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Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 1
Transverse Spin Studies with STAR at RHIC
Carl A. GagliardiTexas A&M University
for the CollaborationSTARSTAR
Outline • Previous results• Separating the underlying effects• Current status• Future plans
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 2
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 3
STAR detector layout
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 4
Transverse spin runs at STAR• RHIC Run 2 (’01-’02)
– First polarized pp run– Used prototype Endcap EMC for forward π0 detection– ~0.15 pb-1 with Pbeam ~ 16%– AN measurement at <η> ~ 3.8
• Run 3 (’03)– Forward π0 detectors (FPD) installed– ~0.25 pb-1 with Pbeam ~ 27%– Measurements at <η> ~ ±3.7 and <η> ~ ±4.0
• Run 5 (’05)– 25 hours of transverse data during June, ’05– ~0.07 pb-1 and Pbeam ~ 46%
• Run 6 (’06)– Started transverse data taking on April 7th
– FPD++ and full Barrel+Endcap EMCs installed– Measurements underway at both forward and mid-rapidities
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 5
First AN Measurement at STAR
PRL 92, 171801 (2004)
Sivers: spin and k correlation in parton distribution functions (initial state)
Collins: spin and k correlation in fragmentation function (final state)
Qiu and Sterman (initial state) / Koike (final state): twist-3 pQCD calculations, multi-parton correlations
Can be described by several models:
Similar to result from E704 experiment (√s=20 GeV, 0.5 < pT < 2.0 GeV/c)
√s=200 GeV, <η> = 3.8
STARSTAR
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 6
Forward π0 production at ISR energies
Bourrely and Soffer, EPJ C36, 371: NLO pQCD calculations underpredict the data at low s from ISR Ratio appears to be a function of angle and √s, in addition to pT
√s=23.3GeV √s=52.8GeV
xF xF
Ed
3 d
p3 [b
/GeV
3 ]
Ed
3 d
p3 [b
/GeV
3 ]
NLO calculations with different
scales:
pT and pT/2
Data-pQCD differences
at pT=1.5GeV
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 7
pp π0 + X cross sections at 200 GeV
NLO pQCD calculations by Vogelsang, et al.
nucl-ex/0602011
STARSTAR
The error bars are statistical plus point-to-point systematic
Consistent with NLO pQCD calculations at 3.3 < η < 4.0
Data at low pT trend from KKP fragmentation functions toward Kretzer. PHENIX observed similar behavior at mid-rapidity.
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 8
Inclusive π0 AN from runs 3+5
• Sizable asymmetries for xF > 0.4
• Back angle data consistent with AN ~ 0
~ 6σ from 0 for xF>0.4
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 9
Combined AN(pT) for xF > 0.4 from runs 3+5Online calibration of CNI polarimeter
Data are consistent with the 1/pT expectation of pQCD
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 10
Separating Sivers and Collins effects
Collins mechanism: asymmetry in the forward jet fragmentation
Sivers mechanism: asymmetry in the forward jet or γ production
SPkT,q
p
p
SP
p
p
Sq kT,π
Need to go beyond π0 detection tojets and direct photons
Sensitive to proton spin – parton transverse motion correlations
Sensitive to transversity
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 11
Event yield with FPD when Nγ > 1
• ~16% arises from “jet-like” events with ≥3 observed photons
• Also expect γ/π0 > 1 for single photons with xF > 0.5
• Need to separate these contributions reliably
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 12
FPD FPD++ for run 6
West end of the STAR interaction region
Runs 3-5
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 13
Run 6
FPD FPD++ for run 6
West end of the STAR interaction region
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 14
Run 6
FPD FPD++ for run 6
West end of the STAR interaction region
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 15
FPD++ enables jet and direct photon detection
• Trigger on EM energy in small cells
• Large enough to integrate over a jet cone
• Large enough for direct photon isolation cuts
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 16
Projected sensitivity
• PYTHIA simulations• Trigger on small cells;
sum over entire side• Vector sum of photon
momenta reproduces most forward hard-scattered parton
• Expect 4~5σ effect for 5 pb-1 if observed π0 AN is due to Sivers effect
L.C. Bland, hep-ex/0602012
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 17
D.
Bo
er
an
d W
. V
og
els
an
g,
Ph
ys.
