Quarkonium Physics with STAR Mauro Cosentino (University of Sao Paulo/BNL)

Slides:



Advertisements
Similar presentations
 Trigger for Run 8 Rates, Yields, Backgrounds… Debasish Das Pibero Djawotho Manuel Calderon de la Barca Analysis Meeting BNL October 16, 2007.
Advertisements

1 Jim Thomas – The Berkeley Lab Three Abstracts for QM 2011 Instrumentation Session The Heavy Flavor Tracker (HFT) The Muon Telescope Detector (MTD) A.
Charm & bottom RHIC Shingo Sakai Univ. of California, Los Angeles 1.
Direct virtual photon production in Au+Au collision at 200 GeV at STAR Bingchu Huang for the STAR collaboration Brookhaven National Laboratory Aug
Bingchu Huang, USTC/BNL 1 Bingchu Huang (for STAR Collaboration) University of Science and Technology of China (USTC) Brookhaven National Laboratory (BNL)
Winter Workshop on Nuclear Dynamics – San Diego, 16 Mar. 2006John Harris (Yale) Suppression of Non-photonic Electrons at High Pt John W. Harris Yale University.
1 Measurement of phi and Misaki Ouchida f or the PHENIX Collaboration Hiroshima University What is expected? Hadron suppression C.S.R.
Quarkonium progress in STAR Manuel Calderón de la Barca Sánchez UC Davis Heavy Flavor Working Group, STAR; XXII Winter Workshop on Nuclear Dynamics La.
Cold Nuclear Matter Effects on Open Heavy Flavor at RHIC J. Matthew Durham for the PHENIX Collaboration Stony Brook University
Johan Gonzalez - Strange Quark Matter 2006, UCLA - March J/ ψ measurements in Au+Au and p+p Collisions at 200 GeV Motivation J/ψ in Au+Au J/ψ in.
4/1/2010MRPC workshop at USTC, Lijuan Ruan (BNL)1 STAR di-lepton measurements Outline: Motivation and Introduction Results from 200 GeV p+p collisions.
 production in p+p collisions in Manuel Calderón de la Barca Sánchez UC Davis STAR Collaboration 23 d Winter Workshop on Nuclear Dynamics Big Sky, Montana.
 (  ->ee) production in d+Au collisions at STAR Haidong Liu For the Collaboration.
Upsilon production in STAR Pibero Djawotho Indiana University Cyclotron Facility October 12, 2007 DNP 2007.
1 The CMS Heavy Ion Program Michael Murray Kansas.
ALICE EMCal Physics and Functional Requirements Overview.
 production in d+Au collisions at STAR Haidong Liu University of California, Davis For the STAR Collaboration.
J/ ψ and Υ measurements in Mauro R. Cosentino for the STAR Collaboration Universidade de São Paulo 1 24 th Winter Workshop, South Padre, TX.
Non-photonic electron production in STAR A. G. Knospe Yale University 9 April 2008.
SQM2006, 03/27/2006Haibin Zhang1 Heavy Flavor Measurements at STAR Haibin Zhang Brookhaven National Laboratory for the STAR Collaboration.
1 The Study of D and B Meson Semi- leptonic Decay Contributions to the Non-photonic Electrons Xiaoyan Lin CCNU, China/UCLA for the STAR Collaboration 22.
Xiaoyan LinQuark Matter 2006, Shanghai, Nov , Study B and D Contributions to Non- photonic Electrons via Azimuthal Correlations between Non-
Υ Measurements at PHENIX Shawn Whitaker RHIC/AGS Users’ Meeting June 20, /20/20111Shawn Whitaker - RHIC/AGS Users Meeting.
Sevil Salur for STAR Collaboration, Yale University WHAT IS A PENTAQUARK? STAR at RHIC, BNL measures charged particles via Time Projection Chamber. Due.
Yuriy Riabov QM2006 Shanghai Nov.19, Measurement of the leptonic and hadronic decays of  and ω mesons at RHIC by PHENIX Yuriy Riabov for the Collaboration.
HFT + TOF: Heavy Flavor Physics Yifei Zhang University of Science & Technology of China Lawrence Berkeley National Lab TOF Workshop, Hangzhou, April,
Measurement of J/ψ production in p+p collisions at √s = 500 GeV at STAR experiment Rongrong Ma (BNL) Hard Probes 2015 McGill University, Montreal, Canada.
Measurements of  Production and Nuclear Modification Factor at STAR Anthony Kesich University of California, Davis STAR Collaboration.
Single Electron Measurements at RHIC-PHENIX T. Hachiya Hiroshima University For the PHENIX Collaboration.
D 0 Measurement in Cu+Cu Collisions at √s=200GeV at STAR using the Silicon Inner Tracker (SVT+SSD) Sarah LaPointe Wayne State University For the STAR Collaboration.
 production in p+p and Au+Au collisions in STAR Debasish Das UC Davis (For the STAR Collaboration)‏
Open charm hadron production via hadronic decays at STAR
Heavy flavor production at RHIC Yonsei Univ. Y. Kwon.
J/Ψ PRODUCTION IN A+A COLLISIONS AT STAR Ota Kukral for the STAR Collaboration Czech Technical University in Prague RHIC & AGS Annual Users’ Meeting 17.
