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Current Results and Future Prospects from. Kieran Boyle (RIKEN BNL Research Center). Topics. Longitudinal Spin Current results Future plans/ideas W physics Plans A first look at Run9 data Transverse Spin Current Results Future plans. RHIC and PHENIX. A few standard slides. RHIC. - PowerPoint PPT Presentation
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Kieran Boyle 1
Kieran Boyle
(RIKEN BNL Research Center)
Current Results and Future
Prospects from
Kieran Boyle 2
Topics• Longitudinal Spin
– Current results– Future plans/ideas
• W physics– Plans– A first look at Run9 data
• Transverse Spin– Current Results– Future plans
Kieran Boyle 3
RHIC and PHENIX
A few standard slides
Kieran Boyle 4
RHIC
BRAHMS & PP2PP (p)
STAR (p)PHENIX (p)
AGS
LINAC BOOSTER
Pol. Proton Source
Spin RotatorsPartial Siberian Snake
Siberian Snakes
200 MeV PolarimeterAGS Internal Polarimeter
Rf Dipoles
RHIC CNI (pC) PolarimetersAbsolute Polarimeter (H jet)
++ +−+−+−−−+ +−− +−
Year s [GeV] L [pb-1] P [%] FoM (P4L)
2003 200 0.35 27 0.0019
2004 200 0.12 40 0.0031
2005 200 3.4 49 0.20
2006 200 7.5 57 0.79
2006 62.4 0.08 48 0.0042
2009 500 ~10 ~35 ~0.150
2009 200
Longitudinal
Year s [GeV] L [pb-1] P [%] FoM (P2L)
2002 200 0.15 15 0.0034
2005 200 0.16 47 0.035
2006 200 2.7 51 0.7
2006 62.4 0.02 48 0.0046
2008 200 5.2 46 1.1
Transverse
In progress
Kieran Boyle 5
PHENIX Detector
BBC
ZDCZDC
EMCaldetection• Electromagnetic Calorimeter (PbSc/PbGl):
• High pT photon trigger to collect trigger to collect 0's, ’s, ’s
• Acceptance: ||x • High granularity (~10*10mrad2)
• Drift Chamber (DC) for Charged Tracks• Ring Imaging Cherenkov Detector (RICH)
• High pT charged pions (pT>4.7 GeV).W± from e± • EMCal: triggering and energy determination • DC: Sign determinationW± from ±
• Muon Identification (MuID)• Tracking (MuTR)• Triggering (RPC and MuTrig Upgrades)Relative Luminosity and Local polarimetry• Beam Beam Counter (BBC)
• Acceptance: 3.0< 3.9• Zero Degree Calorimeter (ZDC)
• Acceptance: ±2 mrad
Kieran Boyle 6
Constraining G
Current Longitudinal Spin Program
G2 Gq q2
Hard Scattering Process
2P22xP
1P
11xP
0
with ~25%, G not as well constrained, L?
Kieran Boyle 7
Why ALL?
• If f = q, then we have this from pDIS• So roughly, we have
+- =
+++
+=
From ep (&pp)(HERA mostly)
pQCD NLOFrom e+e-(& SIDIS,pp)
Kieran Boyle 8
pQCD worksarXiv:0704.3599 [hep-ex]
0 @ 200 GeV Direct @ 200 GeV
Kieran Boyle 9
ALL Results
Large number of independent probesAccepted in PRL: arXiv:0810.0694
Kieran Boyle 10
Focus on 0
• Why 0?– Nothing special about 0 physically– Similar to other single hadron or jet measurements– Pions are abundantly produced in p+p collisions 0 ~99% of the time
– PHENIX triggering on high pT photons ensures large sample
– Fragmentation Function is also reasonably well known• Will get better with BELLE data
– Marquee measurement in the age of
low luminosities.
Kieran Boyle 11
Constraining G• Vary G in GRSV fit, and then generate ALL.
• Calculate 2 for each expectation curve, and plot profile
Use combined Run5 and Run6 results
arXiv:0810.0694
Kieran Boyle 12
Recent Global Fit: DSSV• PRL 101, 072001(2008)• First truly global analysis of polarized DIS, SIDIS
and pp results• PHENIX s = 200 and 62 GeV data used (PRELIMINARY 2006)• RHIC data significantly constrain G in range 0.05<x<0.3
• Experimental systematic uncertainties must be included taking into account correlations.
• Theoretical uncertainties must be considered. See recent paper.