Re
v. D
69
, 0
94
02
5 (
20
04
)Back-to-back di-jets: access to gluon Sivers function
5 pb-1 measurement will be sensitive at level of model predictions
Measurements near mid-rapidity with STAR – search for spin-dependent deviation from back-to-back alignment
> 7 GeV trigger jet> 4 GeV away side jet
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 18
Level-2 trigger monitoring output after ~0.84 pb-1
• Clear back-to-back di-jet signature• 6-fold symmetry from Level-0 (single jet) trigger condition• Level-2 filter is insensitive to the granularity
Occasional high-order bit problem in 1 of 5520 EMC towers
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 19
Di-jet kTx>0Di-jet kTx<0
Related to di-jet Δφ
Level-2 trigger monitoring output after ~0.84 pb-1
• Clear back-to-back di-jet signature• 6-fold symmetry from Level-0 (single jet) trigger condition• Level-2 filter is insensitive to the granularity
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 20
Run 7 and beyond
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 21
Run 7 and beyond
Addition of FMS to STAR provides nearly continuous EMC from -1<η<+4
STAR Forward Meson Spectrometer
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 22
Conclusions
• STAR finds sizable AN for inclusive π0 at forward rapidity
• Separating the Sivers contribution from the Collins contribution requires going beyond π0 measurements
• Measurements are underway at both forward and mid-rapidity
• Stay tuned!
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 23
The STARSTAR CollaborationU.S. Labs:
Argonne, Lawrence Berkeley, and Brookhaven National Labs
U.S. Universities: UC Berkeley, UC Davis, UCLA, Caltech, Carnegie Mellon, Creighton, Indiana, Kent State, MIT, MSU, CCNY, Ohio State, Penn State, Purdue, Rice, Texas A&M, UT Austin, Washington, Wayne State, Valparaiso, Yale
Brazil: Universidade de Sao Paolo
China: IHEP - Beijing, IPP - Wuhan, USTC,Tsinghua, SINAP, IMP Lanzhou
Croatia: Zagreb University
Czech Republic: Nuclear Physics Institute
England:University of Birmingham
France: Institut de Recherches Subatomiques Strasbourg, SUBATECH - Nantes
Germany: Max Planck Institute – Munich University of Frankfurt
India:Bhubaneswar, Jammu, IIT-Mumbai, Panjab, Rajasthan, VECC
Netherlands:NIKHEF/Utrecht
Poland:Warsaw University of Technology
Russia: MEPHI – Moscow, LPP/LHE JINR – Dubna, IHEP – Protvino
South Korea:Pusan National University
Switzerland:University of Bern
STARSTAR
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 24
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 25
Possible mechanisms
• Sivers effect [Phys Rev D 41, 83 (1990); 43, 261 (1991)]: Flavor dependent correlation between the proton spin (Sp), proton momentum
(Pp) and transverse momentum (kT) of the unpolarized partons inside. The unpolarized parton distribution function fq(x,kT) is modified to:
• Collins effect [Nucl Phys B396, 161 (1993)]:
Correlation between the quark spin (sq), quark momentum (pq) and transverse momentum (kT) of the pion. The fragmentation function of transversely
polarized quark q takes the form:
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 26
<z>
<xq>
<xg>
NLO pQCD
S. Kretzer
p p 0, 3.8, s 200GeV
Forward π0 production at a hadron collider
• Large rapidity π production (η~4) probes asymmetric partonic collisions
• Mostly high-x quark + low-x gluon
• 0.3 < xq< 0.7
• 0.001< xg < 0.1
• <z> nearly constant and high ~ 0.7-0.8
• A probe of low-x gluons
N
N
q
g
s 2EN
ln(tan(2))
xq xF / zEN
xqpxgp
xF 2E
s
zE
Eq
xg pTse g
EN
(collinear approx.)
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 27
xF and pT range of existing FPD data
STARSTAR
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 28
Separated xF and pT dependence
6
5
13
3
B
N
pxdp
dE B
TN
F
Similar to ISR analysisJ. Singh et al., Nucl. Phys. B140, 189 (1978).
Carl Gagliardi – STAR Transverse Spin Studies – DIS‘06 29
Single Spin AsymmetryDefinitions
• Definition:
• dσ↑(↓) – differential cross section of when incoming proton has spin up(down)
Two measurement techniques• Single arm calorimeter:
R – relative luminosity (by BBC)
Pbeam – beam polarization
• Two arms (left-right) calorimeter:
No relative luminosity needed
dd
ddAN
L
LR
RNN
RNN
PA
BeamN
1
LRRL
LRRL
BeamN
NNNN
NNNN
PA
1
π0, xF<0
π0, xF>0
Left
Right
p p
positive AN: more 0 going
left to polarized beam