Marzia Rosati mrosati@iastate.edu Iowa State University Third Workshop on Quarkonium IHEP, Beijing China October 15, 2004 Marzia Rosati - ISU 1 SPS CERN, Geneva Pb+Pb 158 AGeV RHIC BNL, New York Au+Au 100+100 GeV LHC CERN, Geneva Pb+Pb 3.3 + 3.3 TeV e/T4 energy density Hunting the Quark Gluon Plasma by Measuring Quarkonium SPS 4 RHIC QGP LHC hadron gas TC ~ 170 MeV temperature New Quarkonium Measurements at SPS: NA60 New Quarkonium Measurements at RHIC: PHENIX Future Opportunities at RHIC and LHC Marzia Rosati - ISU 2 Charmonium as a Probe of QGP Matsui and Satz predicted J/y production suppression in Quark Gluon Plasma because of color screening c c Color Screening Marzia Rosati - ISU 3 The NA50 experiment A closed-geometry muon spectrometer experiment Marzia Rosati - ISU 4 J/y suppression from p-A to Pb-Pb collisions Measured / Expected The J/y production is suppressed in Pb-Pb collisions with respect to the yields extrapolated from proton-nucleus data anomalous suppression ……… Lots of open questions NA60 Marzia Rosati - ISU 5 What’s original in NA60: measuring dimuons in the target region muon trigger and tracking beam tracker ZDC targets magnetic field silicon telescope in a 2.5 T dipole hadron absorber Z-vertex of the interaction determined by the pixel telescope with ~ 200 µm accuracy Indium beam Vertex transverse coordinates determined with better than 20 mm accuracy from the pixel telescope and beam tracker 7 In targets 158 A GeV Beam tracker station target box windows z-vertex (cm) Marzia Rosati - ISU 6 J/y production in Indium-Indium collisions after muon track matching Background s(J/y) : 105 70 MeV matching rate ~ 70% Charm J/y y’ DY A multi-step fit (max likelihood) is performed: a) M > 4.2 GeV : normalize the DY b) 2.2<M<2.5 GeV: normalize the charm (with DY fixed) c) 2.9<M<4.2 GeV: get the J/y yield (with DY & charm fixed) Marzia Rosati - ISU DY yield = 253 ± 16 1964 ± 126 in range 2.9–4.5 GeV J/y yield = 35626 ± 361 7 J/y / Drell-Yan in Indium-Indium collisions B s(J/y) / s(DY) = 19.6 ± 1.3 for L = 6.8 fm or Npart = 128 0.85 ± 0.06 w.r.t. the normal nuclear absorption Projectile J/y L Target all data rescaled to 158 GeV L= mean length of the path of the (cc) system through nuclear matter Marzia Rosati - ISU 8 PHENIX Detector Event characterization detectors in middle Two central arms for measuring hadrons, photons and electrons Two forward arms for measuring muons J/yee in central arms electron measurement in range: || 0.35 pe 0.2 GeV/c Marzia Rosati - ISU J/ymm : forward arms muon measurement in range: 1.2 < || < 2.4 pm 2 GeV/c 9 J/Y Measurement Planned at RHIC p-p : study of production mechanism and cross sections Color evaporation model, Color singlet model, Color octet model Polarization, Rapidity dependence (electron and muon channels) Production of J/Y, Y',.. states Base line for pA and AA p(d)-A : study of "normal nuclear effects": shadowing and energy loss Nuclear dependence of s(J/Y): A or sabs (nuclear absorption) Base line for AA A-A : study of "medium effect" in high density matter J/Y suppression : signature of QGP (Matsui/Satz) J/Y formation by c quark coalescence? Comparisons between various collision species are very important. Studies done via both dielectron and dimuon channels in PHENIX. Marzia Rosati - ISU 10 J/Y in Run 2 p-p Collisions m+m– e+e– Phys.Rev.Lett.92, 051802,2004 Results consistent with shapes from various models and PDF. Take the PYTHIA shape to extract our crosssection Integrated cross-section : 234 ± 36 (stat) ± 34 (sys) ± 24(abs) μb Marzia Rosati - ISU 11 d-Au Collisions Eskola, Kolhinen, Vogt hep-ph/0104124 South Muon Arm North Muon Arm d PHENIX μ, North PHENIX m, SOUTH Au Central Arm PHENIX e PHENIX measurements cover different ranges of the Au parton momentum fraction where shadowing and anti-shadowing are expected All expected to see pT