Kieran Boyle 13
Systematic Uncertainty Impact• Consider impact
of dominant uncertainties:– Polarization– Relative luminosity
• Polarization has negligible impact on G constraint
• Relative luminosity though small (4.6x10-4) is not neglible
G(syst) = 0.1
Accepted in PRL: arXiv:0810.0694
Kieran Boyle 14
Parameterization Uncertainties
Parameterization choice
• Vary g’(x) =g(x) for best fit, and generate many ALL
• Get 2 profile• At 2=9 (~3), we find consistent constraint:
-0.7 < G[0.02,0.3] < 0.5
Our data are primarily sensitive to the size of G[0.02,0.3].
Kieran Boyle 15
Scale Uncertainty
Theoretical Scale Uncertainty: 0 cross section is described by NLO pQCD
within sizable uncertainty in theoretical scale • How does this affect G constraint?• Vary scale in ALL calc. 0.1 uncertainty for positive constraint Larger uncert. for negative constraint
Kieran Boyle 16
Direct Photon G Constraint• Dominated by quark-gluon
Compton scattering• Distinct process from other current RHIC probes• At Leading Order
• Calculate most probable x(gluon) for given pT
– Monte Carlo
• Get A1p from DIS experimental result
– PRD 60 (99) 072004
• Partonic asymmetries calculable in pQCD– Phys.Rept.59:95-297,1980
R. Bennett’sThesis
~80%
Kieran Boyle 17
G/G from Direct Photon• Current data are ~10 pb-1, so very limited
statistics• If we get expected luminosities and
polarizations at 200 (and in future) 500 GeV, will offer significant constraint.
R. Bennett’sThesis
Kieran Boyle 18
Future for PHENIX G
Lower x, correlations and Higher Luminosity
Kieran Boyle 19
s=500 GeV• Higher s allows access to lower x• For W program, we need significant luminosity (~300
pb-1)
• For ALL, if polarization is >60%, this will allow for a very accurate measurement of G.
present (0)x-ranges = 200 GeV
Extend to lower x at s = 500 GeV
Extend to higher x at s = 62.4 GeV
• We will of course repeat our measurements
• ALL expected to be small
• Systematic uncertainties will become significant at low pT, where lowest x is reached.
Kieran Boyle 20
Expectation for 0 ALL
Full spin program
• Limited at high pT due to merging of photons as opening angle decreases
• Relative luminosity systematic uncertainty must be reduced.
Kieran Boyle 21
Particle Correlations• Due to limited acceptance, Jet-Jet measurement is
extremely difficult in PHENIX.• Two particle correlations can be measured, though
this introduces two fragmentation functions.• Also will look at photon-hadron correlations.
Kieran Boyle 22
Silicon Vertex Detector (VTX)• Four layers (2 pixel, 2 stripixel)
• Allow access to G through distinct processes– Heavy flavor via displaced vertices– Gamma-Jet (isolated trigger photon in EMCal, charged energy from VTX)
Heavy flavor• DCA resolution
~50m• c/b separation
by c
|jet| < 1.2jet
PHENIX Direct || < 0.35
Jet
Life time (c) D0 : 125 m B0 : 464 m
DCA
ppD
B
e
e
Simulation
Gamma Jet• Large
acceptance:||<1, ~2 for
Kieran Boyle 23
W-bosons at PHENIX
Accessing the flavor dependent quark sea spin distributions
l+
Kieran Boyle 24
Two ways to get W• Central Rapidity: ||<0.35
– Measure electron in the central arms EMCal– Determine charge sign from tracking
• Forward/Backward: 1.2<<2.4– Measure muon in muon arms– W dominates muon signal above 20 GeV– For measurement, we require:
• Ability to trigger on high momentum • Hadron background reduction
– Upgrading PHENIX for this purpose
μ μ ±
ee+/-+/-
W
Muon pT spectra in the Muon Arms(2000 [1/pb], from PYTHIA5.7)
Kieran Boyle 25
W
• Expectations based on 300 pb-1, 60% pol.
• Different rapidities select different polarized quark and anti quark distributions
Forward AL μ+ Forward AL μ-
Backward AL μ+ Backward AL μ-
Kieran Boyle 26
W
MuID- only existing trigger- no momentum selectivity..
<Muon Trigger Upgrade><Muon Trigger Upgrade>• MuTr FEE Upgrade (MuTRG)• Install RPC (Resistive Plate Chamber)• Install additional Pb absorber
26
Rapidity: 1.2 < <2.2 (2.4)
Kieran Boyle 27
We in Central Arms• Cross section of e+/- from W
& π+/- in the PHENIX acceptance.
