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Studies on nucleon spin at PHENIX
3rd International Conference on New Frontiers in Physics
Kolymbari, Greece
August 2, 2014
Kiyoshi Tanida (Seoul National University) for the PHENIX Collaboration
What are we aiming at?• To study proton’s spin structure• The flagship question:
“Where the proton spin comes from?”– Proton spin puzzle– Helicity distribution of partons in longitudinally polarized
protons, especially gluons– Flavor-decomposed quark helicity distribution using Ws
• What’s there in transversely polarized protons?– dq ≠ Dq– Very hot recently– Needs more than simple
collinear picture to understand
2
Helicity distributions
• Lepton deep inelastic scattering (DIS) experiments– Quasi-elastic scattering of quark and lepton at high
energies where perturbation is applicable– Reaction depends on quark spin spin structure function
Proton spin puzzle• Quark spin carries only 20-30% of the nucleon spin
spin puzzle (crisis)• What carries the rest?
– Gluon spin?– Orbital angular momentum?
LG 2
1
2
1
Our Main Goal
0.2-0.3
What we can’t know from DIS• Photon mediated sensitive to charge2
– u : d : s : g = 4 : 1 : 1 : 0– Gluon is invisible!
(c.f., indirect methods: Q2 evolution, photon-gluon fusion)
• Can we see gluons directly? Yes, what we need is a
Polarized Proton collider
6
RHIC p+p accelerator complex
BRAHMS & PP2PP
STARPHENIX
AGS
LINACBOOSTER
Pol. Proton Source
Spin Rotators
20% Snake
Siberian Snakes
200 MeV polarimeter Rf Dipoles
RHIC pC “CNI” polarimeters
PHOBOS
RHIC
absolute pHpolarimeter
SiberianSnakes
AGS pC “CNI” polarimeter
5% Snake
Coulomb-Nuclear Interference
How can we access gluons?• Typical parton level diagrams ( LO )
• What we actually measure are not partons, but fragmented hadrons– Come from different mix of partons– Parton information ( e.g., Bjorken x ) is obscured
qqqq gggg
g g
g g
gqgq
q g
q g
q
q
q
q
9
Impact on Global Analysis• Including DIS and other data as well as RHIC data
– Based on DSSV [PRL101 (2008) 072001, PRD 80 (2009) 034030]
11
Strong constraint on DG in 0.05 < x < 0.2:
ALW
u(x1)d(x2) d(x1)u(x2)
u(x1)d(x2) d(x1)u(x2)
Parity Violation AsymmetryClean flavor separationw/o fragmentation uncertainty
)0( , ),(
),(
)0( , ),(
),(
2121
21
2121
21
WW
WWL
WW
WWL
yxxMxd
MxdA
yxxMxu
MxuA
W e e
W
W measurement
W asymmetries@500-510 GeV13
ye
Central arm (e) – 2011-13 Muon arm – 2011,12
• Consistent with theories• Will be finalized soon
Transverse spin physics• Transversity dq: Due to Einstein’s relativity, not the
same as Dq – Unexplored leading twist PDF
• AN : left-right asymmetry wrt transverse polarization
xF<0 xF>0
R
L
Left
Right
15
RL
RLNA
Requirements for AN
• Helicity flip amplitude & relative phase
• In QCD, helicity is conserved if mq=0.
AN ~ asmq/pT ~ O(10-3)
in naive collinear picture
Reality
However, large AN
observed in forward
particles. WHY??
We need somethingmore
hot topic
17
PRD90 (2014) 012006
(ii) Collins mechanism: Transversity (quark polarization) × jet fragmentation asymmetry
(i) Sivers mechanism:
correlation between proton spin & parton kT SP
p
p
Sq kT,π
Possible mechanisms (ex.)
SP
kT,qp
p
Sq
Phys Rev D41 (1990) 83; 43 (1991) 261 Nucl Phys B396 (1993) 161
18
(iii) Twist 3: quark-gluon/gluon-gluon correlation A source for Sivers function Expectation: at large pT, AN ~ 1/pT
Recent results -- forward 19
• No √s dependence – scaling effect?• Same behavior for p0 & h
PRD90 (2014) 012006arXiv:1406.3541
Forward – pT dependence 20
• Twist-3 calculation (by Kanazawa & Koike): quite good– Though naïve 1/pT dependence not seen
arXiv:1406.3541
Midrapidity p0 and h
• Exceeds precision of previous result by factor of 20, extends pT range [PRL 95 (2005) 202001]
• AN is zero within 0.1% contrast with forward hadrons
• Theories must be able to explain those features at the same time.
