Overview of spin physics results from PHENIX experiment

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Overview of spin physics results from PHENIX experiment

The 4th International Workshop of High Energy Physics in the LHC Era

Valparaiso, Chile

January 4-10, 2012

Kiyoshi Tanida (Seoul National University)

for the PHENIX Collaboration

Overview of spin physics results from PHENIX experiment

The 4th International Workshop of High Energy Physics in the LHC Era

Valparaiso, Chile

January 4-10, 2012

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?

– d q ≠ D q

– Very hot recently

– Needs more than simple collinear picture to understand

4

PHENIX

The

R

elativistic

H

eavy

I

on

C

ollider accelerator complex at Brookhaven National Laboratory

5

Brahms pp2pp

STAR

RHIC

p+p

accelerator complex

PHOBOS absolute pH polarimeter

RHIC pC “CNI” polarimeters

BRAHMS

& PP2PP

Siberian

Snakes

PHENIX

RHIC

Spin Rotators

Pol. Proton Source

LINAC

BOOSTER

STAR

AGS

Siberian Snakes

5% Snake

AGS pC “CNI” polarimeter

200 MeV polarimeter

20% Snake

Rf Dipoles

Coulomb-Nuclear

Interference

6

PHENIX Experiment

7

P ioneering H igh E nergy N uclear I nteraction E X periment

Universidade de São Paulo, Instituto de Física, Caixa Postal 66318, São Paulo CEP05315-970, Brazil

Institute of Physics, Academia Sinica, Taipei 11529, Taiwan

China Institute of Atomic Energy (CIAE), Beijing, People's Republic of China

Peking University, Beijing, People's Republic of China

Charles University, Ovocnytrh 5, Praha 1, 116 36, Prague, Czech Republic

Czech Technical University, Zikova 4, 166 36 Prague 6, Czech Republic

Institute of Physics, Academy of Sciences of the Czech Republic, Na Slovance 2,

182 21 Prague 8, Czech Republic

Helsinki Institute of Physics and University of Jyväskylä, P.O.Box 35, FI-40014 Jyväskylä, Finland

Dapnia, CEA Saclay, F-91191, Gif-sur-Yvette, France

Laboratoire Leprince-Ringuet, Ecole Polytechnique, CNRS-IN2P3, Route de Saclay,

F-91128, Palaiseau, France

Laboratoire de Physique Corpusculaire (LPC), Université Blaise Pascal, CNRS-IN2P3,

Clermont-Fd, 63177 Aubiere Cedex, France

IPN-Orsay, Universite Paris Sud, CNRS-IN2P3, BP1, F-91406, Orsay, France

Debrecen University, H-4010 Debrecen, Egyetem tér 1, Hungary

ELTE, Eötvös Loránd University, H - 1117 Budapest, Pázmány P. s. 1/A, Hungary

KFKI Research Institute for Particle and Nuclear Physics of the Hungarian Academy of Sciences (MTA KFKI RMKI),

H-1525 Budapest 114, POBox 49, Budapest, Hungary

Department of Physics, Banaras Hindu University, Varanasi 221005, India

Bhabha Atomic Research Centre, Bombay 400 085, India

Weizmann Institute, Rehovot 76100, Israel

Center for Nuclear Study, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo,

Tokyo 113-0033, Japan

Hiroshima University, Kagamiyama, Higashi-Hiroshima 739-8526, Japan

KEK, High Energy Accelerator Research Organization, Tsukuba, Ibaraki 305-0801, Japan

Kyoto University, Kyoto 606-8502, Japan

Nagasaki Institute of Applied Science, Nagasaki-shi, Nagasaki 851-0193, Japan

RIKEN, The Institute of Physical and Chemical Research, Wako, Saitama 351-0198, Japan

Physics Department, Rikkyo University, 3-34-1 Nishi-Ikebukuro, Toshima, Tokyo 171-8501, Japan

Department of Physics, Tokyo Institute of Technology, Oh-okayama, Meguro, Tokyo 152-8551, Japan

Institute of Physics, University of Tsukuba, Tsukuba, Ibaraki 305, Japan

Chonbuk National University, Jeonju, Korea

Ewha Womans University, Seoul 120-750, Korea

Hanyang University, Seoul 133-792, Korea

KAERI, Cyclotron Application Laboratory, Seoul, South Korea

Korea University, Seoul, 136-701, Korea

Myongji University, Yongin, Kyonggido 449-728, Korea

Department of Physocs and Astronomy, Seoul National University, Seoul, South Korea

Yonsei University, IPAP, Seoul 120-749, Korea

IHEP Protvino, State Research Center of Russian Federation, Institute for High Energy Physics,

Protvino, 142281, Russia

INR_RAS, Institute for Nuclear Research of the Russian Academy of Sciences, prospekt 60-letiya Oktyabrya 7a,

Moscow 117312, Russia

Joint Institute for Nuclear Research, 141980 Dubna, Moscow Region, Russia

Russian Research Center "Kurchatov Institute", Moscow, Russia

PNPI, Petersburg Nuclear Physics Institute, Gatchina, Leningrad region, 188300, Russia

Saint Petersburg State Polytechnic University, St. Petersburg, Russia

Skobeltsyn 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

13 Countries; 70 Institutions

Feb 2011

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.

