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RHIC program and machine performances Hugo Pereira Da Costa, CEA Saclay, PHENIX Collaboration, 3 Juillet 2006.

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Presentation on theme: "RHIC program and machine performances Hugo Pereira Da Costa, CEA Saclay, PHENIX Collaboration, 3 Juillet 2006."— Presentation transcript:

1 RHIC program and machine performances Hugo Pereira Da Costa, CEA Saclay, PHENIX Collaboration, 3 Juillet 2006

2 2 Outline the RHIC collider the experiments selected results collider and detector upgrades

3 3 The RHIC collider

4 4 BNL facility 3.83 km Capable of colliding any nuclear species Energy: 500 GeV for p-p 200 GeV for Au-Au (per N-N collision) protons: Linac  Booster  AGS  RHIC ions: Tandems  Booster  AGS  RHIC STAR PHENIX PHOBOS BRAHMS

5 5 Physics program Study the formation of a quark gluon plasma in high energy high density nuclear matter p+p collisions for reference light ions to study cold nuclear matter effects heavy ions to form a quark gluon plasma use as many different probes as possible because of a lack of decisive proof for a phase transition Polarized p+p program : study the polarized structure functions of the nucleon, notably DeltaG/G

6 6 Collision species and energy RunYearSpeciesEnergy (GeV) 012000Au+Au130 022001/2002Au+Au p+p 200 032002/2003d+Au p+p 200 042003/2004Au+Au 200 62 052004/2005Cu+Cu p+p 200 62 22.5 200 062006p+p 200 62 500

7 7 Integrated luminosity (Au+Au)

8 8 Integrated luminosity (p+p) 100 x 100 Gev pp RUN05-06, PHENIX Integrated Luminosity (final delivered) 0 5 10 15 20 25 30 35 40 45 07142128354249566370778491 PHENIX Days in Physics mode Integrated Luminosity (pb ) RUN05 RUN06

9 9 The experiments

10 10 PHOBOS Multiplicity of charged particles for |  < 5.4 Particles down to low p t (~100MeV) near y = 0 Particle ratios, spectra, and correlations

11 11 BRAHMS Measures momentum, energy of charged hadrons at forward rapidity (up to  =3.2). Low x physics, saturation physics.

12 12 STAR Hadrons, electrons and jets at mid rapidity over  =2 

13 13 PHENIX Central arm hadrons; photons; electrons p>0.2 GeV/c |y|<0.35  =  Muon arms muons; stopped hadrons p>2 GeV/c |y| E [1.2,2.4]  =2 

14 14 Selected results

15 15 Particle production G. Roland (QM’05) PHOBOS 200 GeV Au+Au D. Hofman (Moriond ‘04) Total charged particle production

16 16 Particle ratio

17 17 Elliptic flow (1) Study the  distributions of the particles with respect to the reaction plane. Use v 2, the second coefficient of the Fourrier transform to study the anisotropy related to the pressure gradient in the overlapping area. Positive v2 means that the particles are emitted preferentially in the reaction plan as opposed to perpendicular to it.

18 18 Elliptic flow (2) M. Oldenburg (QM’05)

19 19 Elliptic flow (3)

20 20 Jet Quenching (1) No direct Jet reconstruction at RHIC. Study back to back jets by looking at  correlations between particles. Use a trigger particle of high enough p t ; Look at  between partner and trigger particle  ~ 0 same jet  ~  back to back jet

21 21 Jet Quenching (2)

22 22 Nuclear modification factor (1) yield in A+A N col. yield in p+p R AA = N col = number of equivalent p+p collisions N part = number of participant nucleons

23 23 Nuclear modification factor (2) High Pt particle suppression

24 24 Heavy quarks (1) open charm Measure open charm via non-photonic single electron spectra open charm R AA open charm v 2

25 25 Heavy quarks (2) J/Psi in p+p and d+Au Measure charmonium via di-lepton pairs p+pd+Au

