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Event by Event Isolated Photon Identification in PHENIX EMCal

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Singles. Gines MARTINEZ, Subatech. PHENIX Meeting. Palaiseau ... Free parameter amax : amax between 0.8-0.9. Expected Ratio ('fake direct') from p0 real data : ... – PowerPoint PPT presentation

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Title: Event by Event Isolated Photon Identification in PHENIX EMCal


1
Event by Event Isolated Photon Identification
in PHENIX - EMCal
  • Gine MARTINE , SUBATECH
  • (CNRS/IN2P3 EMN - Université de Nantes)
  • Nantes, FRANCE

s Z
z S
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2
Preface
  • This is a short presentation about the PHENIX
    EMCal capabilities to identify high pT photons.
  • PISA simulation results.
  • I know QM2002 new results are more interesting.
  • But, we are in Palaiseau and we have to make a
    full afternoon of French PHENIX presentations.
  • An analysis note soon.
  • Good reading after QM2002.

3
Motivations Reality
  • We want to measure direct photons.
  • pT range 1 25 GeV/c
  • We want to reject meson decay photons.
  • we can always dream
  • The kinematics of the electromagnetic meson decay
    is what it is.
  • The electromagnetic calorimeter is a real
    detector.
  • Acceptance, Thresholds, Reconstruction, PID, etc
  • Our environment is not very  clean .
  • Large Combinatorial Background, High Multiplicity
    Environment.

4
Outlook
  • Kinematics
  •  Maximum Asymmetry  Parameter
  • Algorithm Spectroscopic Isolation Cut Analysis
    (SIC)
  • Isolated percentage ISOLATED/CANDIDATES
  • Flat distribution
  • Power-law distribuion
  • p0 energy estimation.
  • Energy Threshold.
  • High Multiplicity Environment.
  • Direct Photon Excess Extraction.
  • Conclusions.

5
Kinematics of the p0 decay
6
Relative Opening Angle
Relative opening angle (rad)
7
Asymmetry Parameter
  • Looking for a companion photon within a 100
    acceptance disk Cone inside EMCal
  • Invariant Mass Analysis Spectrometer better than
    Calorimeter (Spectroscopic).
  • Asymmetry as a parameter amax
  • Independent on p0 initial energy
  • Asymmetry as probability
  • Compromise Acceptance vs Rejection
  • amax 0.6, 0.7, 0.8, 0.9 and 0.95

8
The algorithm
  • For each photon  i 
  • Look if the disk (cone projection on EMCal) of
    radius Ri(amax(Ep)) around the center of the
    photon cluster, is inside EMCal
  • if Yes ?  Photon Candidate 
  • Looking for photon companion  j  for which the
    minvij100-160 MeV/c2.
  • if No ?  Isolated Photon  (it could be a  fake
    direct  or a  real direct  photon).
  • Studying the ratio
  • Ratio (dNiso/dEg) / (dNcan/dEg)

9
Mono energetic p0
amax 0.9, RatioNiso/Ncan0.1 amax 0.8,
RatioNiso/Ncan0.2
10
Direct Photon Excess
p0
11
Flat Distribution (E1 , E2)
Ratio Niso/Ncan
12
PISA Simulations
  • pT 0 - 12 GeV/c
  • -0.5lt h lt0.5
  • 0 lt j lt 2p
  • Flat distribution
  • Power Law 1/En,
  • n7.02 (p0 _at_ 130A GeV)

13
Flat p0 Simulation in EMCal
candidates
isolated
amax 0.6
amax 0.7
amax 0.9
amax 0.8
14
Ratio for a Flat p0 Simulation
amax 0.6
amax 0.7
Ratio Niso/Ncan
amax 0.9
amax 0.8
Ratio Niso/Ncan
15
Power Law Distribution
n7.02 AuAu _at_ 130A GeV
Ratio Niso/Ncan
16
Power Law p0 Simulation
amax 0.6
amax 0.7
candidates
isolated
amax 0.9
amax 0.8
17
Ratio for a Power Law
amax 0.6
amax 0.7
Ratio Niso/Ncan
amax 0.9
amax 0.8
Ratio Niso/Ncan
18
Realistic Algorithm
  • Initial p0 energy is unknown
  • High Multiplicity environment
  • Energy threshold of the detector

19
p0 energy estimation
20
With Without p0 energy estimation
FLAT
Ratio Niso/Ncan
Without
With
amax 0.7
amax 0.8
amax 0.9
amax 0.95
Ratio Niso/Ncan
21
With Without p0 energy estimation
POWER LAW
Without
Ratio Niso/Ncan
With
amax 0.7
amax 0.8
amax 0.9
amax 0.95
Ratio Niso/Ncan
22
High Multiplicity Environment
  • Combinatorial Background Simulation
  • Power law background
  • 50 p0s per rapidity unit (peripheral)
  • 300 p0s per rapidity unit (central)

Embedded (raw-rel mixing) with
The single p0 uniformly distributed, and
power-law weighted
23
Low Occupancy (Peripheral)
amax 0.7
amax 0.8
Singles
Ratio Niso/Ncan
Embedded
amax 0.9
amax 0.95
Ratio Niso/Ncan
24
High Occupancy (Central)
amax 0.7
amax 0.8
Singles
Ratio Niso/Ncan
Embedded
amax 0.9
amax 0.95
Ratio Niso/Ncan
25
Threshold Energy
26
Energy Threshold
amax 0.7
amax 0.8
Ratio Niso/Ncan
amax 0.9
amax 0.95
Ratio Niso/Ncan
27
Realistic SIC Analysis
  • Initial p0 energy is unknown
  • High Multiplicity environment
  • Energy threshold of the detector

28
Realistic SIC p0 analysis (pp)
amax 0.7
amax 0.8
Ratio Niso/Ncan
amax 0.9
amax 0.95
Ratio Niso/Ncan
29
Realistic SIC p0 analysis (periph)
amax 0.7
amax 0.8
Ratio Niso/Ncan
amax 0.9
amax 0.95
Ratio Niso/Ncan
30
Realistic SIC p0 analysis (central)
amax 0.7
amax 0.8
Ratio Niso/Ncan
amax 0.9
amax 0.95
Ratio Niso/Ncan
31
Realistic g SIC analysis (pp)
amax 0.7
amax 0.8
Ratio Niso/Ncan
amax 0.95
amax 0.9
Ratio Niso/Ncan
32
Realistic g SIC analysis (periph)
amax 0.7
amax 0.8
Ratio Niso/Ncan
amax 0.95
amax 0.9
Ratio Niso/Ncan
33
Realistic g SIC analysis (central)
amax 0.7
amax 0.8
Ratio Niso/Ncan
amax 0.95
amax 0.9
Ratio Niso/Ncan
34
More about Photon Excess Extraction
35
Photon Excess
36
Conclusions
  • High Photon Identification (SIC).
  • Free parameter amax
  • amax between 0.8-0.9
  • Expected Ratio (fake direct) from p0 real data
  • 0.4 - 0.7
  • When can SIC be applied?
  • Low occupancy
  • pT gt 3 GeV/c for amax0.8
  • pT gt 5 GeV/c for amax0.9
  • High occupancy pT
  • pT gt 5 GeV/c for amax0.8
  • pT gt 7 GeV/c for amax0.9

37
Quark Matter 2002
QM2002 Preliminary
Enjoy !
38
Weather in Nantes
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