Jet Production in Polarized pp Collisions at RHIC

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Jet Production in Polarized pp Collisions at RHIC Carl A. Gagliardi Texas A&M University

Jet Production in Polarized pp Collisions at RHIC Carl A. Gagliardi Texas A&M University for the Collaboration STAR Outline • • Carl Gagliardi – DIS 2008 – Jets in pp at RHIC Introduction 2005 results 2006 results Looking ahead 1

Origin of the proton spin? Polarized DIS: 0. 2~0. 3 Poorly Constrained Three recent

Origin of the proton spin? Polarized DIS: 0. 2~0. 3 Poorly Constrained Three recent fits of equality: – ΔG = 0. 13 ± 0. 16 – ΔG ~ 0. 006 – ΔG = -0. 20 ± 0. 41 all at Q 2 = 1 Ge. V 2 Leader et al, PRD 75, 074027 • A primary goal of the RHIC Spin program is to determine the gluon polarization distribution Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 2

Polarized pp collisions at RHIC f: polarized parton distribution functions Partonic fractions in jet

Polarized pp collisions at RHIC f: polarized parton distribution functions Partonic fractions in jet production at 200 Ge. V 0 10 20 30 p. T(Ge. V) Carl Gagliardi – DIS 2008 – Jets in pp at RHIC For most RHIC kinematics, gg and qg dominate, making ALL for jets sensitive to gluon polarization. 3

RHIC: the world’s first polarized hadron collider RHIC p. C Polarimeters Absolute Polarimeter (H

RHIC: the world’s first polarized hadron collider RHIC p. C Polarimeters Absolute Polarimeter (H jet) BRAHMS PHOBOS Siberian Snakes PHENIX STAR Spin Rotators (longitudinal polarization) - Pol. H Source Spin flipper Spin Rotators (longitudinal polarization) Solenoid Partial Siberian Snake LINAC Helical Partial Siberian Snake BOOSTER AGS 200 Me. V Polarimeter AGS Internal Polarimeter AGS p. C Polarimeters Rf Dipole Strong Helical AGS Snake • Spin varies from rf bucket to rf bucket (9. 4 MHz) • Spin pattern changes from fill to fill • Spin rotators provide choice of spin orientation • “Billions” of spin reversals during a fill with little if any depolarization “Thousands of millions” Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 4

STAR detector E-M Calorimeter Projection Chamber Time of Flight Carl Gagliardi – DIS 2008

STAR detector E-M Calorimeter Projection Chamber Time of Flight Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 5

Jet reconstruction in STAR GEANT PYTHIA Particle Detector Data jets MC jets Midpoint cone

Jet reconstruction in STAR GEANT PYTHIA Particle Detector Data jets MC jets Midpoint cone algorithm (Adapted from Tevatron II - hep-ex/0005012) • Seed energy = 0. 5 Ge. V • Cone radius in - • R=0. 4 with 0. 2 < < 0. 8 (2005) • R=0. 7 with -0. 7 < < 0. 9 (2006) • Splitting/merging fraction f=0. 5 Use PYTHIA + GEANT to quantify detector response Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 6

Jet production at RHIC STAR PRL 97, 252001 • Jet structure at 200 Ge.

Jet production at RHIC STAR PRL 97, 252001 • Jet structure at 200 Ge. V is well understood • Mid-rapidity jet cross section is well described by p. QCD over 7 orders of magnitude Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 7

2005 inclusive jets ALL systematics (x 10 -3) Reconstruction + Trigger Bias 2 -5

2005 inclusive jets ALL systematics (x 10 -3) Reconstruction + Trigger Bias 2 -5 (p. T dep) Non-longitudinal Polarization 0. 1 -0. 8 (p. T dep) Relative Luminosity 0. 94 Backgrounds 0. 70 p. T systematic [-5. 4%, +6. 7%] Neutral Energy Fraction • Reconstruction bias: combination of steeply falling spectrum and ~25% jet ET resolution • Trigger bias: non-uniform sampling of gg, qg, and qq processes • Will illustrate impact on ALL with 2006 data Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 8