Victor Ryabov (PNPI) for the PHENIX Collaboration QM2005 Budapest Aug,06, First measurement of the  - meson production with PHENIX experiment at.
Peak extraction Because of scarcity of statistics, the peak parameters are fixed from embedded MC. The relative suppression of the excited states is taken.
Recent Charm Measurements through Hadronic Decay Channels with STAR at RHIC in 200 GeV Cu+Cu Collisions Stephen Baumgart for the STAR Collaboration, Yale.
Charm and J/PSI measurement at RHIC Y. Akiba (KEK) August 9, 2002 Riken Summer study 2002.
Quarkonium Physics with STAR Mauro Cosentino (University of Sao Paulo/BNL)
Measurement of J/  -> e + e - and  C -> J/  +   in dAu collisions at PHENIX/RHIC A. Lebedev, ISU 1 Fall 2003 DNP Meeting Alexandre Lebedev, Iowa State.
Measurements of thermal photons in heavy ion collisions with PHENIX - Torsten Dahms - Stony Brook University February 8 th, 2008 Real photons at low p.
03/13/2012Moriond QCD and High Energy Interactions, Mar Di-lepton production at STAR Outline: Motivation and Introduction Recent results from STAR.
M. Muniruzzaman University of California Riverside For PHENIX Collaboration Reconstruction of  Mesons in K + K - Channel for Au-Au Collisions at  s NN.
Measurement of photons via conversion pairs with PHENIX at RHIC - Torsten Dahms - Stony Brook University HotQuarks 2006 – May 18, 2006.
Non-photonic electron production in p+p collisions at √s=200 GeV Xiaozhi Bai for the STAR collaboration Central China Normal University University of Illinois.
ϒ measurements in p+p collisions at √s = 500 GeV with the STAR experiment Leszek Kosarzewski, for the STAR Collaboration Warsaw University of Technology,
STAR J/  Trigger in dA Manuel Calderon for the Heavy-Flavor Group Trigger Workshop at BNL October 21, 2002.
Study of b quark contributions to non-photonic electron yields by azimuthal angular correlations between non-photonic electrons and hadrons Shingo Sakai.
STAR Analysis Meeting, BNL – oct 2002 Alexandre A. P. Suaide Wayne State University Slide 1 EMC update Status of EMC analysis –Calibration –Transverse.
 Production and Suppression in Heavy Ion Collisions at STAR Anthony Kesich University of California, Davis STAR Collaboration February 5, 2013.
JPS/DNPY. Akiba Single Electron Spectra from Au+Au collisions at RHIC Y. Akiba (KEK) for PHENIX Collaboration.
D.Arkhipkin, Y. Zoulkarneeva, Workshop of European Research Group on Ultra relativistic Heavy Ion Physics March 9 th 2006 Transverse momentum and centrality.
PHENIX results on J/  production in Au+Au and Cu+Cu collisions at  S NN =200 GeV Hugo Pereira Da Costa CEA Saclay, for the PHENIX collaboration Quark.
1 Measurements of Leptonic and Photonic Probes in Au+Au Collisions at PHENIX Run-2 Takashi Matsumoto for the PHENIX collaboration at RHIC & AGS Annual.
Outline Motivation The STAR/EMC detector Analysis procedure Results Final remarks.
Hadronic resonance production in Pb+Pb collisions from the ALICE experiment Anders Knospe on behalf of the ALICE Collaboration The University of Texas.
Bottonium Measurements at Midrapidity at the STAR Experiment Lake Louise Winter Institute Feb Ahmed Hamed (Texas A&M University) 1 Ahmed.
Jet Production in Au+Au Collisions at STAR Alexander Schmah for the STAR Collaboration Lawrence Berkeley National Lab Hard Probes 2015 in Montreal/Canada.
J. Zhao Hard Probe 2012, Cagliari 1, Lawrence Berkeley National Lab, USA 2, Shanghai Institution of Applied Physics, CAS, China Di-electron Production.
PHENIX J/  Measurements at  s = 200A GeV Wei Xie UC. RiverSide For PHENIX Collaboration.
Quarkonia production with the HERA-B experiment J. Spengler, MPI Heidelberg.
Open and Hidden Beauty Production in 920 GeV p-N interactions Presented by Mauro Villa for the Hera-B collaboration 2002/3 data taking:
Analysis Meeting, November 9-11, 2003 Manuel Calderón de la Barca Sánchez Heavy Flavor Working Group Heavy Flavor in ‘04: Prospects for J/ . Heavy.
Winter Workshop in Nuclear Dynamics, February 10, 2005 Manuel Calderón de la Barca Sánchez Indiana Unviersity Heavy Flavor in STAR.
Non-Prompt J/ψ Measurements at STAR Zaochen Ye for the STAR Collaboration University of Illinois at Chicago The STAR Collaboration:
Di-electron elliptic flow in
First physics from the ALICE electromagnetic calorimeters
Open heavy flavor analysis with the ALICE experiment at LHC
Quarkonium production in p-p and A-A collisions: ALICE status report
Quarkonium production in p-p and A-A collisions: ALICE status report
Presentation transcript:

