-30 times larger compared with PHENIX

Crucial for enhancing future heavy flavor measurements

Transverse Momentum pT (GeV/c)

J/Ψ e+ + e- reconstruction efficiency

Heavy Flavor Efficiency Improvement

Nu/Xu
Page 6: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 6/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARCurrent Measurements with J/Ψ

(Run7 64M MB events)

Run10, √sNN = 200 GeV Au+Au collisions:

1) Measure the v2 of J/Ψ, with the help of HLT2) Measure the RAA of J/Ψ at high transverse momentum pT > 5 GeV/c

STAR submitted to PRL 0904.0439

Page 7: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 7/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARSTAR High Level Trigger and TOF

Run9 p+p 200 GeV, May 19 - 25

J/ψ

1) Fast filtering for quick data analysis. Run10: try J/ψ v2 2) Online QA 3) TOF: improve STAR trigger capabilities: vertex, pile-up rejection capability…

Page 8: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 8/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STAR

Low pT (≤ 2 GeV/c): hydrodynamic mass orderingHigh pT (> 2 GeV/c): number of quarks ordering s-quark hadron: smaller interaction strength in hadronic medium light- and s-quark hadrons: similar v2 pattern

=> Collectivity developed at partonic stage!

Partonic Collectivity at RHIC

Page 9: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 9/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARReconstruction Efficiency Improvement

TOF:1) Increase efficiency for all resonances2) Extend the pT reach

= EOS parameters: temperature and collective velocities

Page 10: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 10/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARThe di-Lepton Program at STAR

(1) σ

(2) v2

(3) RAA

Mass (GeV/c2) pT (GeV/c)

ρ ϕ J/ψDY, charm Bk

Chiral Symmetry Restoration

DirectRadiation from The Hot/Dense Medium

* TOF is Crucial for the physics.

PH

EN

IX: S

. Afanasiev,, et al. 0706.30434

Page 11: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 11/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STAR Direct Radiation

Expanding partonic matter at RHIC and LHC!Di-leptons allow us to measure the direct radiation from the matter with medium effects, no hadronization!

- Low mass region: , , e-e+

minv e-e+

medium effect Chiral symmetry

- High mass region: J/ e-e+

minv e-e+

Direct radiation

Page 12: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 12/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARMulti-particle Correlations in STAR

-- evidence of conical emissionSTAR: PRL 102, 052302(2009)

d+Au Au+Au central

Df1

Df2

p0

0

p

Away-side

trigger

= STAR large acceptance for correlation analysis

= Search for Mach cone with identified hadrons =>

Properties of the EoS

Page 13: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 13/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STAR

nuclei

hadron gasCSC

quark-gluon plasma

Tc

Baryon Chemical Potential

Critical Point?

Tem

per

atu

re Ea

rly U

niv

ers

e

1 23

2Density FrontierTE

RHIC, FAIR

1Energy Frontier TC

LHC, RHIC

3Baryon Density1st order pha. tran.FAIR, NICA

RHIC Beam Energy Scan Program

Page 14: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 14/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARSearch for Local Parity Violation …

L or B

The separation between the same-charge and opposite-charge correlations.

- Strong EM fields - De-confinement and Chiral symmetry restoration

- PID LPV analysis with TOF- RHIC BES: disappearance

Page 15: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 15/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARHigh Moment Analysis (BES)

STAR Preliminary, QM09

1) High moments are more sensitive to critical point related fluctuations

2) The 4th moment, Kurtosis, is directly related to the corresponding thermodynamic quantity: susceptibility for conserved quantum numbers such as Baryon number, charge, strangeness…

Page 16: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 16/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STAR Particle Identification at STAR

STAR TPC STAR TOF

STAR EMC

STAR HFT

Neutral particles Strange Jets Heavy Quark hyperons Hadrons

Multiple-fold correlations among the identified particles!

e, μ

πK p d

TPC TOF TPC

Log10(p)

Page 17: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 17/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARHFT: Charm Hadron v2 and RAA

- 200 GeV Au+Au m.b. collisions (500M events). - Charm hadron collectivity drag/diffusion constants

Medium properties!

- 200 GeV Au+Au m.b. collisions (|y|<0.5 500M events)- Charm hadron RAA

- Energy loss mechanism! - QCD in dense medium!

Page 18: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 18/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STAR

HFT

TPC

FGT

STAR Detectors: Full 2π particle identification!

EMC+EEMC+FMS(-1 ≤ ≤ 4)TOF

DAQ1000

HLT

Page 19: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 19/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARTOF Operation and Data Analysis

Operation Data Analysis

BNL, RICE, UT, … Calibrations Reconstruction

BNL, IOPP, LBNL, RICE, SINAP, Tsinghua, USTC, … BNL, KISTI

STAR Physics Working Groups

Page 20: STAR Physics Program with the TOF  Nu Xu for the STAR Collaboration Nuclear Science Division

Nu Xu 20/20STAR-DOE TOF Review, BNL, August 10-11, 2009

STARSummary

TOF is a key upgrade at STAR . It greatly extends STAR’s PID capabilities for multiple physics topics, including:

- Thermalization at RHIC

- QCD phase boundary and critical point

- In-medium properties

- Study gluon-rich phenomena at RHIC

STAR thanks DoE NP and NNSFC for their support!