2005 inclusive jets ALL STAR hep-ex ar. Xiv: 0710. 2048 Model calcs from: Jager

2005 inclusive jets ALL STAR hep-ex ar. Xiv: 0710. 2048 Model calcs from: Jager et al, PRD 70, 034010 200 Ge. V 0. 2 < η < 0. 8 • Comparison to predictions within the GRSV framework with various input values of ΔG demonstrate sensitivity Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 9

Limits on ΔG from 2005 jet results STAR hep-ex ar. Xiv: 0710. 2048 GRSV

Limits on ΔG from 2005 jet results STAR hep-ex ar. Xiv: 0710. 2048 GRSV DIS • Significant new constraints on ΔG when compared to predictions derived from one global fit to DIS data Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 10

Other global analyses xΔg(x) at Q 2 = 10 Ge. V 2 • There

Other global analyses xΔg(x) at Q 2 = 10 Ge. V 2 • There are many other global analyses of the polarized DIS data Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 11

Additional ALL predictions for 2005 • Many predictions for ALL vs. p. T •

Additional ALL predictions for 2005 • Many predictions for ALL vs. p. T • Is the sensitivity unique to GRSV? Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 12

Comparison to other global analyses STAR • The STAR data exclude a broad range

Comparison to other global analyses STAR • The STAR data exclude a broad range of models that have ΔG larger than that in GRSV-std • The counterexample is GS-C, which is negative at large x, has a node near x ~ 0. 1, and has a large first moment at small x Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 13

2006 data Improved figure of merit Ø Luminosity : Ø Polarization: Ø Barrel EMC

2006 data Improved figure of merit Ø Luminosity : Ø Polarization: Ø Barrel EMC coverage: 2 4. 7 pb-1 50% 60% (online polarization) [0, 1] [-1, 1] In addition Ø Jet cone radius: 0. 4 0. 7 Ø -0. 7 < jet axis < 0. 9 Ø Neutral energy fraction < 0. 85 Ø Increased trigger thresholds Ø Inclusion of Endcap EMC towers Ø Improved tracking at large | | Ø Shielding from backgrounds Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 14

Jet reconstruction and trigger bias for 2006 data Step 1: Use PYTHIA+GEANT to estimate

Jet reconstruction and trigger bias for 2006 data Step 1: Use PYTHIA+GEANT to estimate the p. T shift from detector jets to particle jets Step 2: Simulate the difference in ALL between particle and detector jets for various gluon polarization scenarios Particle jets Shifted detector jets Detector jets • • Maximum deviation determines ALL systematic Confidence level calculations take account of any residual Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 15

2006 inclusive jets ALL STAR Model curves calculated with cone radius 0. 7 and

2006 inclusive jets ALL STAR Model curves calculated with cone radius 0. 7 and -0. 7 < < 0. 9 200 Ge. V -0. 7 < < 0. 9 ALL systematics (x 10 -3) Reconstruction + Trigger Bias [-1, +3] (p. T dep) Non-longitudinal Polarization ~ 0. 03 (p. T dep) Relative Luminosity 0. 94 Backgrounds 1 st bin ~ 0. 5 else ~ 0. 1 p. T systematic 6. 7% • Statistical uncertainties are 3 -4 times smaller than in ’ 05 data for p. T > 13 Ge. V/c Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 16

Limits on ΔG from 2006 jet results STAR GRSV DIS • Within the GRSV

Limits on ΔG from 2006 jet results STAR GRSV DIS • Within the GRSV framework: – GRSV-std excluded with 99% CL – ΔG < -0. 7 excluded with 90% CL Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 17

Looking beyond inclusive ALL measurements • Inclusive ALL measurements at fixed p. T average

Looking beyond inclusive ALL measurements • Inclusive ALL measurements at fixed p. T average over a broad x range. • Need a global analysis to determine the implications • Can hide considerable structure if Δg(x) has a node Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 18

DSSV – first global analysis with polarized jets de Florian et al. , ar.

