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Quarkonia Measurements in p+p Collisions at STAR Pibero Djawotho Indiana University Cyclotron Facility for the STAR Collaboration 2006-11-19 16:20:00

Quarkonia Measurements in p+p Collisions at STAR

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Quarkonia Measurements in p+p Collisions at STAR. Pibero Djawotho Indiana University Cyclotron Facility for the STAR Collaboration 2006-11-19 16:20:00. Why Quarkonia?. Charmonia: J/ y , Y ’, c c Bottomonia: (1S), (2S), (3S) Key Idea: Melting in the plasma - PowerPoint PPT Presentation

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Page 1: Quarkonia Measurements in p+p Collisions at STAR

Quarkonia Measurements in p+p Collisions at STAR

Pibero DjawothoIndiana University Cyclotron Facility

for the STAR Collaboration2006-11-19 16:20:00

Page 2: Quarkonia Measurements in p+p Collisions at STAR

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Why Quarkonia? Charmonia: J/, ’, c Bottomonia: (1S), (2S), (3S)

Key Idea: Melting in the plasma• Color screening of static potential between heavy quarks:

– J/suppression: Matsui and Satz, Phys. Lett. B 178 (1986) 416• Suppression of states is determined by TC and their binding energy

• Lattice QCD: Evaluation of spectral functions Tmelting

– Sequential disappearance of states: Color screening Deconfinement QCD thermometer Properties of QGP

H. Satz, HP2006

When do states really melt?Tdiss(’) Tdiss(c)< Tdiss((3S)) < Tdiss(J/) Tdiss((2S)) < Tdiss((1S))

Page 3: Quarkonia Measurements in p+p Collisions at STAR

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and J/ States in STARJ/, ’• J/ likely to melt at RHIC• ’ melts at RHICPros• moderate rate• J/ and ’ can be separatedCons• co-mover absorption affects

yield• recombination affects yield• trigger only in pp (still low eff.)• moderate electron PID in J/

momentum range

, ’, ’’ (1S) no melting at RHIC

standard candle (reference) (2S) likely to melt at RHIC

(analog J/) (3S) melts at RHIC (analog ’)Pros• co-mover absorption negligible• recombination negligible at RHIC• STAR efficient trigger and large

acceptanceCons• extremely low rate• need good resolution to separate 3

S states STAR’s strength are the states

Page 4: Quarkonia Measurements in p+p Collisions at STAR

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STAR Detectors Used for Quarkonia

• EMC• Acceptance: || < 1 , 0 < < 2• PID with EMC detectors

• Tower (energy) p/E• High-energy tower trigger enhance high-pT sample• Essential for quarkonia triggers• Luminosity limited for

Page 5: Quarkonia Measurements in p+p Collisions at STAR

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STAR J/ Trigger• L0 (hardware)

– J/ topology trigger: two towers above ET≈1.2 GeV

– Separated by 60° in φ• L2 (software)

– Match EMC high tower to CTB slat photon rejection

– Tower clustering– Cut on mee=√2E1E2(1-cosθ)– Cut on cosθ

• High background contamination ~1.5 GeV/c

• Rejection~100 not sampling full luminosity

• Challenging analysis!!!• Efficiency × acceptance ≈ 12%

Real Data, p+p Run V

prel

imin

ary

Page 6: Quarkonia Measurements in p+p Collisions at STAR

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STAR J/ Signal• Signal in 200 GeV p+p from 2006

• Tested and working trigger in p+p• No trigger for Au+Au until full ToF in 2009

• Integrated luminosity in 2006: 377 nb-1

• Analysis in progress

preliminary

prel

imin

ary

Page 7: Quarkonia Measurements in p+p Collisions at STAR

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STAR Trigger

• Similar L0+L2 triggers– Higher mass state higher energy

threshold– Pros: Easier and cleaner to trigger– Cons: Small yield; need large

luminosity and acceptance• Full EMC acceptance |η|<1 in run 6• Integrated luminosity ≈ 9 pb-1 in run 6

Sample -triggered Event• e+e-

• mee = 9.5 GeV/c2

• cosθ = -0.67• E1 = 5.6 GeV• E2 = 3.4 GeV

charged tracks

Page 8: Quarkonia Measurements in p+p Collisions at STAR

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STAR Mass Resolution

State Mass [GeV/c2] Bee [%] (dσ/dy)y=0 Bee×(dσ/dy)y=0

9.46030 2.38 2.6 nb 62 pb

10.02326 1.91 0.87 nb 17 pb

10.3552 2.18 0.53 nb 12 pb

++ 91 pb

• STAR detector does not resolve individual states of the – Finite p resolution– e-bremsstrahlung

• Yield is extracted from combined ++ states

• FWHM ≈ 1 GeV/c2

W.-M. Yao et al. (PDG), J. Phys. G 33, 1 (2006);R. Vogt et al., RHIC-II Heavy Flavor White Paper

Page 9: Quarkonia Measurements in p+p Collisions at STAR

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Analysis: Electron Id with TPC and EMC

trigger enhances electrons• Use TPC for charged tracks selection• Use EMC for hadron rejection• Electrons identified by dE/dx ionization

energy loss in TPC• Select tracks with TPC, match to EMC

towers above 3 GeV

prel

imin

ary

electrons

K p d

A. Knopse

preliminarypreliminary

e

π

Page 10: Quarkonia Measurements in p+p Collisions at STAR

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• Signal + Background unlike-sign electron pairs• Background like-sign electron pairs

(1S+2S+3S) total yield: integrated from 7 to 11 GeV from background-subtracted mee distribution

• Peak width consistent with expected mass resolution• Significance of signal is 3σ

preliminary

preliminary

STAR Invariant Mass

Page 11: Quarkonia Measurements in p+p Collisions at STAR

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STAR Cross Section

dtdyN

dydB

yee L

0

geo 0.263±0.019

L0 0.928±0.049

L2 0.855±0.048

2(e) 0.47±0.07mass 0.96±0.04

0.094±0.015

=geo×L0×L2×2(e)×mass

geo is geometrical acceptanceL0 is efficiency of L0 triggerL2 is efficiency of L2 trigger(e) is efficiency of e recomass is efficiency of mass cut

preliminary

Page 12: Quarkonia Measurements in p+p Collisions at STAR

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STAR Cross Section at Midrapidity

N 48±15(stat.)

0.094±0.023

Ldt (5.6±0.8) pb-1

dy 1.0

pb(syst.)22(stat.)2891dydσB

Υ"Υ'Υ

0yee

preliminary

Page 13: Quarkonia Measurements in p+p Collisions at STAR

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pb22(syst.)28(stat.)91dydσB

'Υ'Υ'Υ

0yee

STAR 2006 √s=200 GeV p+p ++→e+e- cross section consistent with pQCD and world data

preliminary

STAR vs. theory and world data

Page 14: Quarkonia Measurements in p+p Collisions at STAR

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Summary and Outlook• Full EMC + trigger quarkonium program in STAR• Run 6: first midrapidity measurement of ++→e+e-

cross section at RHIC in p+p collisions at √s=200 GeV – Bee×(dσ/dy)y=0=91±28(stat.)±22(syst.) pb– STAR measurement is consistent with pQCD and world data

• Look for improved STAR cross section in Au+Au collisions at √s=200 GeV in upcoming run