Electron Flow in AuAu@200GeV

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1 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

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Electron Flow in AuAu@200GeV. Frank Laue ( [email protected] ) for the STAR Collaboration. Outline Motivation Analysis (Preliminary) Results Outlook. 200GeV (old) Au+Au minimum bias trigger. Motivators. Kai Schweda STAR QM2004. All mesons behave the same All baryons behave the same - PowerPoint PPT Presentation

Transcript of Electron Flow in AuAu@200GeV

Page 1: 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

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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 ?

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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

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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

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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)

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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)

Page 7: Electron Flow in AuAu@200GeV

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

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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§

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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.)

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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§

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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+

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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)

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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

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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

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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

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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)

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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

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Hot Quarks 2004 Frank Laue, BNL ([email protected]) 18

Yields vs (phi-psi)

black = electrons red = fit to electrons blue = hadrons

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Hot Quarks 2004 Frank Laue, BNL ([email protected]) 19

Electron v2

all chargeselectrons

positrons