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Measurements of Nuclear Modification Factor and Elliptic Flow of F Mesons at RHIC. Xiangzhou Cai For the STAR Collaboration Shanghai INstitute of Applied Physics University of California, Los Angeles. Outline Motivations F Spectra, fit function and comparison
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Measurements of Nuclear Modification Factor and Elliptic Flow of F Mesons at RHIC Xiangzhou Cai For the STAR Collaboration Shanghai INstitute of Applied Physics University of California, Los Angeles Outline • Motivations • F Spectra, fit function and comparison • RCP: particle type or particle mass dependence • Elliptic Flow of F Mesons in AuAu 200GeV collision • Summary
Particle types dependence of RCP &v2 PHENIX: PRL91, 182301(03) STAR: PRL92, 052302(04) nucl-ex/0306007 Models: Greco et al, PRC68, 034904(03) RCPsuppression of AuAu collisionsat intermediatePT. Particle type dependence of RCP from Au+Au collisions has been observed. The particle type dependence of the RCP at intermediate pT in AuAu collisions can be explained by Recombination/Coalescence model. R.C.Hwa et al. University of Oregon C.M.Ko et al. Texas A@M R. J. Fries et al. Duke/Minnesota QB Xie et al., Univ. of ShanDong …… 200GeV Au+Au Baryon Meson
Saturation at intermediate pT Baryon and meson difference -- Constituent Quark Number Scaling Hydrodynamic model can describe data well at low pT while the intermediate pT range may be described by ReC/Coalescence model
How about f Meson? • Phi production can be a good probe • OZI rule suppression • small cross section for scattering with nonstrange hadrons • Information from earlier time? • Sensitive to early flow? • Production mechanism: • ggg -> • s sbar -> • K+K- -> • May determine whether the particle dependence of the nuclear modification factor is dividing by the particle mass or particle type mf~1019 MeV/c2 ; mL~1116 MeV/c2; mKs~498 MeV/c2 • m ~ 1019 MeV/c2 , ~ 4.45 MeV/c2,ct ~ 41 fm • Vector meson • quark content : s, sbar • Studied decay channel: K+ K- (49.2%)
Data set of f analysis 62.4 GeV Au+Au collision Divide into 4 Multiplicity Bins 130 GeV Au+Au collision Divide into 3 Multiplicity Bins 200 GeVAu+Au collision Divide into 5 Multiplicity Bins Run 2 &Run 4 200 GeV d+Au collision Divide into 4 Multiplicity Bins 200 GeV p+p collision Divide into 1 Multiplicity Bins Compare the f production between different collision energy & collision system 1)dE/dx identify stable charged particles in a certain momentum range. 2) Fmeson is identified by event mixing method.
f double exp. fit Spectra of f and fits STAR Preliminary Exponential fit AuAu 62GeV AuAu 130GeV Exponential fit pp Double Exp. fit 1)Statistical errors only. 2)Spectra of Au+Au collisions in measured pT range can be described by an exponential function while spectra of d+Au and p+p collisions deviate from the exponential distribution and have a power-law tail at intermediate pT 3)measurements of 200GeV Au+Au collisions at STAR for Run II and Run IV are consistent d+Au200GeV
Most central f spectra in different collision system STAR Preliminary Spectra ofAu+Au collisions at limited pT range can be described by exponential function Spectra ofpp and d+Au collisions have a power-law tail at intermediate PT region Double exponential function can fit the data well. Measure at (mt-mf)>2.5GeV/c2 for AuAu collision may be necessary to see a power-law tail!
’s production mechanics STAR Preliminary 1)/K- as function of system size and energy are constant • kaon coalescence ruled out for production 2)<pT> of in AuAu collisions doesn’t change significantly as a function of collision centrality, unlike pions, kaons and proton. does not show a significant radial flow from late hadronic stage. It is consistent with a f early freeze-out scenario.
RCP of f AuAu 200 GeV Run II dAu 200 GeV • Mesons(Ks, K, f) have the similar RCP for dAu & AuAu collisions at intermediate pT • Baryons (L, X) have the similar RCP too, but higher than mesons. Particle production at intermediate pT region is divided by the particle’s types, not the masses STAR: behaves like mesons, despite of its large mass FAVOR: Recombination/Coalescence model Run IV:AuAu 200 GeV
RCP of f for different collision system STAR Preliminary • Yield suppression at intermediate PT in central Au+Au collisions • Data at 62.4 GeV Au+Au collisions is statistics limited. • RCP in d+Au collisions is enhanced Some Cronin effect for f mesons in d+Au collisions as well.
F V2(use reaction plane method) • Run IV AuAu200 (FullField+ReversedFullField) • ~14M minibias events • main cuts in the analysis: |η|<1.0 NHits>15, NHits/NHitsPoss>0.52 |NSigmaKaon|<2. DipAngle>0.04 |ReactionPlanecut|<Π/20 (event mixing) |vertextZ|<30 ReactionPlane tracks:|NsigmaKaon|>2.0 1 2 1 Event-mixing techniques
Analysis details 1.reaction-plane (Ψ) 2.Azimuth angle distribution a*(1+2*v2*cos(2(Φ-Ψ))) 1.0<pT<1.5GeV/c res: 0.6178 +- 0.00021 3. reaction-plane resolution v2 = v2obs/res
Preliminary results v2 STAR Preliminary 1. the elliptic flow of Φ-meson is close to Ks 2. error bars in high pt range (2.5GeV,5.0GeV) are still large
Summary • We have measured the productions of f for various collisions energy and collisions system. • Within our pT coverage, thef spectra of dAu and pp collisions can be described better by a double exponential function, which is different in AuAu collisions. • The RCP values of f are similar to other mesons at intermediate pT.The particle yield at intermediate pT depends on particle types, instead of on particle masses. • The elliptic flow v2 have been measured in run IV Au+Au 200GeV collisions. Since phi cannot be made via K+K- fusion, this implies partonic collective at RHIC!
Azimuth angle distribution 0.5<pT<1.0GeV/c 1.5<pT<2.0GeV/c 2.0<pT<2.5GeV/c 2.5<pT<3.0GeV/c
Back-up slide---Information via RXX R ~1 -- no nuclear effects:A+B = C * (p+p) deviation from 1 indicate presence of nuclear effects: R>1 enhancement R<1 suppression (energy loss in dense medium)
RAA and RdAu of f ______________ STAR Preliminary RdAu of is closer to that of pion and kaon than that of proton Particle production at intermediate pT region is sorted by the particle’s types, not the masses
Back-up slide---RAA/RCP: h± (200GeV) RAA & RdA RCP dAu dAu AuAu AuAu Charged Hadrons: • Au + Au : RCP and RAA ~ suppression • d + Au : RCP and RdA ~ enhancement
STAR Discrepancy between STAR and PHENIX ?? PHENIX Johann Rafelski etc. nucl-th/0412072