DSSV – first global analysis with polarized jets de Florian et al. , ar. Xiv: 0804. 0422 [hep-ph] • The first global NLO analysis to include inclusive DIS, SIDIS, and RHIC pp data on an equal footing • Finds a node in the gluon distribution near x ~ 0. 1, but with the opposite phase from GS-C Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 19

The next few years: di-jets and Δg(x) STAR Mass 2005 preliminary di-jet distributions Rapidity

The next few years: di-jets and Δg(x) STAR Mass 2005 preliminary di-jet distributions Rapidity |cos( *)| Ratio • Di-jets provide direct access to parton kinematics at LO Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 20

Projected di-jet sensitivity for the 2009 run Rel FOM ~ 70% x 1 ~

Projected di-jet sensitivity for the 2009 run Rel FOM ~ 70% x 1 ~ 0. 33 x 2 ~ 0. 044 GS-C x 1 ~ 0. 45 x 2 ~ 0. 16 x 1 ~ 0. 27 x 2 ~ 0. 27 • Assumes 50 pb-1 of 200 Ge. V pp collisions with 60% polarization Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 21

Conclusions • STAR inclusive jet ALL measurements have excluded extreme gluon polarization scenarios •

Conclusions • STAR inclusive jet ALL measurements have excluded extreme gluon polarization scenarios • Over the next few years, STAR di-jet measurements will provide direct information about Δg(x) • STAR will also obtain complementary information about Δg(x) from γ + jet • Stay tuned! Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 22

Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 23

Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 23

Double longitudinal spin asymmetry, ALL N : Spin dependent yields (# of reconstructed jets)

Double longitudinal spin asymmetry, ALL N : Spin dependent yields (# of reconstructed jets) P : Beam polarization (measured by RHIC Polarimeter) R : Relative luminosities between different spin states Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 24

STAR detectors for jet measurements § Time Projection Chamber | |<1. 4 tracking §

STAR detectors for jet measurements § Time Projection Chamber | |<1. 4 tracking § Barrel EM Calorimeter | |<1 triggering & calorimetry § Endcap EM Calorimeter 1. 09< <2 triggering & calorimetry § Beam-Beam Counters 3. 4<| |<5 triggering, luminosity, local polarimetry Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 25

Other global analyses xΔg(x) at Q 2 = 10 Ge. V 2 Carl Gagliardi

Other global analyses xΔg(x) at Q 2 = 10 Ge. V 2 Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 26

Additional ALL predictions for 2005 ALL Carl Gagliardi – DIS 2008 – Jets in

Additional ALL predictions for 2005 ALL Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 27

Estimating the non-jet background Data Monte Carlo Charged Energy Fraction Data Carl Gagliardi –

Estimating the non-jet background Data Monte Carlo Charged Energy Fraction Data Carl Gagliardi – DIS 2008 – Jets. Charged Energy Fraction in pp at RHIC Charged Energy Fraction • Non-jet backgrounds stand out in the data as single-jet events that have a small charged energy fraction • Isolate the background in the ratio of mono-jet to di-jet events vs. charged energy fraction 28

ALL vs. run index for 2006 data STAR Preliminary Carl Gagliardi – DIS 2008

ALL vs. run index for 2006 data STAR Preliminary Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 29

False asymmetries in 2006 data STAR Preliminary • Longitudinal single-spin (parity-violating) asymmetries are consistent

False asymmetries in 2006 data STAR Preliminary • Longitudinal single-spin (parity-violating) asymmetries are consistent with zero, as expected at this precision Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 30

Inclusive jet ALL for fixed values of ΔG • Calculations by Stratmann and Vogelsang

Inclusive jet ALL for fixed values of ΔG • Calculations by Stratmann and Vogelsang within the GRSV framework Carl Gagliardi – DIS 2008 – Jets in pp at RHIC 31