measurement of upsilon production cross section in d+au collisions at √ s nn =200 gev
DESCRIPTION
Measurement of Upsilon production cross section in d+Au collisions at √ s NN =200 GeV. Anthony Kesich STAR Collaboration University of California, Davis Summer Quarkonium Workshop June 13, 2011. Quarkonia as a Temperature Probe. A . Mocsy , BNL Quarkonia Workshop, June 2011. - PowerPoint PPT PresentationTRANSCRIPT
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Measurement of Upsilon production cross section in d+Au collisions at √sNN=200 GeV
Anthony KesichSTAR Collaboration
University of California, DavisSummer Quarkonium Workshop
June 13, 2011
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Quarkonia as a Temperature Probe
Slide 2
A .Mocsy, BNL Quarkonia Workshop, June 2011
•Quarkonia suppression is a proposed signature of QGP formation•Degree of suppression is a probe of initial QGP temperature•Need d+Au measurements to constrain cold nuclear matter effects• e.g. Shadowing, Cronin effect
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STAR Detector
Slide 3
Time Projection Chamber•Gas Ionization Tracker•Used for eID•Full coverage in φ•|η|<1
Electromagnetic Calorimeter
•Fast detector•Used for triggering and eID•Full coverage in φ•|η|<1
No Silicon Tracker!Reduces EM material budget from 0.06 to 0.01 radiation lengths. Removed in Run 8 and beyond.
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Upsilon Trigger
Slide 4
E2 Cluster
q
E1 Cluster
L0 Trigger Tower
•Called every time we see a high energy tower (>4.2 GeV)•Looks for an associated high energy cluster•Required opening angle larger than 90°•Cuts on reconstructed mass•Only looks at the electromagnetic calorimeters
p+p
Data
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Slide 5
eID via Energy Loss
•Identify electrons via energy loss in the TPC•Some contamination from hadrons• Contamination is less at higher momenta
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Track Matching and E/p
Slide 6
•We can reject out-of-time tracks by matching to the EMC• EMC is a fast detector as opposed to the TPC
•Once matched, we can compute E/p for the track• “Over-cut” on dE/dx to get a more pure sample (but smaller)• Due to their low mass, electrons will have E/p ≈ 1• Some variation from 1 due to background and E loss
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Observed Upsilon Signal
Slide 7
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 me+e- distribution Raw Yield: 172 +/- 20 (stat.) Strong signal (8σ significance)
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Efficiencies
Slide 8
dtdy
N
dy
dB
y
eeL
0
acc 0.34±0.025
L0+L2 0.71±0.05
2(TPC reco) 0.72±0.07
2(eID cut) 0.87±0.04
mass 0.96±0.04
0.15±0.02
=acc×L0+L2×2(TPC reco)×2
(eID cut) × mass
• acc is the efficiency of EMC detector and the geometrical acceptance
• L0+L2 is the efficiency trigger system• (TPC reco) is efficiency of e reco in TPC• mass is efficiency of mass cut• (eID cut) is efficiency of eID cuts
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Upsilon d+Au Cross Section
Slide 9
N 172 ± 20
0.15 ± 0.02
Ldt 32 nb-1
dy 1.0
σ=35 ± 4(stat.) ± 5(syst.) nb
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Nuclear Modification Factor
Slide 10
€
R dAu =1
Nbin ×σ dAuσ pp
×
Bee ×dσ dAu
dy
⎛
⎝ ⎜
⎞
⎠ ⎟y =0
Υ+Υ'+Υ"
Bee ×dσ pp
dy
⎛
⎝ ⎜
⎞
⎠ ⎟y =0
Υ+Υ'+Υ"
•Measure of suppression vs. binary scaled pp collisions• RdAu=1 means no net cold nuclear effects
• RdAu=0 is full suppression
•σpp=42 mb, σdAu=2.2 b
•From Glauber model: <Nbin>=7.5±0.4•pp Y->ee mid-rapidity cross section: 114±38±24 pb• PRD 82 012004 (2010)
•RdAu=0.78±0.28(stat.)±0.20(syst.)•Note: Doesn’t include background like Drell-Yan
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Summary and Outlook
• Run 8 d+Au greatly increased our available data in a low material environment
• Measured RdAu=0.78±0.28(stat.)±0.20(syst.)– Consistent with minimal cold nuclear matter
shadowing• Additional statistics ( ×3) in Run 9 pp 200 ∼
GeV will further shrink the RdAu uncertainty
Slide 11
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Summer Quarkonia Workshop, June 2011
Back-ups
Slide 12
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Summer Quarkonia Workshop, June 2011 Slide 13
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Summer Quarkonia Workshop, June 2011 Slide 14
With SVT Without SVT