21
PRD90 (2014) 012006
Summary & Outlook• Gluon helicity distribution
– gluon spin in this x range is not enough to explain proton helicity.
– √s=500 GeV data will come soon for lower x.
• Flavor decomposed quark distribution via W– AL are consistent with predictions from existing PDFs
– 2013 muon data will be available soon
• Transverse spin physics– Large AN seen only in forward region, independent of
collision energy– Twist-3 calculation gives a rather good agreement,
though naïve 1/pT dependence is not seen
• More results are there and still to come
22
The Relativistic Heavy Ion Collideraccelerator complex
at Brookhaven National Laboratory
PHENIXSTAR
Brahmspp2pp
24
RHIC p+p accelerator complex
BRAHMS & PP2PP
STARPHENIX
AGS
LINACBOOSTER
Pol. Proton Source
Spin Rotators
20% Snake
Siberian Snakes
200 MeV polarimeter Rf Dipoles
RHIC pC “CNI” polarimeters
PHOBOS
RHIC
absolute pHpolarimeter
SiberianSnakes
AGS pC “CNI” polarimeter
5% Snake
Coulomb-Nuclear Interference
25
13 Countries; 70 Institutions
Abilene Christian University, Abilene, TX 79699, U.S.Baruch College, CUNY, New York City, NY 10010-5518, U.S.Collider-Accelerator Department, Brookhaven National Laboratory, Upton, NY 11973-5000, U.S.Physics Department, Brookhaven National Laboratory, Upton, NY 11973-5000, U.S.University of California - Riverside, Riverside, CA 92521, U.S.University of Colorado, Boulder, CO 80309, U.S.Columbia University, New York, NY 10027 and Nevis Laboratories, Irvington, NY 10533, U.S.Florida Institute of Technology, Melbourne, FL 32901, U.S.Florida State University, Tallahassee, FL 32306, U.S.Georgia State University, Atlanta, GA 30303, U.S.University of Illinois at Urbana-Champaign, Urbana, IL 61801, U.S.Iowa State University, Ames, IA 50011, U.S.Lawrence Livermore National Laboratory, Livermore, CA 94550, U.S.Los Alamos National Laboratory, Los Alamos, NM 87545, U.S.University of Maryland, College Park, MD 20742, U.S.Department of Physics, University of Massachusetts, Amherst, MA 01003-9337, U.S. Morgan State University, Baltimore, MD 21251, U.S.Muhlenberg College, Allentown, PA 18104-5586, U.S.University of New Mexico, Albuquerque, NM 87131, U.S. New Mexico State University, Las Cruces, NM 88003, U.S.Oak Ridge National Laboratory, Oak Ridge, TN 37831, U.S.Department of Physics and Astronomy, Ohio University, Athens, OH 45701, U.S.RIKEN BNL Research Center, Brookhaven National Laboratory, Upton, NY 11973-5000, U.S.Chemistry Department, Stony Brook University,SUNY, Stony Brook, NY 11794-3400, U.S.Department of Physics and Astronomy, Stony Brook University, SUNY, Stony Brook, NY 11794, U.S.University of Tennessee, Knoxville, TN 37996, U.S.Vanderbilt University, Nashville, TN 37235, U.S.
