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1 Xiangli Cui (for the STAR Collaboration) Di-electron elliptic flow in 200 GeV Au+Au collisions at STAR University of Science and Technology of China (USTC) Brookhaven National Laboratory (BNL) Thermal Radiation Workshop Xiangli Cui
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Xiangli Cui (for the STAR Collaboration)

Feb 06, 2016

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Di-electron elliptic flow in 2 00 GeV Au+Au collisions at STAR. Xiangli Cui (for the STAR Collaboration). University of Science and Technology of China (USTC) Brookhaven National Laboratory (BNL). Outline. Introduction Electron identification Analysis technique - PowerPoint PPT Presentation
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Page 1: Xiangli Cui  (for the STAR Collaboration)

1

Xiangli Cui (for the STAR Collaboration)

Di-electron elliptic flow in 200 GeV Au+Au collisions at STAR

University of Science and Technology of China (USTC)Brookhaven National Laboratory (BNL)

Thermal Radiation Workshop Xiangli Cui

Page 2: Xiangli Cui  (for the STAR Collaboration)

Outline

IntroductionElectron identificationAnalysis techniqueCentrality, mass and pT dependence of v2

Summary

2Thermal Radiation Workshop Xiangli Cui

Page 3: Xiangli Cui  (for the STAR Collaboration)

Introduction

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Low mass region (Mll <1.1 GeV/c2):In-medium modifications of vector mesons.Chiral symmetry restoration?

R. Rapp, et al .,Phys.Rev. C63 (2001) 054907.

Intermediate mass region (1.1< Mll <3.0 GeV/c2 ):QGP thermal radiation.

NA60: Eur. Phys. J.C 61(2009) 711-720

Thermal Radiation Workshop Xiangli Cui

Page 4: Xiangli Cui  (for the STAR Collaboration)

Introduction

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Rupa Chatterjee , et al., Phys Rev C 75, 054909 (2007)

The mass and pT dependences of di-lepton v2 could give very rich information on specific stages of the fireball expansion

Measurements of v2 of thermal di-lepton could distinguish partonic and hadronic radiation sources

Thermal Radiation Workshop Xiangli Cui

Page 5: Xiangli Cui  (for the STAR Collaboration)

5Thermal Radiation Workshop Xiangli Cui

Time Projection Chamber (0<ϕ<2π, |η|<1 )

Tracking – momentum Ionization energy loss (dE/dx, PID) Time Of Flight (0<ϕ<2π, |η|<0.9)

Timing resolution <100ps - significant improvement for PID

STAR detector

Page 6: Xiangli Cui  (for the STAR Collaboration)

Electron identification

Thermal Radiation Workshop Xiangli Cui 6

Clean electron PID Au+Au collisions with a combination of TPC dE/dx and TOF velocity ✓ electron purity ~97% in Au + Au Min Bias collision.

Combine data sets of year 2010 and 2011 ~ 720M

TOF velocity cut to remove slow hadrons

Page 7: Xiangli Cui  (for the STAR Collaboration)

Invariant mass distribution

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Au+Au 0-80%@200GeV

pTe>0.2

|ηe|<1

|yee|<1

efficiency uncorrectedefficiency uncorrected

Thermal Radiation Workshop Xiangli Cui

Background: Like-sign (same) or Unlike-sign (mixed); Signal: Unlike-sign(same) – Background;Signal + Background: Unlike-sign(same)

Mee<=0.7 GeV/c2 : Subtract the like-sign backgroundMee>0.7 GeV/c2 : Subtract the normalized mixed-event background (normalized to like-sign background at Mee(0.7,3) GeV/c2 and pT (0,4)) GeV/c.

We mix events which are in the same centrality bin (9), vertex z bin (10) and event plane angle bin (100), same magnetic field.

