Uncertainty determination of Polarized gluon distributions from Global Analysis of World Data
Gluon polarization and jet production at STAR
Transcript of Gluon polarization and jet production at STAR
![Page 1: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/1.jpg)
Gluon polarization and jet production at STAR
Pibero Djawotho for the STAR Collaboration Texas A&M 4 June 2013
![Page 2: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/2.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
The proton spin sum rule
• Quark polarization ΔΣ ≈ 0.3 from polarized deep inelastic scattering
• Gluon polarization (ΔG) and orbital angular momentum (L) are poorly constrained
• A primary charge of RHIC spin physics ⇒ map Δg(x)
LGS +Δ+ΔΣ==21
21
2
![Page 3: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/3.jpg)
Jet Transverse Momentum (GeV/c)0 5 10 15 20 25 30 35 40 45 50
Subp
roce
ss F
ract
ion
0
0.1
0.2
0.3
0.4
0.5
0.6
qq+qq'
qg
gg
jet+X→pp=200 GeVs
NLO CTEQ6M R=0.7
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
Polarized pp collisions at RHIC
LLba
baLL a
ffffA ˆΔΔ
∝+
−=
−+++
−+++
σσσσ
Δf: polarized parton distribution functions
For most RHIC kinematics, gg and qg dominate, making ALL for jets sensitive to gluon polarization.
3
![Page 4: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/4.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
RHIC: The World’s First Polarized Hadron Collider
• 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 depolarization
BRAHMS
PHENIX
AGS
BOOSTER
Spin Rotators (longitudinal polarization)
Solenoid Partial Siberian Snake
Siberian Snakes
200 MeV Polarimeter AGS Internal Polarimeter
Rf Dipole
RHIC pC Polarimeters Absolute Polarimeter (H↑ jet)
AGS pC Polarimeters Strong Helical AGS Snake
Helical Partial Siberian Snake
Spin Rotators (longitudinal polarization)
Spin flipper
Siberian Snakes
STAR
PHOBOS
Pol. H- Source LINAC
4
![Page 5: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/5.jpg)
STAR detector in two views
BEMC
EEMC FMS FPD TPC
BBC
• High precision tracking with the TPC • Electromagnetic calorimetry with the BEMC, EEMC, and FMS • Additional detectors for relative luminosity, local polarimetry, and minbias
triggering
ZDC ZDC
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 5
![Page 6: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/6.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
Midpoint cone algorithm (Adapted from Tevatron II - hep-ex/0005012)
• Seed energy ETseed = 0.5 GeV
• Cone radius R = √Δη2+Δφ2 = 0.7
• Split/merge fraction f = 0.5
Jet reconstruction in STAR D
etec
tor
GE
AN
T PY
TH
IA
etcpe
,,,π
γν ,,
gq,
Data jets MC jets
Part
icle
Use PYTHIA + GEANT to quantify detector response
6
R from jet axis (rad)60 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8
Frac
tion
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
jet+XApp = 200 GeVs
<0.9d-0.7<R=0.7
> = 10.32 GeV/cT
<p
> = 24.42 GeV/cT
<p
> = 34.72 GeV/cT
<p
PRD 86 032006 (2012)
![Page 7: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/7.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
2006 inclusive jet cross section
• Data well described by NLO pQCD+Hadronization+Underlying Event
preliminary
preliminary
7
![Page 8: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/8.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
2006 inclusive jet ALL
• Sampled 5.5 pb-1 at ~57% average beam polarization • STAR data rule out several previous models of gluon polarization
8
(GeV/c)T
p5 10 15 20 25 30 35
-0.02
0
0.02
0.04
0.06
0.082006 STAR DataGRSV-std
g=06GRSV g=-g6GRSV
GS-CDSSV
LLA
8.3% scale uncertainty from± polarization not shown
jet+XApp
PRD 86 032006 (2012) STAR!
![Page 9: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/9.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
• First global NLO analysis to include DIS, SIDIS, and RHIC pp data on equal footing • Finds node in gluon distribution near x ~ 0.1
de Florian et al, PRL 101 072001 (2008) DSSV – First Global Analysis with Polarized Jets
STAR
9
![Page 10: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/10.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
2009 upgrades • 2009 jet patch trigger upgrades
– Overlapping jet patches and lower ET threshold improve efficiency and reduce trigger bias
• Net increase of 37% in jet acceptance – Remove beam-beam counter trigger requirement:
• Trigger more efficiently at high jet pT • Measure non-collision background
– Increased trigger rate enabled by DAQ1000
• Improvements in jet reconstruction – Subtract 100% of track momentum from struck tower energy
(2009) instead of MIP (2006) – Overall jet energy resolution improved from 23% to 18% – Switching to anti-kT algorithm for final result
• Reduces sensitivity to underlying event effects • Collected 4 times the figure-of-merit of 2006
– Sampled 20 pb-1 at 58% average beam polarization
10
![Page 11: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/11.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 11
From 2006 to 2009
• 2009 STAR data is a factor of 3 (high-pT) to >4 (low-pT) more precise than 2006 STAR data
• Results fall between predictions from DSSV and GRSV-STD • Precision sufficient to merit finer binning in pseudorapidity
arXiv:1106.5769
![Page 12: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/12.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
2009 inclusive jet ALL
• ALL separated into two pseudorapidity ranges • Forward jets involve:
• A larger fraction of quark-gluon scattering with: • Higher x quarks that are more polarized • Lower x gluons that are less polarized
• Larger |cos(θ*)|, which reduces âLL
• ALL falls between the predictions from DSSV and GRSV-STD
12
Mid rapidity Forward rapidity
![Page 13: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/13.jpg)
New global analysis with 2009 RHIC data
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 13
Special thanks to the DSSV group!
