constraining the sivers functions using transverse spin asymmetries at star

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Constraining the Sivers Constraining the Sivers Functions using Transverse Spin Functions using Transverse Spin Asymmetries at STAR Asymmetries at STAR XII International Workshop on Deep Inelastic Scattering , Strbske Pleso, High Tatras, Slovakia , April 16 th 2004 Renee Fatemi for the Collaborat ion

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Constraining the Sivers Functions using Transverse Spin Asymmetries at STAR. Renee Fatemi for the. Collaboration. XII International Workshop on Deep Inelastic Scattering , Strbske Pleso, High Tatras, Slovakia , April 16 th 2004. Outline. Why Transverse Spin? - PowerPoint PPT Presentation

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Page 1: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Constraining the Sivers Functions Constraining the Sivers Functions using Transverse Spin using Transverse Spin Asymmetries at STARAsymmetries at STAR

XII International Workshop on Deep Inelastic Scattering , Strbske Pleso, High Tatras, Slovakia , April 16th 2004

Renee Fatemi for the

      

Collaboration

Page 2: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

• Why Transverse Spin?Why Transverse Spin?• Definition of Sivers Functions Definition of Sivers Functions • Access to Sivers Functions at STARAccess to Sivers Functions at STAR• Spin Physics at RHIC in the STAR detectorSpin Physics at RHIC in the STAR detector• Forward Forward 0 Analysis Analysis • Mid-Rapidity Leading Charged Particle Mid-Rapidity Leading Charged Particle

AnalysisAnalysis• Accessing Sivers Functions with DijetsAccessing Sivers Functions with Dijets• Update on Dijet analysis Update on Dijet analysis • Conclusions and Plans for Future WorkConclusions and Plans for Future Work

Outline

Page 3: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Why Transverse Spin?Why Transverse Spin?

PSP

S

Let S and P be the spin and momentum of 2 colliding Let S and P be the spin and momentum of 2 colliding proton beamsproton beams

If S· P If S· P = 0= 0

If S· P = If S· P = 11

Partonic kT to S×P can give Left/Right Asymmetries

No Azimuthal Asymmetry

# Observables cos()

x

Information on

asymmetries in k = S x P direction

Sk

SID

E V

IEW

BE

AM

VIE

W

Page 4: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Sivers FunctionsSivers Functions

Where Where qqNN is the Sivers Function is the Sivers Function – produces – produces “side preferences”“side preferences”

kPS

)k(PS)k(x,ƒΔ

21

)k(x,ƒ)s,k(x,ƒPP

pPq

NqqPq

Flavor dependent correlation between the proton spin (Sp), momentum (Pp) and transverse momentum (kT) of the unpolarized partons inside. The unpolarized parton distribution function fq(x,k) is modified to:

P P

kT

kT

Page 5: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Sivers correlation is a time-reversal Sivers correlation is a time-reversal odd triple product and therefore odd triple product and therefore

previously thought to vanish previously thought to vanish identically.identically. Recent theoretical Recent theoretical

results show this to be untrue!results show this to be untrue!

• Boer, P.J. Mulders, F. Pijlman, Nucl.Phys.B Boer, P.J. Mulders, F. Pijlman, Nucl.Phys.B 667 (2003) 201 667 (2003) 201

• S.J. Brodsky, D.S. Hwang and I. Schmidt, S.J. Brodsky, D.S. Hwang and I. Schmidt, Phys. Lett. B 530 (2002) 99. Phys. Lett. B 530 (2002) 99.

• A.V. Belitsky, X. Ji and F. Yuan, Nucl. Phys. B A.V. Belitsky, X. Ji and F. Yuan, Nucl. Phys. B 656 (2003) 165656 (2003) 165

• J.C. Collins, Phys. Lett. B 536 (2002) 43J.C. Collins, Phys. Lett. B 536 (2002) 43

Page 6: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Access to Sivers Functions Access to Sivers Functions in STARin STAR

• High-rapidity High-rapidity 0 Production Production p↑ p → p↑ p → 00 + X + X

• Mid-rapidity Leading Charged Particle Mid-rapidity Leading Charged Particle AnalysisAnalysis

p↑ p → hp↑ p → h+/-+/- + X + X

Di-jet productionDi-jet production p↑ p → jet + jet + Xp↑ p → jet + jet + X

Page 7: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Polarized Proton Operation at RHIC

Year 2002 -2003

s = 200 GeV

YEAR 2003•Luminosity = 2x1030 s-1cm-2

•Integrated Luminosity = 0.5/0.4 pb-1 T/L•Polarization = 0.3

YEAR 2002•Luminosity = 5x1029 s-1cm-2

•Integrated Luminosity = 0.3 pb-1

•Polarization = 0.2

Page 8: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

STAR DetectorSTAR Detector

Forward Pion

Detector

Barrel EM Calorimeter

Endcap EM Calorimeter

Beam-Beam

Counters

Time Projection Chamber-1<η< 1

0<η< 1

1<η< 2

-4.1<η< -3.3

2<|η|< 5

Page 9: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Prototype Forward Pion Prototype Forward Pion Detector Detector

• 24 layer Pb-Scintillator Sampling Calorimeter • 12 towers• Shower-Maximum Detector - 2 orthogonal layers of 100 x 60 strips • 2 Preshower Layers

Top-Bottom-South Detectors• 4x4 array of Lead-Glass • No Shower Max• Used for systematic error studies

TRIGGER EDEP > 15 GeV

Page 10: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Single Spin Single Spin 0 0

AsymmetryAsymmetry

00

00

ππ

ππN

YY

YY

Pol1

A

For <> = 3.7 possible contributions to AN are:

Sivers Effect – Spin dependent initial partonic transverse momentum

Collins Effect – Spin dependent transverse momentum kick in fragmentation

Sterman and Qiu – Initial State twist 3

Koike – Final State twist 3

s

2EX

0πF

hep-ex/0310058

Page 11: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Sivers at Mid-rapidity?Sivers at Mid-rapidity?Need an observable which is correlated with Partonic kT. The Leading Charged Particle (LCP) is a high statistics candidate!