Quarkonium Physics with STAR Mauro Cosentino (University of Sao Paulo/BNL)

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/ –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?

3 The STAR Detector TPC: |  | < 1, 0 <  < 2  ToF: -1 <  < 0,  = 0.1 EMC: |  | < 1, 0 <  < 2 

4 Golden Decay Mode : Need: Electron ID Hadron Rejection Trigger Typical electron p range for: J/  : 1-3 GeV/c  : > 3.5 GeV/c

5 electrons  Kp d Electron ID Works from p= GeV/c TPC: dE/dx for p > 0.5 GeV/c –Electrons can be discriminated well from hadrons up to 8 GeV/c –Allows to determine the remaining hadron contamination after EMC ToFEMC

6 Electron ID at medium-p T ToF –Cut at |1/  –1| < 0.03 –clean e ± identification with TPC- ToF up to 2.5 GeV/c Downside: only patch (  / <  <0) Future (2008): full barrel (2 , |  |<1.0) will enable J/  physics (also trigger in AA) p T < 2 GeV/c so far EMC+TPC only not sufficient TPC – particle energy loss e  K p

7 Electron ID at high-pT EMC Towers energy & TPC momentum → p/E≈1 for electrons SMD: hadrons and electrons have different shower shapes hadronselectrons

8 J/  Trigger Level-0 (topology): Fast: t ≤ 1ms 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 L0 rate: ~100 Hz L2 rate: ~ 1 Hz Au+Au will require ToF upgrade

9  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

10 Results J/  (Run IV) Just a faint signal For efficient J/  trigger, full barrel ToF is needed (Run V) trigger commissioning (~1.7M events) Results compatible with expectations Run VI (this year): expect S = (work in progress)

11 Au+Au (Run IV): comissioning run ½ EMC Several technical issues upper limit only p+p (Run VI): Expect significant signal Results  trigger threshold No N ++ +N -- subtracted Cannot resolve different S states   (1S+2S+3S)  e+e-

12 Future & Rates SignalRHIC Exp.ObtainedRHIC-I (>2008) RHIC-IIRHIC-II / R2D LHC / ALICE + J/  → e + e  J/  →     PHENIX~80 ~7000 3,300 29,000 45, ,000 4,300,000 9, ,000  → e + e -  →     STAR PHENIX ,200 1,040 39,000 2,600 8,400 B → J/  → e + e  B → J/  →     PHENIX ,700 67,000 N/A  c → e + e    c →  +    PHENIX ,600 2,900* 117,000* 670,000 N/A D→KD→K STAR~0.4×10 6 (S/B~1/60 0) 30,000** N/A8000 Upgrades: DAQ1000: high data taking rate, no trigger dead time ToF full barrel: → J/  PID and trigger (  veto) RHIC-II: e-cooling, 40  nominal luminosity

