Interplay between v2 and jets at 200GeV Au+Au collisions at RHIC-PHENIX ShinIchi Esumi for
Electron Flow in AuAu@200GeV
description
Transcript of Electron Flow in AuAu@200GeV
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Electron Flow in AuAu@200GeV
Outline•Motivation•Analysis•(Preliminary) Results•Outlook
200GeV (old) Au+Au
minimum bias trigger
Frank Laue([email protected])
for
the STAR Collaboration
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 2
Motivators
•All mesons behave the same
•All baryons behave the same
•Mesons behave differently from baryons
Kai Schweda
STAR QM2004
•NCQ scaling
•dynamic governed by partonic phase, which is observed after coalescence/recombination of quarks ?
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 3
Motivators
Fries,Mueller,Nonaka,Bass
nucl-th/0308051
•NCQ scaling doesn’t work everywhere ?
•v2 is very sensitive probe
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 4
Questions/Problems •Data suggests NCQ scaling (coalescence,recombination) for Elliptic Flow and RCP ! Partonic Phase (hey, ho the QGP!)
•What about hydro-dynamics ? (governed by mass, not NCQ)
•successful spectra (Tkin,f), Nu Xu plot (Teff vs mass)! radial flow
•Radial / Elliptic Flow both caused but pressure, shouldn’t they scale similarly ?
•Why does NCQ scaling works so good at higher pT (phasespace scarcely populated, coalescence less likely)
•s(trongly interacting)QGP, parton-hydrodynamics ?
•u,d¼ 5MeV; s¼150MeV, c¼1.5GeV
! look at charm, both in partonic and hadronic world the charm is very heavy; should be very sensitive
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 5
Line of Thought • Can not measure Charm-Flow directly (yet)• Do D-Meson decay electrons reflect the D-
Meson flow ?• Electron Identification
• Where do the Electrons come from ?• Backgrounds from
• misidentification (contamination) • physics processes (0 ! e+e- + B.R.
1.198%)• detector effects ( ! e+e- : few %, dep. on
material)
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 6
Do Decay-Electrons Reflect the Parent Flow ?Electron vs D Momenta
pelectron (GeV/c) pelectron (GeV/c)
pD
-Meso
n (
GeV
/c)
pD
-Meso
n (
GeV
/c)
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 7pelectron (GeV/c) pD-Meson (GeV/c)
D-
Ele
ctro
n
D-
Ele
ctro
n
Do Decay-Electrons Reflect the Parent Flow ? vs D Momenta
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 8
Do Decay-Electrons Reflect the Parent Flow ?Pythia/Mevsim Simulation
pT / (GeV/c) pT / (GeV/c)
v2 %
v2 %
•D0 (input)
oe§
• 0 (input)
oe§
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 9
Where Do The Electron Come From ?(Pythia)
pelectron (GeV/c)
Fraction of electrons from:
• 0 ! e+ + e- +
•D ! e§ + X
F
pelectron (GeV/c)
d2N
/(d
pdy)
(a
.u.)
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 10
Where Do The Electron Come From ?(Pythia, STAR Simulation/Analysis Chain)
Pythia 6.2
Heavy Quarks turned on
GStar
Reconstruction
Track Associations
| eta | < 1
DCA < 2cm
23 < #fit-Points < 100
20 < #dEdx-Points < 100
0
K0L
,
K0
D0,D§
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 11
TPC dE/dx vs p
log10(p/(GeV/c)
dE/d
x/(
KeV
) +
dE/d
x/(
KeV
)
log10(p/(GeV/c)
-
e+
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 12
Electron Selection• “clean” electrons between the blue lines
• conversion removed via invariant mass method (~50% efficiency)
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 13
Deuteron Contamination (preliminary)
•more than ½ of (anti-)deuterons out of dEdx band
• 2x as many deuterons and anti-deuterons
• 2x(3) more electrons(positrons) than extrapolated (anti-)deuterons
p/(GeV/c)
raw
-yie
ld
dE/d
x/
(KeV
)
log10(p/(GeV/c)
- <20% contam
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 14
-conversions and 0-Dalitz Decays
pT/(GeV/c)v 2
%
mass/(GeV/c2)
dN/d
mas
s 0 ! e+ + e- +
~50-80% of ’s can be removed with invariant mass method
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 15
V2 vs pT
cos(2(-))
pT/(
GeV
/c)
pT/(GeV/c)
black = electrons+positrons
electrons
positrons
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 16
PHENIX PRELIMINARY
STAR Preliminary
Flow of electrons (charm): v2 from PHENIX & STAR
Slightly different dE/dx cut:
3.4<dE/dx<5.0
Au+Au @200GeV
•Run II
•Run IV (fast offline)
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 17
Outlook / To-Do-List• Quantitative measurements
• contaminations and background (yields)• measure flow of contam./ background• ! non-photonic v2
• deuteron flow (constituent model)• 100x better statistics in Run IV (already on tape)
• centrality dependence• reduce backgrounds by 80% with tighter cuts
• EMC electron analysis is already prepared • too low statistics for 62GeV• higher pT , bkg reduction
• Pixel Vertex Detector (¼ 100m Vertex Resolution)• (almost) background free identification of D/B-Mesons
Hot Quarks 2004 Frank Laue, BNL ([email protected]) 18
Yields vs (phi-psi)
black = electrons red = fit to electrons blue = hadrons