• Use PYTHIA 6.2 to simulate pp collisions for s = 200 GeV

• Identify true LCP in event with 0.4 < pT < 5 GeV

• Calculate vector sum of Initial Partonic kT

• Calculate opening angle, , between LCP and kT directions

(degrees)

kT=kT1+kT2

LCP

kT = kT1+kT2

PY

TH

IAP

YT

HIA

2.5/1

Uses True LCP

Page 12: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Correlation is Kinematic Effect dependent on

T

TT

LCPp

kkR 21

Region I → R < 0.8Region II → 0.8 < R

< 1.3Region III → 1.3 < R

< 1.8Region IV → R > 1.8

Correlation gone for R <

0.2

(degrees)

IV

IIIIII

kT = kT1 + kT2 (GeV)

LC

P p

T (

GeV

)

PY

TH

IAP

YT

HIA

PYTHIAPYTHIA

LCP pT

kT1 + kT2

Transverse Momentum (GeV)

PY

TH

IAP

YT

HIA

Page 13: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Compare Forward o correlation with Mid-rapidity LCP

• Track partonic kT = kT1

• Find LCP in || < 1

0.4 < pT < 5 GeV

• Find leading 0 with E > 20 Gev and 3.3 < < 4.1

•Calculate opening angle, , between kT and 0 pT (LCP pT)

• Forward 0 correlation 4/1

• LCP correlation 1.4/1

• LCP correlation reduced 2x from ideal case

• Forward region → Valence Quark Sivers Functions• Mid-rapidity → Gluon Sivers Functions• 0 has stronger Correlation with Initial kT then LCP• LCP less sensitive than 0 to Collins Effect, both sensitive to higher twist effects

Forward 0

LCP

Uses Fiducial LCP

kT = kT1 ONLY

(degrees

)

PY

TH

IAP

YT

HIA

Page 14: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Mid-rapidity Leading Charged Particle Analysis

LCP

§ 1.5 Million Minbias Triggers

• Use TPC to identify charged hadron with largest pT

•0.4 < pT < 5 GeV, |η|< 1.0, s = 200 GeV

• LCP pT agrees with inclusive charged particle pT spectrum at pT > 1.5 Gev

P r e l i

m i n a r

y

P r e l i

m i n a r

y

Page 15: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Single Spin LCP Single Spin LCP AsymmetryAsymmetry

•Averaged AN for both beams

•Yellow/Blue Beam Pol = 0.2

•Error bars statistical + CNI

AN Consistent with 0

P r e l i

m i n a r

y

P r e l i

m i n a r

y

AN for charge separated LCP also consistent

with 0

Page 16: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Sivers Effect in DijetsSivers Effect in DijetsDeviations from = due to

Partonic kT

Theoretical Results by W.Vogelsang and D.Boer, hep-

ph/0312320

AN

DijetDijet

DijetDijetN

YY

YY

Pol1

A8 < pT1,2 < 12

GeV

|η1,2 | < 1

Very Sensitive to Gluon Sivers !

• Gluon = U + D / 2• Gluon = 0• Gluon = D• Gluon = D + kT

2 = 2.5

Jet #1

Jet #2

Dominated by Leading Twist!

Maximal Effects at = 0.4-0.5

This region experimentally available!

SP

Page 17: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Dijet AnalysisDijet AnalysisJet Finder

•Use Cone Jet Finder R = 0.7

•Charged Energy from TPC

•Neutral Energy from BEMC

•Use HT trigger Data

Trigger Jet

•Reconstructed from EMC and TPC

•Includes high tower trigger

•Defines energy scale and first thrust axis

•0.2 < < 0.65 and 4.2 < J1 < 6

•Et > 7 GeV Away Side Jet

•Charged particles only

•Determines second thrust axis

•-0.5 < η < 0.5

J2

J1

Requires Full Jet Reconstruction. Dihadron Analysis not sufficient!

Page 18: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

0.03

0.05

4.1 E -4

Partonic kT from Dijet Analysis

kT = <kT>2 = ET sin (σ)

ET = 13.0 0.7sys → Trigger Jet

STAR agrees

well with World

Data on Partonic

kT

σ = 0.23 ± 0.02 ±

Page 19: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Conclusions and Future Conclusions and Future PlansPlans

• Transverse Spin Collisions provide insight into partonic transverse momentum

• Need to find observables which isolate Collins, Sivers and Twist 3 mechanisms

• LCP, Dijets and Forward 0 all sensitive to Sivers effects

• Next step in Dijet analysis is spin sorting

• Plans to extend LCP analysis to include Y2003 minbias events

•Need more polarized proton running to get meaningful results from LCP and Dijet analysis !

Page 20: Constraining the Sivers Functions using Transverse Spin  Asymmetries at STAR

Dihadron AsymmetriesDihadron AsymmetriesHigher statistics and simpler analysis make Di-hadrons cheaper. But is the correlation with kT strong enough?

J1

J2

h1

h2

kT

h1+h2

Use PYTHIA 6.2 to simulate pp collisions. Find LCP and next to LCP (nLCP). Require 0.4 < pT < 5 GeV. If they are separated by 180 +/- 600 then find opening angle, , between their bisector and 1 of the initial parton kT directions. • Correlation 1.3/1 - weak for ideal case

• kT seems to point in direction of LCP

(degrees)

kT = kT1+kT2

Uses Real LCP, nLCP

PY

TH

IAP

YT

HIA