• DSSV++ is a new, preliminary global analysis from the DSSV group that includes the 2009 RHIC ALL data (STAR inclusive jets and PHENIX π0’s)
• First experimental evidence of non-zero Δg(x) in RHIC range (0.05 ≤ x ≤ 0.2)
Δg(x,Q2 =10 GeV2)dx = 0.10−0.07+0.06
0.05
0.20∫
-0.1
0
0.1
0.2
10-2
10-1
DSSV
DSSV+
DSSV++
Q2 = 10 GeV2
x6g
x
RHIC 200 GeV
6r2
0 6g(x,Q2) dx0.2
0.05
DSSV
DSSV+
DSSV++Q2 = 10 GeV2
6r2= 2% in DSSV analysis
0
5
10
15
-0.1 0 0.1 0.2
arXiv:1304.0079
![Page 14: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/14.jpg)
2009: from preliminary towards final • STAR is switching from the
mid-point cone algorithm to the anti-kT algorithm for the final 2009 inclusive jet ALL measurement: – Anti-kT tends to have a more
rigid cone – Reconstructed jet energy is
less sensitive to nearby underlying event contributions (and pile-up)
• Provides a significant reduction in the systematic uncertainties associated with trigger and reconstruction bias
• Final results available soon Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
14
![Page 15: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/15.jpg)
Projected sensitivity for future inclusive jet ALL
• 500 GeV collisions sample smaller xT=2pT/√s • Projected statistical uncertainties • Expected asymmetries are quite small
– Control of systematics (esp. relative luminosity) will be important
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 15
Inclusive Jet A_LL for |eta|<1
-0.015
-0.010
-0.005
0.000
0.005
0.010
0.015
0.020
0.025
0 0.05 0.1 0.15 0.2 0.25 0.3 0.35x_T
A_L
LRuns 9+14 Proj (200)Run 12 Proj (500)GRSV-Std (500)DSSV (500)GRSV-Std (200)DSSV (200)
![Page 16: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/16.jpg)
Correlation measurements
x1,2 =1spT 3e
±η3 + pT 4e±η4( )
cosθ * = tanh η3 −η42
• Inclusive probes at fixed pT sample broad x range ⇒ global analysis needed to disentangle shape of Δg(x)
• Reconstructing dijet final state (jet pT and η) provides information on initial parton kinematics (x1,2 and cosθ*) at LO
• STAR is well suited for correlation measurements and full jet reconstruction with its large acceptance
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 16
![Page 17: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/17.jpg)
2006 dijet cross section
• Data shows good agreement with NLO pQCD + CTEQ6M including Hadronization + Underlying Event Corrections
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 17
![Page 18: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/18.jpg)
2009 dijet partonic coverage
STAR!
( )
( )
2tanhcos
2ln21
|ηη||θ|
ηηxxy
sxxM
epeps1x
epeps1x
43*
43
2
1
21
ηT,4
ηT,32
ηT,4
ηT,31
43
43
−=
+==
=
+=
+=
−−
x x
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 18
![Page 19: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/19.jpg)
2009 dijet ALL
• STAR data fall between predictions of DSSV and GRSV-STD
preliminary
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 19
arXiv:1107.0917 STAR!
preliminary preliminary
![Page 20: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/20.jpg)
Projected sensitivity for dijet ALL at 500 GeV
• Higher energy accesses lower xg
• Expect smaller ALL
• Projections show expected sensitivity for the ongoing 2013 run
⎟⎠
⎞⎜⎝
⎛ +±=
2exp 43
21ηη
sMx,x
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR 20
![Page 21: Gluon polarization and jet production at STAR](https://reader035.fdocument.org/reader035/viewer/2022071216/62cbbf6cb2c021788a58752e/html5/thumbnails/21.jpg)
Pibero Djawotho - INPC2013 - Gluon polarization and jet production at STAR
Summary
• STAR inclusive jet and dijet cross sections are in good agreement with NLO pQCD calculations when hadronization and underlying event effects are included
• STAR inclusive jet ALL from 2006 provides significant constraints on gluon polarization in NLO global analyses
• 2009 STAR inclusive jet ALL is factor of 3 (high-pT) to >4 (low-pT) more precise than 2006 results
– First experimental evidence for non-zero gluon polarization within the RHIC range (0.05 ≤ x ≤ 0.2)
• STAR will provide additional high-precision measurements of inclusive jet and dijet ALL during the next few years
21