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Spin Physics at RHIC Towards Precision QCD Physics, KEK, March 10, 2007 Naohito SAITO (KEK)

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Presentation on theme: "Spin Physics at RHIC Towards Precision QCD Physics, KEK, March 10, 2007 Naohito SAITO (KEK)"— Presentation transcript:

1 Spin Physics at RHIC Towards Precision QCD Physics, KEK, March 10, 2007
Naohito SAITO (KEK)

2 Why Spin? Fundamental Concept in Physics
Appears in Many Different Levels Galaxy to Space-Time Structure Fundamental Quantum Number for Elementary Particles Important in Symmetry Test Parity Time Reversal

3 Proton Spin Crisis Anomaly SLAC:Pol’ electron scattering
Consistent with QM CERN:Pol’ muon Discovery of Anomaly Q-Spin Cont: DS ~ 0 DESY:Pure Proton Confirm Anomaly SLAC&CERN:Hi Precision Establish Anomaly DS ~ >> ~

4 First Crisis? Proton has gone through many crisis Spin
Mass : mu~5 MeV/c2, md~10 MeV/c2 Saved by constituent quark model Momentum : Saved by gluon momentum Spin Helicity SR: Theory guideline for separation (nf=3) (Ji, Tang, and Hoodboy)

5 Probing the Proton Structure
EM interaction Photon Sensitive to electric charge2 Insensitive to color charge Strong interaction Gluon Sensitive to color charge Insensitive to flavor Weak interaction Weak Boson Sensitive to weak charge ~ flavor Insensitive to color

6 Spin Structure Studies: Exp’mt
COMPASS Pol.m HERMES Pol.e± JLab Exp’s Pol.e- RHIC Spin Pol. pp BELLE e+e- Pol.m Beam: RICH-1 Pol.Target SM1 SM2 2-stage spectrometer LAS (Large angle) Kp SAS(Small angle)  SAS LAS Ecal1 & Hcal1 m filter 1 m filter 2 Ecal2 & Hcal2 RICH-2

7 RHIC at BNL Two independent rings: 3.83 km Max Energy Luminosity
NY City Two independent rings: 3.83 km 120 bunches/ring 106 ns bunch intvl Max Energy p-p GeV Au-Au 100/N + 100/N GeV Luminosity p - p 2x1032 cm-2s-1 (Polarized) Au-Au 2x1026 cm-2s-1 RHIC

8 RHIC:First Polarized pp Collider

9 Gluon Polarization

10 Gluon is expected to be Polarized
To compensate the Spin SR: (not necessarily) To recover QM expectation thru axial anomaly Through Q2 evolution: DS and Dg mix Dg~0.3 would be enough Dg~2 required Q2 evolution of the 1st Moment

11 History of Dg Hunting Hunting for Dg Direct Probe Indirect Probe
FNAL E704 High-pT p0 High-mass Multi-g pair DESY HERMES High-pT hadron pair Indirect Probe NLO Analysis by SMC PRL 84(00)2584 PLB261(1991)197 PRD58(1998)112002 PLB336(1994)269

12 Status of Dg/g(x) from Lepton Scat. Or w/o RHIC Spin
Photon-Gluon Fusion Process for 2-”jet” Open Charm New COMPASS results! Gluon Pol. Can be +, 0, - Courtesy Vogelsang and Stratmann

13 Constraints on Dg(x) w/ p0 Prod.
pp  p0 X is sensitive to gggg and gqgq

14 “Standard” value of DG from pre-RHIC DIS data
Constraints on DG “Standard” value of DG from pre-RHIC DIS data Assuming DG = 0

15 AAC updates (S.Kumano, M. Hirai, NS, PRD (2006)
Include J-Lab, HERMES, COMPASS new data Trial inclusion of PHENIX p0 ALL data K-factor method a la CTEQ Gluon Uncertainty significantly reduced!