26 26 Heavy quarks (3) J/Psi in Cu+Cu and Au+Au forward rapiditymid rapidity

27 27 Detector upgrades and future RHIC program

28 28 Future physics program Heavy ion High pT phenomena (identified particle, p T >20 GeV/c and  -jet) Lepton pair continuum (low masses to Drell-Yan) Heavy flavor production (c and b physics) Charmonium spectroscopy (J/ ,  ’ and  ) Nucleon structure in nuclei Gluon saturation and the color glass condensate at low x Spin structure of the nucleon (p+p) Gluon spin structure (  G/G) with heavy flavor and  -jet correlations Quark spin structure (  q/q) with W-production Transversity

29 29 RHIC II luminosity upgrade SpeciesunitsObtainedRHIC II p+ppb -1 ~633 d+Aunb -1 4.562 Cu+Cunb -1 2.425 Au+Aumb -1 1602500 T. Frawley (QWG 06)

30 30 STAR upgrades Full acceptance time of flight barrel Micro vertex detector TPC electronic upgrade (faster, higher rate capability) Forward tracking upgrade Compact fast TPC using GEMS

31 31 PHENIX upgrades Central and forward Silicon Vertex detector Hadron blind detector Nose cone calorimeter Muon trigger upgrade (resistive plate chambers) Reaction plane detector

32 32 Conclusion

33 33 Conclusion (1) Heavy flavors at RHIC II and LHC RHIC IILHC Heavy flavor yields/yearsimilar QGP temperature2T c 4T c QGP lifetime~7fm/c~17fm/c N cc /collision10115 N bb /collision0.055 J/psi mechanismsuppression + coalescencecoalescence Upsilon mechanismsuppressionsuppression + coalescence Open b easier  high cross section Open c harder  high feed down from b T. Frawley (QWG 06)

34 34 Conclusion (2) http://en.wikipedia.org/wiki/Relativistic_Heavy_Ion_Collider Fears among the public Before RHIC started operation, there were fears among the public that the extremely high energy could produce one of the following catastrophic scenarios: RHIC creates a black holeblack hole RHIC creates a transition into a different quantum mechanical vacuumtransitionquantum mechanicalvacuum RHIC creates strange matter that is more stable than ordinary matterstrange mattermatter The main issue in the controversy was the demand by critics for physicists to show an exactly zero probability for such a catastrophic scenario, which physics cannot provide. However, by following the same argument of the critics, and using the same experimental and astrophysical constraints, physicists are also unable to demonstrate a zero probability, but just an upper limit for the likelihood, that tomorrow Earth will be struck with a "doomsday" cosmic ray, resulting in the same destructive scenarios. According to this argument of upper limits, RHIC would still modify the chance for the Earth's survival by an extremely marginal amount.physicistsprobabilityastrophysicaldoomsday

35 35 Additional slides

36 36 PHENIX upgrades Aerogel and time-of-flight provide complete p/K/pi separation for momenta up to ~10 GeV/c Hadron-blind detector detects electrons from near the vertex Reaction plane detector measures reaction plane with resolution better by factor 2 minimum bias trigger for low energy runs Vertex detector detects displaced vertices from the decay of charm or bottom mesons Forward calorimeter provides photon+jet studies over a wide kinematic range Resistive plate chambers triggers on rare probes (J/psi, upsilon, W) at high luminosity

37 37 Bibliography http://www.phenix.bnl.gov/phenix/WWW/publish/dave/colloquia/BNL_colloquium.ppt http://qm2005.kfki.hu/Talks/Globe/aug9/1100//IT_QM05_Summary.ppt http://www.phenix.bnl.gov/phenix/WWW/publish/zajc/sp/presentations/RBUP05 http://www-rnc.lbl.gov/qm2004/talks/parallel/Tuesday04/ADrees_PPTWin.ppt https://www.phenix.bnl.gov/phenix/WWW/p/draft/frawley/QWG_phenix_quarkonium_june30_2006.pdf http://en.wikipedia.org/wiki/Relativistic_Heavy_Ion_Collider

38 38 Elliptic flow (1) M. Oldenburg (QM’05)

39 39 Jet quenching (3) J. Jia Lower threshold for trigger and partner. The way side jet is here but its shape is affected by the medium.

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