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Quarkonium Physics with STAR Mauro Cosentino (University of Sao Paulo/BNL)
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2 Why Quarkonia ? Using F 1 : S. Digal, P. Petreczky, H. Satz, Phys. Lett. B514 (2001) 57 Using V 1 : C.-Y. Wong, hep-ph/0408020 –Key Idea: Melting in the plasma Suppression of states is determined by T C and their binding energy Color screening Deconfinement QCD thermometer Properties of QGP Is the sequential suppression pattern the smoking gun?
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3 The STAR Detector TPC: | | < 1, 0 < < 2 ToF: -1 < < 0, = 0.1 EMC: | | < 1, 0 < < 2 Mag.Field: 0.5 T
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4 Golden Decay Mode : Need: Electron ID Hadron Rejection Trigger Typical electron p range for: J/ : 1-3 GeV/c : > 3.5 GeV/c
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5 Electron Identification Association of TPC and BEMC information –TPC gives dE/dx and momentum (p) –BEMC gives the energy (E) –Selected particles are within specifics dE/dx and p/E ranges.
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6 J/ Trigger Level-0 (topology): Φ divided in 6 sections Find a tower above threshold (E > 1.2 GeV) Look for other towers above threshold on the 3 opposite sections Level-2 (software): Full EMC tower data available Towers clustering → E e CTB matching (veto photons) Vertex: BBC resolution ~6cm for Au+Au, 30cm for p+p Invariant mass assuming straight tracks: m 2 inv 2E 1 E 2 [1-cos( 12 )] Trigger for m inv > 2.5 GeV/c 2 Decision is taking up to 500 s This J/ trigger setup is efficient only for p+p Au+Au will require ToF upgrade
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7 Trigger Implementation L0 Trigger –Simple single high tower trigger E T >3.5 GeV L2 Trigger –Use similar L2 to J/ Very efficient > 80% Large rejection power –100 at L0 –100 at L2 Luminosity limited Works in p+p and central Au+Au Exploit full STAR acceptance, 2 & | |<1
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8 Results J/ J/ data, Gaussian Fit and simulation line shape. Cross-section calculation being reviewed, but preliminary results consistent with pQCD calculations and PHENIX measurement.
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9 Results STAR cannot resolve different S states (1S+2S+3S) e+e-
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10 Cu+Cu analysis The same analysis for p+p was applied to Cu+Cu@200 GeV data, but without simulations and embedding, no cross-sections quoted No specific triggers. For the a high-tower threshold of 3.75 GeV mimetized the L0 –trigger.
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12 STAR Contribution Large Acceptance at Mid-Rapidity –| |<1, 0< <2 –Pair acceptance~(single acceptance) 2 Electron identification capabilities –TPC dE/dx –EMC E>1-2 GeV (operating full barrel) –TOF p<2-3 GeV/c Trigger capabilities on Barrel EMC –Suitable for single electron (see F. Laue’s talk) –Suitable for di-electrons(?) Heavy-Quarkonia states are rare – : efficient trigger for all systems –J/ trigger in p+p only, need large min. bias. dataset in Au+Au
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13 Efficiency and Purity of the Id
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14 J/ in Au+Au (Run IV) No trigger due to high background Dataset: Au+Au@200 GeV Just a faint signal For efficient J/ trigger, full barrel ToF is needed (just patch in Run IV)
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15 Analysis for Au+Au: Upper Limit 90% C.L.: signal < 4.91 B*d /dy C.L. < 7.6 b Acceptance increase will help (Factor ~4) Scaling from Au+Au to elementary: =1
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16 ToF Upgrade Construction FY 06 – FY 08 23,000 channels covering TPC & Barrel Calorimeter Will allow to deploy J/ trigger in Au+Au Coincidence: ToF slat + EMC tower substantially reduces photon background MRPC Time of Flight Barrel in STAR
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17 Origin of J/ suppression on SPS Assume: 1.N J/ (observed) = 0.6 N J/ + 0.4 N c (compatible w Hera-B data) 2.J/ doesn’t melt c dissociation = ’ dissociation Right or wrong, it shows how important the missing cc measurement is! F. Karsch, D. Kharzeev, H. Satz, hep-ph/0512239
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18 EXTRA: trigger pre-calibration for BEMC Online energy resolution ~ 17%/√E Offline energy resolution ~ 14 %/√E
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