16 Gluon Polarization Dg>0 preferred at large-x Dg=0.3±0.3
HERMES and COMPASS A1d data Higher-twist effects? Dg=0.3±0.3 Additional scale error of ~20% previously 0.5±1.3 If no p0 data 0.5±1.1 Additional scale error ~20%

17 Improved Constraints Newly obtained 1st moments (Q2=1 GeV2)
Dg = 0.3±0.3 With additional scale error of ~20% DS = 0.27±0.07 Still need to improve precision Dg Lq and Lg, too! GPD Compare with Ji, Tang,Hoodboy Expectation

18 Extend x Range ALL(p0) from Run 6/7 (65 pb-1) will extend x range to larger x STAR jet measurement also provides precision data 500 GeV run will cover smaller x-range FWD rapidity coverage also useful for smaller-x region W. Vogelsang

19 Prompt Photon Production
Gluon Compton Dominates 10% Contamination from Annihilation No fragmentation contribution in LO k2 P1 P2 k1 i ) ( 2 1 g q gq a x e A LL Ä D = å 1 0.001

20 Direct photon in Run-2006/7 W. Vogelsang k2 P1 P2 k1

21 Uncertain Unpolarized Glue
Valence-Q well determined Sea is uncertain at large-x Gluon is unknown at large and small-x Need direct measurement Not only for Dg but also for LHC

22 Sea Polarization

23 Sea Constraints: SDIS and QCD fit
QCD fit often assumes SU(3) symmetric sea Need to include SIDIS data Flavor separation by HERMES (talk by L. de Nardo)  important progress! Still compatible with QCD fit Significant constraints observed by de Florian et. al. Small-x issue remains

24 W Production in pp Collisions
W is produced through pure V-A Chirality is fixed  ideal for spin structure studies W couples to weak charge ~ flavor Flavor is (almost) fixed  ideal for flavor structure studies Parity Violating Asymmetry AL : J. Soffer et al.

25 Sea Constraints: RHIC W Prospects
Clear flavor separation Weak charge ~ flavor Clear spin information Left handed current only Start in 2009! The 1st Commission starts tomorrow! Projected statistical precision

26 Transverse Spin Physics

27 Single Transverse Spin Asymmetries
Fermilab E-704 reported Large Asymmetries AN Could be explained as Transversity x Spin-dep fragmentation (Collins effect), Intrinsic-kT imbalance (Sivers effect) , or Twist-3 (Qiu-Sterman, Koike) Or combination of above Left Right

28 BRAHMS Results on AN BRAHMS observed Large AN in charged pion production Similar Trend to E704, but deviation from ZERO starts earlier? Need to explore further!

29 More from BRAHMS p+ K+ K- p p- Pion Kaon Proton “+”>0 “-” <0
“-” >0 !! Proton “+” = 0 “-” > 0

30 RHIC Spin Roadmap submitted to DOE, Feb. 11, 2005 http://spin. riken
Year P(%) Weeks (Com/Ph) Lumi CM Energy Goals 2002 15 8 (5/3) 0.5 pb-1 200 GeV Transverse Spin 2003 30 0.35 pb-1 Longitudinal Spin Gluon Polarization? 2004 40 5(5/0) 0.15 pb-1 RHIC Commissioning Pol. Gas Jet Target 2005 50 10 3.8 pb-1 410 GeV Gluon Pol/Transv. Commissioning 2006/7 70 13+10 ~120 pb-1 0.1 pb-1 62.4 GeV 500 GeV 2008/9 10+10 ~150 pb-1 ~180 pb-1 W-Physics/Transv.

31 Past and Future of RHIC Spin Luminosity
Lost Future

32 Asymmetries calculated for RHIC
RHIC Luminosity should be improved to realize these measurements…

33 Summary No final answer yet… but qualitatively new picture of spin structure is emerging! RHIC is still catching up Kodaira-san’s prediction We would like to contribute to precision QCD physics by providing experimetal results from RHIC, and J-PARC.


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