Charm & bottom RHIC Shingo Sakai Univ. of California, Los Angeles 1.

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Presentation transcript:

Charm & bottom RHIC Shingo Sakai Univ. of California, Los Angeles 1

Outline Non-photonic e result in AuAu b/c separation in non-photonic electron by electron-hadron pp Bottom production Discuss heavy flavor energy loss in the dense matter 2

Heavy flavor & HIC 3 D mesons,  ’,  Heavy quarks (charm & bottom) are produced by gluon fusion in the initial collisions. Total charm yields in AuAu RHIC is scaled by binary collisions heavy quarks are produced before the medium formed and through the matter. probe of QCD matter PRL 94, (2005) AuAu 200 GeV

4 BR D 0 ->K π (3.85±0.10 %) BR D ± ->e+X (17.2 %) Charm quark RHIC  Heavy flavor production has been studied by measuring electrons decay from charm and bottom (non-photonic electron) at RHIC Measured electron  Photonic electron - photon conversion - Dalitz decay  Non-photonic electron - primarily semi-leptonic decay of mesons containing c & b D meson M = [GeV] τ ~ [s] c τ ~ 300 [ μ m]

PHENIX vs. STAR detector 5 o DC + PC ; momentum o RICH ; ring image o EMC ; energy o TPC ; momentum, dE/dx o EMC ; energy o SMD ; shower shape  electron ID is carried with

Photonic electron determination Cocktail method Calculate photonic electron by using measured photonic sources (PHENIX) Converter method Install additional converter. Then compare yield w. w/o converter (PHENIX) Invariant mass Reconstruct photonic electron by calculating Inv. Mass of ee (STAR) photonic e  Main background in electron measurement is photonic electron

Non-photonic e production in AuAu 77 PRL 98, (2007)  binary scaling of total e ± yield from heavy flavor decay => hard process production  high p T e ± suppression increasing with centrality => heavy flavor energy loss => very high dense matter is formed in AuAu collisions

Models for energy loss radiative energy loss with typical gluon densities is not enough (Djordjevic et al., PLB 632(2006)81) models involving a very opaque medium agree better (Armesto et al., PLB 637(2006)362) collisional energy loss / resonant elastic scattering (Wicks et al., nucl-th/ , van Hees & Rapp, PRC 73(2006)034913) A. Suaide QM06

Models for energy loss radiative energy loss with typical gluon densities is not enough (Djordjevic et al., PLB 632(2006)81) models involving a very opaque medium agree better (Armesto et al., PLB 637(2006)362) collisional energy loss / resonant elastic scattering (Wicks et al., nucl-th/ , van Hees & Rapp, PRC 73(2006)034913)  Uncertainty from bottom quark contribution not only theory but also high pT A. Suaide QM06

e HF -h correlation in AuAu 10 trigger  Away side structure is similar to mach cone shape  The other evidence of heavy quark energy lose 0 – 20%: 3 < p T trig < 6 GeV/c & 0.15 < p T asso < 1 GeV/c STAR preliminary QM08 Gang Wang

(1) Charm quark thermal + flow (2) large cross section ; ~10 mb (3) Elastic scattering in QGP [PRC72,024906] [PRC73,034913] [Phys.Lett. B ] charm quark flow -> partonic level thermalization There is also uncertainty from high pT  Strong elliptic flow for non-photonic electron Non-photonic electron v 2 PRL (2007)

pQCD prediction for Bottom  Since charm and bottom are heavy, their production have been predicted by pQCD  FONLL predicts bottom quark contribution significant (c/b = 1) around 5 GeV/c in non-photonic electron yield with large uncertainty.  Separate charm/bottom by using e-h correlations *Uncertainty comes from mass, PDF, etc in the calculation *FONLL =A Fixed-Order plus Next- to-Leading-log 12

e HF and hadron correlation e D – h (MC) e B – h (MC) fitting GeV 13  Near side width for B decay is wider than that of D decay due to decay kinematics  measuring e-h correlation in pp & fit by MC with B/(B+D) as parameter

e and K correlation 14  Electron-Kaon charge correlation  D meson decay => opposite sign eK pair  B meson decay => same sign eK pair disentangle charm and remaining bottom contribution via (PYTHIA) simulation QM08 Y. Morino

e and D0 correlaion  Request like-sign e-K pair o near-side ; bottom dominant o away-side ; charm dominant 15 compared with MC simulations to get B/D ratio QM08 A. Mischke

B decay contribution  B decay contribution to non-photonic electron  Three independent method (STAR & PHENIX) are consistent  B decay contribution increase with pT  > 50% e decay from B above 4-5 GeV/c  good agreement with pQCD (FONLL) prediction 16

Bottom pp 17  data (c->e & b->e)/pQCD from PHENIX  ratio is almost flat -> pQCD well represent the p T shape   data /  FONLL ~2 reasonable value QM08 Y. Morino upper limit of pQCD Charm decay Bottom decay Data/pQCD

Large Bottom energy loss ?  Bottom quark contribution is ~50% above 4-5 pp => there would be significant bottom contribution in AuAu, too  R AA for non-photonic electron consistent with hadrons  Indicate large energy loss not only charm but also bottom in the dense matter 18 C:B ~ pp

R AA c & R AA b correlation (1)  R AA C and R AA B are connected B decay pp  With the measurements of pp and R AA, we can derive a relationship between R AA c and R AA b. 19 Relation between R AA for charm and bottom decay

R AA c & R AA b correlation (2) o R AA c & R AA b correlation from STAR o Dominant uncertainty is normalization in R AA analysis o R AA b < 1 ; B meson suppressed o prefer Dissociate and resonance model (large b energy loss) 20 I; Phys. Lett. B 632, 81 (2006) ; dN g /dy = 1000 II; Phys. Lett. B 694, 139 (2007) III; Phys.Rev.Lett.100(2008) STAR preliminary p T >5 GeV/c

Summary d+Au Au+Au Same trends of heavy & light in the dense matter R AA Azmuthal correlation v2v2

Summary Heavy quark behavior is same as light quark in the hot & dense RHIC => energy loss & flow STAR & PHENIX extract B decay contribution in non-photonic electron by using electron-hadron correlations in pp. B decay contribution is more than 50% above 5 GeV/c in pp collisions PHENIX study bottom pp and it is consistent with pQCD prediction. STAR study bottom energy loss and the result show B meson suppression with 90% C.L.