Title: Update on Prospects for Drell Yan at RHIC
1Update on Prospects for Drell Yan at RHIC
L.C. Bland Brookhaven National Laboratory Transver
se Partonic Structure Workshop Yerevan, 26 June
2009
2Outline
- Motivation for transverse spin Drell Yan
- Requirements
- Progress towards large-y DY
3Transverse Spin Drell Yan at RHIC vs p-Sivers
Asymmetry in Semi-Inclusive Deep Inelastic
Scattering
- Important test at RHIC of recent fundamental QCD
predictions for the Sivers effect, demonstrating
- attractive vs repulsive color charge forces
- Possible access to quark orbital angular momentum
- requires very high luminosity (RHIC II)
- both STAR and PHENIX can make important,
exciting, measurements - o
Transverse-Spin Drell-Yan Physics at RHIC L.
Bland, S.J. Brodsky, G. Bunce, M. Liu, M.
Grosse-Perdekamp, A. Ogawa, W. Vogelsang, F.
Yuan http//spin.riken.bnl.gov/rsc/write-up/dy_fin
al.pdf
4Attractive vs Repulsive Sivers Effects Unique
Prediction of Gauge Theory !
Simple QED example
Drell-Yan repulsive
DIS attractive
Same in QCD
As a result
5 Experiment SIDIS vs Drell Yan SiversDIS -
SiversDY Probes QCD attraction and QCD
repulsion
HERMES Sivers Results
RHIC II Drell Yan Projections
0
Sivers Amplitude
M. Diefenthaler arXiv0706.2242 (final results
from HERMES just released arXiv0906.3918)
0
0.1 0.2 0.3 x
6Rapidity and Collision Energy Transverse Spin
Asymmetries for the DY Processhttp//spin.riken.b
nl.gov/rsc/write-up/dy-final.pdf
Light mass DY, Mggt 4 GeV/c2 Rapidity
distributions for different ?s
Large rapidity acceptance required to probe
valence quark Sivers function, also where
p?p?pX transverse spin asymmetries are found to
be large at RHIC.
7Benchmarking Simulations
pp ? J/?X ? ll-X, ?s200 GeV
PHENIX, PRL 98(2007) 232002
mm- 1.2lthlt2.2
ee- hlt0.35
J/? is a critical benchmark that must be
understood before Drell-Yan
8Dilepton Backgrounds
Drell-Yan
J/?
?
?
Isolation needed to discriminate open heavy
flavor from DY, and is possible at PHENIX with
planned upgrades.
9Summary of Transverse SSA Drell-Yan Requirements
- 250 pb-1 transverse polarization Drell-Yan data
sample probes Sivers function sign relative to
SIDIS. - Isolation required to discriminate low-mass DY
from open-heavy flavor. - Large rapidity will require tracking for
charge-sign discrimination. - Likely optimal at ?s 500 GeV, given
demonstrated luminosity - Useful to pursue DY measurement where ANgt0 is
found for p?p?pX - Large rapidity will require benchmarked
simulations to establish tracking requirements.
Benchmarking starts with J/? (see below).
10LuminosityRun-9 performance
Source RHIC Collider Projections, W. Fischer et
al. (2009)
- Challenges remain to be overcome to realize the
best-case scenarios - Luminosity increases at ?s500 GeV relative to
?s200 GeV were realized - Depolarizing resonances in RHIC will require new
tunes to reduce their impact
11LuminosityFuture Projections
Source RHIC Collider Projections, W. Fischer et
al. (2009)
- Luminosity projections for ?s 500 GeV are
sufficient for transverse-spin DY - Improved polarization would be useful to achieve
sufficient accuracy
12STAR Detector
Forward Meson Spectrometer commissioned/operated
in RHIC run 8.
Cluster-pair triggered readout of Forward Time
Projection Chamber in ongoing RHIC run 9.
13From FPD To FMS
- 1264 Lead Glass Detectors
- Full azimuthal coverage for 2.5 lt ? lt 4
FPD Prior to Run 8
FMS Run 8 and beyond
14FMS Detector
C.Perkins, QM09
- 20x more acceptance than previous forward
electromagnetic calorimeters at STAR
Geometric Efficiency J/Psi xF
FPD
FMS
- Increased acceptance not only increases pion
yields and kinematic range but also give much
higher geometric efficiency for high-xF J/Psi
15Field Effects
- Does the signal survive the field?
