Photon Identification via Conversion in 62 GeV Au Au Collisions

About This Presentation
Title:

Photon Identification via Conversion in 62 GeV Au Au Collisions

Description:

Guoji Lin Yale University. 1. Photon Identification via Conversion in 62 GeV Au Au Collisions ... Guoji Lin Yale University. 16. Peak. About 70 times as many as ... –

Number of Views:39
Avg rating:3.0/5.0
Slides: 25
Provided by: guoj1
Learn more at: https://www.star.bnl.gov
Category:

less

Transcript and Presenter's Notes

Title: Photon Identification via Conversion in 62 GeV Au Au Collisions


1
Photon Identification via Conversion in 62 GeV
AuAu Collisions
  • Guoji Lin (Yale)
  • Haibin Zhang(BNL)

2
Outline
  • Data set.
  • AuAu 62 GeV 8M events after event cuts, minium
    bias
  • Photon reconstruction via V0 structure (idea
    from Gene van Buren).
  • cuts
  • results
  • Photon reconstruction via global track
    combination (lots of help from Alexei Chikanian,
    mainly refer to the work of Ian J. Johnson and
    Alexander Wetzler).
  • cuts
  • results
  • Preliminary results on gamma-gamma HBT
  • Conclusions

3
V0 Structures
Typical V0 structure particle identification for
neutral particle which weakly decays into two
oppositely charged particles.
DCADaughterPVertex gt0.7cm
DCAV0Daughters lt1.0cm
DCAV0PVertex lt1cm
open anglelt30 degrees

decay lengthgt2cm
4
Topological Cuts of V0 Structure
  • Distance of closest approach (DCA) of two
    daughter tracks lt 1cm.
  • Decay length of photon gt 2cm.
  • DCA between the reconstructed photon and the
    primary vertex lt 1cm.
  • DCA between the daughter tracks and the primary
    vertex gt 0.7cm.
  • The open angle between the two daughter tracks lt
    30 degrees.
  • Number of hits to reconstruct the daughter
    tracks gt 15.
  • The momentum magnitudes of two daughter
    particles gt 0.1 GeV.
  • The absolute value of the photon rapidity lt 0.5.

5
Armenteros ( ) Cut (1)
First introduced in J. Podolanski and R.
Armenteros, Phil. Mag 45, 13 (1954).
6
Armenteros ( ) Cut (2)

We set the cut for photons as lt
0.01 GeV.
7
dE/dx Cut
  • Plots are from primary tracks.
  • We require that .

8
Mass Cut
and
Black ones are photons without mass cuts. Red
ones are actually that pass the
Pta and dE/dx cuts.
9
Photon Distribution
10
Photon Spectra
  • Raw photon spectra
  • About 10 times less than Alexs result.

11
Peak
The two photons of each pion0 have different
positive and negative daughter track IDs.
12
Cuts for Global Track Reconstruction
  • Photon
  • 10cm lt conv. r lt 200cm
  • DCAxy at conv.lt1.5cm
  • DCAz at conv. lt 1.3cm
  • dip angle diff. lt 0.03 rad
  • full opening angle lt 0.4 rad
  • ? dip lt 0.035 rad
  • ? phi lt 0.05 rad
  • imass lt 0.012 GeV
  • (? dip and phi are the angular difference between
    the photon momenum and the vector from the
    primary vertex to the conversion point)
  • Event
  • vertex has to be found
  • abs(vertexZ) lt 30 cm
  • Track
  • -2 lt dE/dx-dev lt 4
  • fitPoints gt 12
  • Hits/PossHits gt 55
  • if (pt lt 0.3) SDCA gt 0
  • Pion0
  • PosTrackID1?PosTrackID2
  • NegTrackID1?NegTrackID2

13
Photon Distribution
Black line is the result of the global track
combination method. Red line is the rescaled
result of the V0 structure method.
Now we have more than 1 photon per event.
14
photon reconstruction efficiency
From Alexander Wetzlers result
15
Photon Spectra
  • With photon reconstruction efficiency
    correction.
  • Consistent with Alexs result.

16
Peak
About 70 times as many as that from V0 structure
method.
17
Spatial Distribution of Conversion Point
18
Q Variables and
19

20

21

We have to further check why it is not symmetric.
22

23

We dont know what the peak around the origin is.
Is it the HBT signal??
24
Conclusions
  • The method using global track combination is
    much more effective than the one using V0
    structure.
  • There is a strong peak around the origin in the
    C2-1 plot, which still needs further check.
  • We will continue to work on the Calorimeter
    photons and the AuAu 200 GeV data.
Write a Comment
User Comments (0)
About PowerShow.com