13 Summary & Conclusion Quarkonia trigger tested successfully J/  –Expect moderate sample in p+p and Au+Au compared to PHENIX Require ToF upgrade  –Large acceptance & clean trigger –Strength of STAR’s quarkonium program Also: –J/  at forward rapidities -> FPD & FMS (upgrade) –Testing  detectors (re-use CTB, magnet=absorber)

14

15 J/  e + e - Au+Au √s NN =200 GeV J/  e+e- p+p √s=200 GeV Quarkonia in STAR Slowly getting started with J/  : Signal in 200 GeV p+p from 2005 Tested and working trigger in p+p No trigger for AuAu until full ToF in 2009 Much more from 2006 in the works… Also signal in Au+Au with TPC only Large hadron contamination Need full EMC STAR Preliminary

16  in STAR Cannot resolve different S states   (1S+2S+3S)  e + e - STAR –Large acceptance (|  | < 1, full EMC) –PID for electrons (EMC, TPC) –Trigger Very efficient > 80% –Luminosity limited trigger threshold No N ++ +N -- subtracted Scaling from Au+Au to elementary:  =1 First look in 2004: ½ EMC, little statistics 90% C.L.: signal < 4.91 B·d  /dy C.L. < 7.6  b STAR Preliminary

hadrons electrons Electron ID in STAR – EMC 1.TPC: dE/dx for p > 1.5 GeV/c Only primary tracks (reduces effective radiation length) Electrons can be discriminated well from hadrons up to 8 GeV/c Allows to determine the remaining hadron contamination after EMC 2.EMC: a)Tower E ⇒ p/E~1 for e - b)Shower Max Detector Hadrons/Electron shower develop different shape Use # hits cuts 85-90% purity of electrons (p T dependent) h discrimination power ~

18 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.

19 Why Quarkonia? J/  would “melt” in QGP due to screening of static potential between heavy quarks: –Matsui and Satz, Phys. Lett. B 178 (1986) 416 Recent developments shows that the dissociation temperature for heavy quarkonia states are considerably higher than first supposed Using F 1 : S. Digal, P. Petreczky, H. Satz, Phys. Lett. B514 (2001) 57 Using V 1 : C.-Y. Wong, hep-ph/ Feed down from excited states could account for observed suppression [Matsui and Satz, Phys. Lett. B 178 (1986) 416]

20 Achieving our Goals A complete understanding of suppression requires a broad range of systematic studies –p+p, Au+Au, vs. centrality, vs. √s –Measurement of J/  and excited states –Measurement of  and excited states small cross-section  high luminosity  trigger good mass resolution to resolve 1S, 2S, 3S states

21 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

22 Efficiency and Purity of the Id

23 J/  Trigger Level-0 (topology) Fast: t ≤ 1  s Φ divided in 6 sections Find a tower above threshold Look for other towers above threshold on the 3 opposite sections If signal above threshold found, issue trigger

24 J/  Trigger Level-2 (software) Looks for e + e - pairs Towers above threshold→ “seeds” → clusters CTB matching (veto photons) cos(  12 ) obtained from clusters and vertex positions Vertex: BBC resolution ~6cm for Au+Au, 30cm for p+p Pairing clusters and neglecting m e : m 2 inv  2E 1 E 2 [1-cos(  12 )] Decision is taking up to 500  s Real Data, p+p Run V

25 Applicability of the trigger J/  Au+Au: –Only peripheral events have good rejection –Most of J/  yield is on central events (98% of signal on top 60% central) –So, J/  trigger not suitable for Au+Au – Alternative is large min. bias dataset J/  trigger efficient only for p+p

26  trigger: L0 + L2  large mass –Simpler L0, requiring one single tower with E T >3.5 GeV – Use similar L2 algo –Can trigger p+p and central Au+Au events Rare triggers go to “express stream” processing But… very low production rate –Less than 100 expected for full Run IV Au+Au dataset –Actually, only a few achieved, for several reasons

27 J/  in Au+Au (Run IV) No trigger due to high background Dataset: GeV Just a faint signal For efficient J/  trigger, full barrel ToF is needed (just patch in Run IV)