- Radial and Azimuthal fields impart impulses in
the F direction - These impulses are small and in opposite
directions (they nearly cancel each other) - Field effects on our signal are small
C.Perkins, DNP08
16FMS Minbias Simulations and Association Analysis
- Simulation
- PYTHIA 6.222 full GEANT simulations
- 9.2 nb-1 Integrated Luminosity
- Fast J/? generator full GEANT simulations
- Data
- Plot includes lt 1 of full data set
- Reconstructed quantities match generated
quantities quite well
- Full simulation models Mpair data very well
C.Perkins, QM09
17Forward pp J/? 2-Cluster Analysis
Reconstructed 2-cluster invariant mass
- Fit with Gaussian Polynomial
- Gaussian Fit Parameters
- µ 3.083 0.017 GeV/c2
- s 0.028 0.011 GeV/c2
- ?2/d.o.f. 24.6/25
- Significance from fit
- 2.1 s
- Background Simulation
- Needs more statistics
- Normalized to integral of data
- Cuts Applied
- Epair gt 60.0 GeV
- energy sharing, Zpair lt 0.7
- Isolation Radius
C.Perkins, QM09
- pair mass background modeled well by simulation
- significance of J/? not large here, but including
requirements on pT,cluster further reduces
background by suppressing low-pT p0 production.
18Forward pp J/? 2-Cluster Analysis
Reconstructed 2-cluster invariant mass / ( 6
pb-1 Sampled Luminosity)
C.Perkins, QM09
- Fit with Gaussian Offset
- Gaussian Fit Parameters
- µ 3.080 0.020 GeV/c2
- s 0.082 0.026 GeV/c2
- ?2/d.o.f. 20.83/26
- Significance from fit
- 4.5 s
-
- Cuts Applied
- E_pair gt 60.0 GeV
- Z?? lt 0.7
- Isolation Radius
- 0.4 Dh-Df
- pT_cluster gt 1.0 GeV/c
- high-xF J/? may have implications for intrinsic
charm at large Bjorken-x in proton - use to benchmark simulations for future
transverse-spin Drell-Yan experiment
19Forward pp J/? 3-Cluster Analysis
- Reconstructed invariant mass of candidate ?C ?
J/? ? events
- Peak Counts 8.40 2.88
- 2.9 s Significance
- µ 2.97 0.025 GeV
- s 0.070 0.025 GeV
- ?2/d.o.f. 0.7 with 14 points fit.
- Significance depends on background model
- 2.9 s significance with currently estimated
background.
C.Perkins, QM09
20Why does high-xF intrinsic heavy flavor matter?
- Diffractive Higgs production at the LHC via QQ in
proton - May provide a clear signal for Higgs production
due to small background - How can high-xF intrinsic heavy flavor happen?
- Not from Gluon Splitting (extrinsic heavy flavor)
- Heavy quarks are expected to be multi-connected
to the valence quarks within a proton and appear
at large x via
Phys.Rev. D73 (2006) 113005
QED
QCD
- Can intrinsic heavy flavor expectations be tested
experimentally?
21Status/Plan of Large-xF DY
- Large-xF J/? production has been observed from
bare large-y calorimeter response in RHIC run 8. - Cluster-pair trigger is operational for acquiring
large-y tracking data in RHIC run-9. Pending
analysis, requirements for future DY can be
established (e.g., fast-tracking inside solenoid,
space points in front of FMS). - Sufficient luminosity for pp ?s500 GeV
collisions has been established further
development of polarization is required, as is
measurement of AN(xF) for p?p?p0X at ?s500 GeV
and measurement of large-xF J/? and U production
at ?s500 GeV, to bracket light-mass DY region. - Technical solutions exist for fast tracking
inside solenoid (GEM trackers) and space points
in front of FMS (forward meson preshower).
Construction to span 2.5lthlt4 region is required,
and could be completed in 2 years, pending
approval. - RHIC schedule is oversubscribed ? DY would be
after RHIC run 11 (gt2011). - Run-10 will be AuAu energy scan for
deconfinement critical point search, and AuAu at
?sNN200 GeV. - Run-11 is expected to be polarized pp, with
unknown mix of ?s200,500 GeV and
longitudinal/transverse polarization.
22Backup
23PHENIX Detector
- p0/g/h detection
- Electromagnetic Calorimeter (PbSc/PbGl)
- High pT photon trigger to collect p0's, hs, gs
- Acceptance hlt0.35, f 2 x p/2
- High granularity (1010mrad2)
- p/ p-
- Drift Chamber (DC) for Charged Tracks
- Ring Imaging Cherenkov Detector (RICH)
- High pT charged pions (pTgt4.7 GeV).
- Relative Luminosity
- Beam Beam Counter (BBC)
- Acceptance 3.0lt hlt3.9
- Zero Degree Calorimeter (ZDC)
- Acceptance 2 mrad
- Local Polarimetry
- ZDC
- Shower Maximum Detector (SMD)
EMCal
24Energy Dependent Corrections
C.Perkins, QM09
- Reconstructed photon energies were individually
corrected as dictated by detector simulations.
- Electromagnetic shower shape profiles and
analysis code have been successfully adapted from
FPD for use with FMS - When the p0(h) mass is properly reconstructed, so
is its energy