Page 8: Xiangli Cui  (for the STAR Collaboration)

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Dominant particle contribution in different mass ranges

STAR Preliminary Mee(0-0.14) : π0+others

Mee(0.14,0.3): η+others

Mee(0.5,0.7) : charm+ρ+ others

Mee(0.7,0.9): ω+others

Mee(0.9,1.1): ϕ+others

Mee(1.1,2.9): charm+other

Thermal Radiation Workshop Xiangli Cui

ϕ

Page 9: Xiangli Cui  (for the STAR Collaboration)

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)1()(

22)(

2BS

SBT

BS

SS

N

Nvv

N

Nv

ji rv /))(2cos( 22

Thermal Radiation Workshop Xiangli Cui

Background: Like-sign (same) or Unlike-sign (mixed).Signal + Background: Unlike-sign(same). Signal: Unlike-sign(same) – Background.

v2T : Signal + Background v2,

v2B: Background v2,

v2S: Signal v2

NS/N(S+B): Signal/(Signal + Background)rj : Resolution of event plane in centrality j<>: average over all di-electron pairs in all events

STAR Preliminary

Analysis technique

Page 10: Xiangli Cui  (for the STAR Collaboration)

Unlike-sign and background v2

10

)1()(

22)(

2BS

SBT

BS

SS

N

Nvv

N

Nv

In each mass bin:

Au+Au 0-80%@200GeV

Thermal Radiation Workshop Xiangli Cui

Calculated the v2T, v2

B and NS/N(S+B) , use above formula to get v2S

Background: Mee <=0.7 GeV/c2: Like-sign same event, Mee >0.7 GeV/c2 : Unlike-sign mixed-event

Page 11: Xiangli Cui  (for the STAR Collaboration)

Cocktail v2 and pT input (Mee<1.1GeV/c2)

Phys. Rev. C 80, 054907 (2009)

http://drupal.star.bnl.gov/STAR/files/Bai_Yuting.pdf (Ph.D thesis)

11Thermal Radiation Workshop Xiangli Cui

Phys.Rev. C 79,051901(2009)

components : π0, η, ω, ϕ

Input: flat rapidity (-1,1);

pT: Tsallis function;

φ:1+ 2v2cos(2φ).

Page 12: Xiangli Cui  (for the STAR Collaboration)

Cocktail simulation results (Mee<1.1GeV/c2)

Thermal Radiation Workshop Xiangli Cui 12

1. Reconstruct e+e- pairs after they decay in the STAR simulators.

2. Same acceptance cuts applied as in data.

3.obtain each component v2 and yield.

4. The cocktail v2 obtained by combining each component v2 (weight by its yield).

5.The cocktail v2 and each component contribution (weighted by the yield) are shown in the plot.

Page 13: Xiangli Cui  (for the STAR Collaboration)

Mee dependence of v2 in Au+Au 200 GeV

13

Di-electron v2 is consistent with simulation using the measured meson v2 as input in Au+Au at 200 GeV.

Work in progress to include intermediate mass region v2

Thermal Radiation Workshop Xiangli Cui

pTe>0.2 (GeV/c)

|ηe|<1, |yee|<1

Page 14: Xiangli Cui  (for the STAR Collaboration)

PT dependence of v2 in Au+Au 200 GeV

Au+Au 0-80%@200GeV

14Thermal Radiation Workshop Xiangli Cui

Simulated v2 is consistent with measured di-electron v2 within uncertainties in 0-80% Au+Au collisions.

The v2 of di-electrons in the ϕ mass region is consistent with the results of ϕKK within error

Page 15: Xiangli Cui  (for the STAR Collaboration)

π0 Dalitz decay v2 and pT Input in different centralities (Mee<0.14 GeV/c2 )

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http://arxiv.org/abs/1203.2644v1PHYSICAL REVIEW C 80, 054907 (2009)

Phys. Rev. Lett. 97 (2006) 152301

components : π0

Input: flat rapidity (-1,1);

pT: MT scaling;

φ: 1+2v2cos(2φ).Thermal Radiation Workshop Xiangli Cui

Page 16: Xiangli Cui  (for the STAR Collaboration)

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Centrality dependence of v2 (Mee<0.14 GeV/c2 )

Thermal Radiation Workshop Xiangli Cui

For each centrality:

1. Reconstruct e+e- pairs after π0 decay in the STAR simulators.

2. Same acceptance cuts applied as in data.

3. obtain e+e- pairs v2

Di-electron v2 is consistent with simulated results for different centralities in Au+Au at 200 GeV.

Page 17: Xiangli Cui  (for the STAR Collaboration)

Summary

For Mee <1.1 GeV/c2, the simulated cocktail v2 are consistent with the measured di-electron v2

For Mee <0.14 GeV/c2, the simulated e+e- v2 are consistent with the measured di-electron v2 in different centralities.

Work in progress to include intermediate mass region v2

17Thermal Radiation Workshop Xiangli Cui

Thanks!