28  trigger in Au+Au  →e + e - channel L0: events with E tower > 3.5 GeV L2: events with pair mass > 7 GeV/c 2 High efficiency (80%) Needs full BEMC for that (only ½ in RunIV) Little statistics trigger threshold No N ++ +N -- subtracted

29  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

30 Run V data sample (p+p) 1.7M events Simulation: yield of J/  Data: yield small but consistent with simulation

31 Data  Simulation Width consistent with detector resolution Mass slightly lower than simulation (2  ) Left tail in simulation due to bremsstrahlung in material at r < 50 cm (beam pipe, SVT, SSD, air, TPC field cage)

32 Run VI p+p (just finished) Barrel EMC full installed L2 widely used (jets, dijets,…) Both triggers are on (J/  and  ) just ended –~3.3M J/  triggered events taken (~800J/  ) –~1.9M  triggered events taken (~80  ) Most of events not reconstructed yet

33 Future perspectives Completed Run VI with sufficient dataset to measure J/  cross-section J/  trigger also deployed for 62.4 GeV Medium-Term Upgrades: –ToF (full barrel) –Heavy Flavor Tracker (HFT) –See next talk (Tony Frawley)

34 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

35 Origin of J/  suppression on SPS Assume: 1.N J/  (observed) = 0.6 N J/  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/

36 EXTRA: trigger pre-calibration for BEMC Online energy resolution ~ 17%/√E Offline energy resolution ~ 14 %/√E

37 J/  in Au+Au (Run IV) No trigger due to high background Dataset: GeV (Minbias) Invariant mass spectra from dE/dx selection (skiping hadron bands) Subtracted spectrum shows a 3.5  signicance peak arount J/  mass Zoom Same event Mixed event J/ψ  e + e - (BR = 5.93%) p (GeV/c) dE/dx Johan Gonzalez, SQM2006

38 Invariant mass spectra vs. centrality Number of J/  in each centrality class is determined by bin counting Gaussian fits (widths are held fixed to the value seen in minbias events) are used to estimate systematics Signal in the 0-20% bin is rather weak, so only an upper limit is quoted Johan Gonzalez, SQM2006

39 Centrality dependence of scaled J/  yields The N bin -scaled yields are plotted vs number of participants Bars indicate statistical uncertainties and the bands indicate the systematic uncertainties An upper limit is quoted for the most central bin Binary Scaling (black line and grey band) Determined from PHENIX data (nucl-ex/ ) Johan Gonzalez, SQM2006

40 Centrality dependence of scaled J/  yields Statistical Hadronization Synopsis: Complete screening of primordial J/ψ’s J/ψ’s regenerated at chemical freezout from thermalized c-cbars Statistical Hadronization[1] calculations are shown for various values of the differential ccbar cross section The model appears to overpredict the scaled J/ψ yields (~Ncc2) for most values of the ccbar cross section However, it should be noted that the uncertainties in the measured[2,3] c-cbar cross sections are rather large at this time. [1] A. Andronic et al., Phys.Lett. B571 (2003) [2] PHENIX, Phys.Rev.Lett. 96 (2006) [3] STAR, Phys. Rev. Lett. 94 (2005) pQCD x-section from:Cacciari, Nason, Vogt, PRL 95 (2005) Johan Gonzalez, SQM2006

41  trigger in Au+Au L0: events with E tower > 3.5 GeV L2: events with pair mass > 7 GeV/c 2

42 Trigger performance in Au+Au 4-20 M events sampled per day Variation on daily samples sizes due to several STAR goals Other triggers reduced the  trigger livetime

43  Analysis for Au+Au 34.2  b -1 sampled –200M+ mb events scanned with  trigger –Only 50M off-line –Small dataset processed Only 3 signal counts (no BG) observed Half field running, no BEMC-based triggers.

44 Trigger performance in Run V Online monitoring of the trigger: Extremely fast turnaround No need for offline production to check the trigger Energy (MeV) Invariant mass (MeV/c 2 )

45 Trigger performance for Run VI Trigger monitoring shows consistency with Run V tests

46 Run VI data analysis Only a few hundred k events, for both triggers, are reconstruct so far Besides limited statistcs is available data seem promissing ~270k  trigger events were enough to give a hint of signal

47  Preliminary analysis Subtracted invariant mass spectrum 270k events