broadening dE/dx not expected to be significant effect at RHIC energies Overall absorption expected Marzia Rosati - ISU 12 J/Y in Run 3 d-Au Collisions In RUN3, we accumulated ~3nb-1 d-Au collisions. m+mm±m± North Arm dAu 780 J/ψ’s s ~ 165 MeV combinatorial background is subtracted using the like-sign pairs physical background (open charm/Drell-Yan) is fitted using an exponential Marzia Rosati - ISU 13 Cross section versus pT J/Y m+mJ/Y m+m- High x2 ~ 0.09 Low x2 ~ 0.003 <pT2> = <pT2>dAu – <pT2>pp 1.77 ± 0.35 GeV2 1.29 ± 0.35 GeV2 (preliminary) pT is broadened for dAu Marzia Rosati - ISU 14 dAu/pp versus pT pT broadening comparable to lower energy (s = 39 GeV in E866) s dA s pp 2197 ) Marzia Rosati - ISU Low x2 ~ 0.003 High x2 ~ 0.09 15 J/Y Rapidity Distribution in dAu and pp Marzia Rosati - ISU 16 dAu/pp versus rapidity compared to lower s RdA Low x2 ~ 0.003 (shadowing region) 1st J/ψ’s at large negative rapidity! Klein,Vogt, PRL 91:142301,2003 Kopeliovich, NP A696:669,2001 Data favors (weak) shadowing + (weak) absorption ( > 0.92) With limited statistics difficult to disentangle nuclear effects. We will need another dAu run! (and more pp data also) Marzia Rosati - ISU 17 Run2 AuAu Phys.Rev.C69, 014901,2004 y = 1.0 Coalescence model (Thews et al) y = 4.0 Stat. Model (Andronic et al.) Absorption model (Grandchamp et al.) Disfavor models with enhancement relative to binary collision scaling. Cannot discriminate between models that lead to suppression relative to binary collision scaling. Marzia Rosati - ISU 18 Simple expectation for AuAu J/ψ’s based on nuclear dependence observed in dAu • Renormalize model predictions to dAu measurement (top panel). • Then reverse RdAu and multiply by itself (bottom panel) • Variations between models not too large at mid-rapidity, but substantial in the large negative or positive rapidity regions. Better models (physics understanding) might help, but a higher statistics dAu baseline, especially in the mm regions is needed. • 2004 AuAu run: ~50 times more data (than RUN2) and we already see c lear J/Y signals Marzia Rosati - ISU 19 Near future at RHIC Full exploration of J/Y production versus “Nbinary” Look forward to future runs with high luminosity where also studies for different collision species and with varying energy can be made Upcoming run in December 2004 CuCu collisions and long p-p run Marzia Rosati - ISU 20 PHENIX Upgrade Ultimately we want to detect open charm “directly” via displaced vertices Development of required Si tracking for PHENIX well underway Marzia Rosati - ISU 21 RHIC-II Luminosity Upgrade RHIC-II: L = 5·1032 cm-2 s-1 (pp) L = 7-9·1027 cm-2 s-1 = 7-9 mb-1 s-1 (AuAu) hadr. min bias: 7200 mb 8 mb-1 s-1 = 58 kHz 30 weeks, 50% efficiency Ldt = 80 nb-1 100% reconstruction efficiency Assume here: sAA = spp (AB) Au+Au, 30 weeks, 50% efficiency produced number of events 2.7·108 J/Y 1·107 Y’ 170100 (1S) 29700 (2S) 32400 (3S) Marzia Rosati - ISU 22 The Physics Landscape: Pb+Pb Collisions SPS->RHIC->LHC d Extrapolation of RHIC results favors low values Marzia Rosati - ISU 23 LHC Heavy Ions ALICE e+e- ALICE μ+μ- CMS ATLAS J/y 2.1x104 8.0x105 3.7x104 2.5x104 1.4x104 5.0x103 2.6x104 2.1x104 Marzia Rosati - ISU 24 Summary The good and bad news: the phenomenology of charmonium in nuclear collisions is richer than anyone supposed There is enough interesting physics to keep us busy Things are not as simple as first supposed The goal of the field has shifted from “discovering the quark-gluon plasma” to “characterizing the nuclear medium under extreme conditions” This is a plus – we’ve moved past presupposing how things will behave and towards measuring and understanding what really happens Charmonium is a critical probe in this wider effort New data from RHIC and NA60 is right around the corner Experimental program will continue at LHC Marzia Rosati - ISU 25