• Expected asymmetry of W (assuming 70 % polarization, no background or detector resolution included)
e+
e-
pi+pi+
pions: NLO pQCD calculation from W. VogelsangW: RHICBOS (Nadolsky, Yuan)
<Charged hadron rejection>EMCal intrinsic: 50-150Shower profile: 2-4 Isolation cut: ~10Total: 1000-6000
Kieran Boyle 28
We Run 9 • Polarization ~35%• Luminosity ~10%
Measure cross section• alpha [rad.] ~ 0.1/
mom [GeV/c]• “energy / mom < 3” cut
appliedeta
pi0
negative charge
positive charge
Energy v.s. Inclination of the track
Energy dist. (Black: +, Red: -)
Only analyzed part of data set
Kieran Boyle 29
Event Display of High energy events
3. W detection @ PHENIX 29
Found W candidates.
Analysis is under way!
Kieran Boyle 30
Transverse Spin results
Kieran Boyle 31
AN from 0, h+/- (<0.35)
PRL 95, 202001 (2005)
Analysis with high statistics 2006+2008 data in progress Smaller statistical uncertainties (more than factor of 7 improvement)
Higher pT data points possible
PHENIX transverse running at 2002
PHENIX transverse running in 2005
Kieran Boyle 32
Constrain gluon Sivers effect0 AN from PHENIX 2002 data
Upper bound for gluon Sivers function that is consistent with PHENIX results, assuming vanishing sea contribution
Anselmino et al, Phys. Rev. D 74, 094011
Kieran Boyle 33
Forward 0 AN
Forward asymmetries contain mixture of• Sivers• Transversity x CollinsPHENIX 0 results available for s=62GeV
Analysis of large 2008 s=200 GeV dataset – AN of 0 and – 5.2 pb-1, 46% Polarization– work in progress
PLB 603,173 (2004)
Process contribution to 0, =3.3, s=200 GeV
Kieran Boyle 34
SSA from di-hadron production
SSA from Interference Fragmentation Function (IFF)
• Measure di-hadron asymmetry with hadron pairs in central arm (0,h+) (0,h-), (h+,h-)
•
• Transversity extraction will become possible with Interference Fragmentation Function measurement in progress at BELLE
Jaffe, Jin and Tang, PRL 80 (1998) 1166Bacchetta and Radici, Phys. Rev. D 74, 114007 (2006)
• Two different theoretical models gave different prediction of mass dependence
• Sign change is not observed in HERMES/COMPASS results
Kieran Boyle 35
IFF: Definition of Vectors and Angles
1 2
1 2
1 2
, : momenta of protons
, : momenta of hadrons
( ) / 2
: proton spin orientation
A B
h h
C h h
C h h
B
P P
P P
P P P
R P P
S
= +
= −
ur ur
ur ur
ur ur ur
ur ur ur
ur
1hPur
2hPur
APur
BPur
CPur
BSur
pp hhX↑ →
1 2hadron plane: ,
scattering plane: ,
h h
C B
P P
P P
ur ur
ur ur : from scattering plane
to hadron planeRφ : from polarization vector
to scattering plane Sφ
Bacchetta and Radici, PRD70, 094032 (2004)
2 CRur
sin sin( )R SA A φ φ φ= −
Kieran Boyle 36
Added statistics from 2008 running No significant asymmetries seen at mid-rapidity.
SSA from di-hadron production
Kieran Boyle 37
Added statistics from 2008 running No significant asymmetries seen at mid-rapidity.
SSA from di-hadron production
Kieran Boyle 38
Summary• PHENIX has measured ALL of numerous final state particles
which can constrain G• While neutral pions have been used by DSSV, other
measurements, while statistically limited individually, will make the result more robust.
• Future G constraint will also include particle correlation. PHENIX is well prepared to measure photon-hadron correlations, and with the VTX, can look at photon jet.
• PHENIX is on schedule for the W physics program, and are studying results from the recent engineering 500 GeV run.
• PHENIX has a number of transverse spin measurements, from the recent long transverse runs, and will have more to come.
Kieran Boyle 39
Backups
Kieran Boyle 40
Measuring ALL
Helicity Dependent Particle Yields , , , , , etc
(Local) Polarimetry Relative Luminosity (R=L++/L+-) ALL
+ - = Opposite helicity =
++ = Same helicity
+
+=
Kieran Boyle 41
Kieran Boyle 42
Fragmentation Functions• Cross sections in e+e- for 0, +, -, +, -,
• 60 fb-1 data below b resonances• 600 fb-1 data at b resonances
– Can be used for high z data if statistics are an issue
– Not an issue for above particles
• Data will be systematically limited
Kieran Boyle 43
Estimating Average x gluonR. Bennett’sThesis