Universidade de São Paulo, Instituto de Física, Caixa Postal 66318, São Paulo CEP05315-970, BrazilInstitute of Physics, Academia Sinica, Taipei 11529, TaiwanChina Institute of Atomic Energy (CIAE), Beijing, People's Republic of ChinaPeking University, Beijing, People's Republic of ChinaCharles University, Ovocnytrh 5, Praha 1, 116 36, Prague, Czech RepublicCzech Technical University, Zikova 4, 166 36 Prague 6, Czech RepublicInstitute of Physics, Academy of Sciences of the Czech Republic, Na Slovance 2, 182 21 Prague 8, Czech RepublicHelsinki Institute of Physics and University of Jyväskylä, P.O.Box 35, FI-40014 Jyväskylä, FinlandDapnia, CEA Saclay, F-91191, Gif-sur-Yvette, FranceLaboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS-IN2P3, Route de Saclay, F-91128, Palaiseau, FranceLaboratoire de Physique Corpusculaire (LPC), Université Blaise Pascal, CNRS-IN2P3, Clermont-Fd, 63177 Aubiere Cedex, FranceIPN-Orsay, Universite Paris Sud, CNRS-IN2P3, BP1, F-91406, Orsay, FranceDebrecen University, H-4010 Debrecen, Egyetem tér 1, HungaryELTE, Eötvös Loránd University, H - 1117 Budapest, Pázmány P. s. 1/A, HungaryKFKI Research Institute for Particle and Nuclear Physics of the Hungarian Academy of Sciences (MTA KFKI RMKI), H-1525 Budapest 114, POBox 49, Budapest, HungaryDepartment of Physics, Banaras Hindu University, Varanasi 221005, IndiaBhabha Atomic Research Centre, Bombay 400 085, IndiaWeizmann Institute, Rehovot 76100, IsraelCenter for Nuclear Study, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, JapanHiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, JapanKEK, High Energy Accelerator Research Organization, Tsukuba, Ibaraki 305-0801, JapanKyoto University, Kyoto 606-8502, JapanNagasaki Institute of Applied Science, Nagasaki-shi, Nagasaki 851-0193, JapanRIKEN, The Institute of Physical and Chemical Research, Wako, Saitama 351-0198, JapanPhysics Department, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501, JapanDepartment of Physics, Tokyo Institute of Technology, Oh-okayama, Meguro, Tokyo 152-8551, JapanInstitute of Physics, University of Tsukuba, Tsukuba, Ibaraki 305, JapanChonbuk National University, Jeonju, KoreaEwha Womans University, Seoul 120-750, KoreaHanyang University, Seoul 133-792, KoreaKAERI, Cyclotron Application Laboratory, Seoul, South KoreaKorea University, Seoul, 136-701, KoreaMyongji University, Yongin, Kyonggido 449-728, KoreaDepartment of Physocs and Astronomy, Seoul National University, Seoul, South KoreaYonsei University, IPAP, Seoul 120-749, KoreaIHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics, Protvino, 142281, RussiaINR_RAS, Institute for Nuclear Research of the Russian Academy of Sciences, prospekt 60-letiya Oktyabrya 7a, Moscow 117312, RussiaJoint Institute for Nuclear Research, 141980 Dubna, Moscow Region, RussiaRussian Research Center "Kurchatov Institute", Moscow, RussiaPNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, RussiaSaint Petersburg State Polytechnic University, St. Petersburg, RussiaSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Vorob'evy Gory, Moscow 119992, Russia Department of Physics, Lund University, Box 118, SE-221 00 Lund, Sweden
Feb 2011
The PHENIX Detector• Philosophy
– high resolution & high-rate at the cost of acceptance
– trigger for rare events
• Central Arms– |h| < 0.35, Df ~ p– Momentum, Energy, PID
• Muon Arms– 1.2 < |h| < 2.4– Momentum (MuTr)
• Muon piston calorimeter– 3.1 < |h| < 3.9
28
Forward Calorimetry: MPCMuon Piston Calorimeter (3.1 < |h| < 3.9) : lower x10-3
29
Cluster (p0 dominant) ALLDecay photon
π0
Direct photon
PT
Fra
ctio
n of
clu
ster
s
How to extract Dg(x)? (1)• p0s come from quarks and gluons of various x
Deconvolution necessary• Are we sure that we understand contribution of
partons? YES!– NLO-pQCD calculation
reproduces s well
p0@200 GeV, h~0
PRD76:051106,2007
30
How to extract Dg(x)? (2)• Practical analysis
– Assume functional form: e.g., Dg(x)=Cg(x)xa(1-x)b
– Search optimum parameters using data, including DIS.• Ex : GRSV ( M. Gluck et al., PRD 63 (2001) 094005. )
– Assume DG, other parameters are determined from DIS.– Several versions for various DG ( GRSV-std, max,
min, ... )• Several other analyses
– For the same integral, DG, Dg(x) could be very different– Our measurement mostly constrains DG[0.02,0.3]
31
Global Fit including Run9 0 ALL By S.Taneja et al (DIS2011)
ala DSSV with slightly different uncertainty evaluation approach
DSSV DSSV + PHENIX Run9 0 ALL
No node …Uncertainties decreased
A node at x~0.1 ?
32