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Open charm production at RHIC. Xin Dong University of Science and Technology of China - USTC. Introduction Charm production in elementary collisions Open charm production in heavy ion collisions Summary and outlook. Thanks to Conference organizers. B. Mueller, nucl-th/0404015. - PowerPoint PPT Presentation
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1Aug. 10-15, 2005, XXXV ISMD, Czech X.Dong, USTC
Open charm production at RHIC
Xin DongUniversity of Science and Technology of China - USTC
Introduction
Charm production in elementary collisions
Open charm production in heavy ion collisions
Summary and outlook
Thanks toConference organizers
2X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Why Charm? – an ideal probe for studying QGP
B. Mueller, nucl-th/0404015
Heavy ! Charm quarks created at
early stage of HIC
total yields scaled by Nbin
Sensitive to the partonic
rescatterings Collectivity, flow?
light flavor thermalization
Charm as a probe to test early thermalization!
Note: to test the bulk medium response, low pT region are relevant!
3X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Charm energy loss
k
E
M
dP
k
dkkdCdP Fs
,
)/1()(
0
2220
022
022
22
Y. Dokshitzer & D. Kharzeev PLB 519(2001)199
Radiative energy loss of heavy quarks and light quarks
--- Probe the medium property !
Heavy quark has less dE/dx due to suppression of small angle gluon radiation
“Dead Cone” effect
M. Djordjevic, et. al. PRL 94(2005)112301
B.W. Zhang et. al. PRL 93(2004)072301
N. Armesto et. al. PRD71(2005)054027
R. Rapp et. al. ……
J. Adams et. al, PRL 91(2003)072304
h±
4X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Charm elliptic flow
V. Greco et al., PLB 595(2004)202
Coalescence approach
Large X-sec needed to reach high v2 → Charm quark flows →Indication of light flavor thermal equilibrium! Is this large cross section realistic?
AMPT transport model
B. Zhang et al., nucl-th/0502056
5X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
The key point is to determine
Charm collectivity
6X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Charm measurements at RHIC
central arms --- electrons: DC (tracker), Ring Image Cherenkov (RICH), EMCal for(back)ward muon arms --- muons: muon tracker, muon identifier
D recon. from hadronic decay channels: TPC (+TOF) electrons: TPC, TPC+TOF, TPC+EMC
Advantages: -- low material budget, clean environ. -- central, forward/backward coverage
Advantages: -- reconstruction of D mesons -- large acceptance |φ|<2π,|η|<1.5
7X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Issue I - total charm cross section
1) STAR > pQCD PHENIX >~ pQCD
2) Charm total cross section is a critical reference for J/ψ suppression/enhancement justification.
3) Scales (μF and μR ) may be energy dependent.
STAR, PRL, 94, 062301 (2005)
R. Vogt, private communication
8X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Issue II - pT spectrum
PYTHIA spectrum is steeper than data spectrum beauty contamination:Typical pQCD calculations: Beauty will take over charm beyond ~4 GeV/c M. Cacciari et. al. hep-ph/0502203
PYTHIA curves from S. Kelly, QM04
9X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Centrality dependence of non-photonic electrons in Au + Au
PHENIX, PRL 94, 082301(2005)
As expected --- charm quarks are mostly created from initial NN interactions!
QM05
10X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Challenges to theoretical friends
M. Djordjevic, et. al. nucl-th/0507019 N. Armesto et. al. private comm.
Current energy loss mechanisms can only account for part of strong suppression of RAA for electrons.
any beauty?
11X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
V. Greco et al.PLB 595(2004)202
Non-photonic electron v2
Experiments do not agree (2<pT(e)<5 GeV/c)! v2(e) favors v2(c)=v2(q) at pT(e)<2 GeV/c
B. Zhang et al.nucl-th/0502056
12X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Summary
Charm production cross section at 200 GeV measured in
elementary collisions. Total charm yields in HIC approximately obey Nbin scaling.
v2(e) favors non-zero v2(c) !?
RAA(e) ≈ RAA(h) !?
An exciting heavy flavor program has started at RHIC!
Open Issues: pQCD description where is beauty?
Heavy flavor collectivity!
Light flavor thermalization!@RHIC
If confirmed
13X.Dong, USTCAug. 10-15, 2005, XXXV ISMD, Czech
Summary
Before any physics conclusion, experimental data must agree! Single electron approaches are placeholder. Identified open charm (beauty) measurements are definitely
necessary. The upgrade programs in PHENIX and STAR are essential!
Electron approach experiences: 1) spectrum low pT: no distinguishing power high pT: beauty is largely uncertain 2) v2
large statistical and systematical uncertainties