transverse single spin asymmetries and cross-sections for ... · cluster 0.2 0.4 0.6 0.8 1 1.2 1.4...
TRANSCRIPT
Transverse Single Spin Asymmetries And Cross-sections for Forward π0 And η Mesons at
Len K. Eun, for the STAR CollaborationLawrence Berkeley National Laboratory
PhD: Penn State UniversityThesis Advisor: Steve Heppelmann
1Thursday, June 14, 2012
Transverse Single Spin Asymmetry
Previous STAR Measurement shows that π0 asymmetry is large in the region where the
production cross-section is reasonably well described by NLO pQCD prediction, up to xF of ~0.5.
2Thursday, June 14, 2012
Invariant Mass (GeV)0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1
1
10
210
310
410
signal0
signal daughter(s) (+ other tracks)0
, no prompt photon0no Prompt photon (+ other tracks)
FPD ES
FPD EN
Bea
m B
eam
Cou
nter
STAR Time Projection Chamber
Interaction Point
~8 m
East FPD in Run 2006
)tan(-0.4 -0.2 0 0.2 0.4
3.4
3.6
3.8
40
)tan(-0.4 -0.2 0 0.2 0.4
3.4
3.6
3.8
4
STAR Forward Pion Detector (FPD)
STAR FPD is a Pb-glass calorimeter in the very forward region of the
STAR.
Each of the main modules, placed on either side of the
beam line, consists of 49 Pb-glass cells, forming a
7X7 array.
For this analysis, we employed the “Center Cut”, defined by (ηγγ-3.65)2 + Φγγ2 < 0.15.
We look at di-photon event sample dominated by π0 decays.
3Thursday, June 14, 2012
Cluster Energy (GeV)45 50 55 60 65 70 75 80
max
(FPD
cel
l wid
th)
Clu
ster
0.2
0.4
0.6
0.8
1
1.2
1.4
1
10
10
10
Cluster Energy (GeV)45 50 55 60 65 70 75 80
max
(FPD
cel
l wid
th)
Clu
ster
0.2
0.4
0.6
0.8
1
1.2
1.4
1
10
10
10MC Data
Cluster Energy (GeV)40 45 50 55 60 65 70 75 80
max
(FPD
cel
l wid
th)
Clu
ster
0.2
0.4
0.6
0.8
1
1.2
1.4
1
10
10
Cluster Energy (GeV)40 45 50 55 60 65 70 75 80
max
(FPD
cel
l wid
th)
Clu
ster
0.2
0.4
0.6
0.8
1
1.2
1.4
1
10
10
10MC Data
π0 - γ Separation at high xF
The separation between merged π0 clusters and single photons is primarily achieved through studying the second moment of clusters vs. cluster energy.
Previously, the weighting function was simply the energy deposited in a cell. Using logarithm of energy instead improves the separation at high xF significantly.
OLDLinear E
NEWLog of E
4Thursday, June 14, 2012
Thrown Energy (GeV)10 20 30 40 50
Mea
n of
Dep
osite
d / T
hrow
n En
ergy
0.96
0.98
1
1.02
1.04
1.06
Energy loss
Cerenkov, 4800 photons / GeV
Cerenkov, 1400 photons / GeV
Gaussian Mean of Deposited / Thrown Energy Distribution
Thrown Energy (GeV)10 20 30 40 50
Sigm
a of
Dep
osite
d / T
hrow
n En
ergy
0
0.01
0.02
0.03
0.04
0.05
0.06
0.07
0.08
0.09
0.1Gaussian Sigma of Deposited / Thrown Energy Distribution
Reconstructed Energy (GeV)30 35 40 45 50
0 /
MM
1
1.02
1.04
1.06
1.08
1.1 2 cluster events, Data
2 cluster events, Pythia + GSTAR
Mass shift in data not explained by systematic error in di-photon separation measurement: Shift in gain.
Charged particle energy loss and Cherenkov with no attenuation has no energy dependence of gain.
Energy Dependence of Invariant MassStudy of di-photon mass vs. E
indicates that the gain increases with photon energy.
Cherenkov effect + attenuation of optical photons reproduces the observed mass shift vs. E.
Incident angle (~5˚) effect alters the shower shape. Superposition of 4 shower functions corresponding to 4 “z-slices” approximates the deformation.
Distance from cell to photon (cm)-6 -5 -4 -3 -2 -1 0
Frac
tion
of th
e C
lust
er E
nerg
y
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0
20
40
60
80
100
0 cm to 10 cm
Distance from cell to photon (cm)-6 -5 -4 -3 -2 -1 0
Frac
tion
of th
e C
lust
er E
nerg
y
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0
20
40
60
80
100
120
140
160
180
200
220
10 cm to 20 cm
Distance from cell to photon (cm)-6 -5 -4 -3 -2 -1 0
Frac
tion
of th
e C
lust
er E
nerg
y
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0
20
40
60
80
100
120
140
160
20 cm to 30 cm
Distance from cell to photon (cm)-6 -5 -4 -3 -2 -1 0
Frac
tion
of th
e C
lust
er E
nerg
y
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0
20
40
60
80
100
30 cm to 45 cm
Distance from cell center to photon (cm)-4 -3 -2 -1 0 1 2 3 4
Frac
tion
of c
lust
er e
nerg
y in
a c
ell
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0
2
4
6
8
10
12
14
Shower Shape in Vertical Direction
Distance from cell center to photon (cm)-4 -3 -2 -1 0 1 2 3 4
Frac
tion
of c
lust
er e
nerg
y in
a c
ell
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0
2
4
6
8
10
12Shower Shape in Horizontal Direction
ϒϒ
ϒϒ
~5
EM-Shower Modeling
5Thursday, June 14, 2012
Physics Results)2
GeV
3b
c (3
dp
3E
d
-610
-510
-410
-310
-210
-110
1
10
210 = 200 GeV s + X at , 0 STAR p + p
>=3.68 <0
>=3.68 <
>=3.68 NLO pQCD <0
97 (2006)PRL>=4.0 STAR 2003 <0
>=3.8 STAR 2002 <0
>=3.3 STAR 2002 <0
Fx0.3 0.4 0.5 0.6 0.7
ratio
0 /
0
0.5
1STAR
Fx0.3 0.4 0.5 0.6 0.7
N A
0
0.2
0.4
0.6
0.8 = 200 GeV s + X at , 0 + p STAR p
101 (2008)PRL>=3.7 no center cut, <0
>=3.68 center cut, <0
>=3.68 center cut, <
Cross-sections for π0 and η are consistent with expectations.
Transverse spin asymmetry for η is 2.2 sigma larger than that of the π0 for xF > 0.55
arXiv:1205.6826, recently submitted to PRD RC
6Thursday, June 14, 2012
Summary
Transverse single spin asymmetry at RHIC, measured by STAR, PHENIX, and BRAHMS, provides a useful avenue to test the current understanding of the pQCD.
STAR has measured both the cross-section and the asymmetry of forward neutral pions up to xF of 0.5. Cross-section is an important complimentary measurement that enables us to understand the spin measurement within the framework of pQCD.
We have made a number of improvements in analysis techniques to extend the xF reach of both cross-section and asymmetry measurements up to xF of 0.75.
In addition to π0, we also measured η-meson cross-section and asymmetry.
We find that the cross-sections are consistent with expectations based on pQCD + global fragmentation analysis.
The transverse spin asymmetry for the η is 2.2 standard deviation larger than that for the π0.
7Thursday, June 14, 2012