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

9

PART 1:

Helicity distribution with longitudinal polarization

Helicity distribution

• 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?

1

2

1

2

D

0.2-0.3

 D

G

L

Our Main Goal

What we can’t know from DIS

• Photon mediated  sensitive to charge 2

– u : d : s : g = 4 : 1 : 1 : 0

– Gluon is invisible!

(c.f., indirect methods: Q 2 evolution, photon-gluon fusion)

13

• Can we see gluons directly?

 Yes, what we need is a

Polarized Proton collider

What we measure?

A

LL

(



)

(



)

 

 

(



)

(



)

~ (parton pol.) 2 × (a

LL in parton reaction)

14

How can we access gluons?

• Typical parton level diagrams ( LO ) gg

 gg gq

 gq qq

 qq

15

 g g g g

 q g q g

D q

D q q q

• What we actually measure are not partons, but fragmented hadrons

– Come from different mix of partons

– Parton information ( e.g., Bjorken x ) is obscured

Some examples

• Direct photon: g + q  g

+ q

– No fragmentation

– Small contamination (e.g.

` qq  gg

)

• Jet, high-p

T hadron production

– Mix of all subprocesses

– LO  highest statistics

 Good measurement with lower luminosity

• Heavy quarks (charm, bottom)

– gg→ ` qq is the main process at RHIC

• W : sensitive to quark flavors

– e.g., W + comes from

` du

16

Accumulated data

with longitudinal polarization

Year

2003 (Run 3)

 s [GeV] Recorded L Pol [%]

200 .35 pb -1 27

2004 (Run 4)

2005 (Run 5)

200

200

.12 pb -1

3.4 pb -1

40

49

2006 (Run 6)

2006 (Run 6)

2009 (Run 9)

2009 (Run 9)

2011 (Run 11)

200

62.4

200

500

500

7.5 pb -1

0.08 pb -1

16 pb -1

10 pb -1

17 pb -1

57

48

55

39

44

FOM

(P 4 L)

1.5 nb -1

3.3 nb -1

0.2 pb -1

0.69 pb -1

5.3 nb -1

1.5 pb -1

0.23 pb -1

0.64 pb -1

17

Results

p

0 A

LL

@200 GeV

18

Run5

Run6

Run9

Precision reaches O(10 -3 ), but still consistent with 0 asymmetry

How to extract

D

g(x)? (1)

• p

0 s come from quarks and gluons of various x

 Deconvolution necessary

• Are we sure that we understand contribution of partons? YES!

– NLO-pQCD calculation reproduces

 well p 0

@200 GeV, h

~0

19

PRD76:051106,2007

How to extract

D

g(x)? (2)

• Practical analysis

– Assume functional form: e.g., D g(x)=Cg(x)x a

(1-x) b

– Search optimum parameters using data, including DIS.

• Ex : GRSV ( M. Gluck et al., PRD 63 (2001) 094005.

– Assume D

G, other parameters are determined from DIS.

– Several versions for various D

G ( GRSV-std, max, min, ...

• Several other analyses

– For the same integral, D

G,

D g(x) could be very different

– Our measurement mostly constrains D

G

[0.02,0.3]

20

RHIC data

21 D

G: Global Fit

DSSV analysis

(Run 9 data not taken into account)

Phys. Rev. Lett.

101, 072001(2008)

Uncertainty estimation:

D

2 =1

D

2 /

2 =2%

Node in

D g(x)?

Global Fit including Run9

p

0

A

LL

By S.Taneja et al (DIS2011) ala DSSV with slightly different uncertainty evaluation approach

22

DSSV

A node at x~0.1 ?

DSSV + PHENIX Run9 p

0 A

LL

No node …

Uncertainties decreased

Extend x-range

different

s

p

0 at | h

|<0.35: x g distribution vs p

T bin

23

 s=62 GeV

2-2.5 GeV/c

4-5 GeV/c

9-12 GeV/c

2-2.5 GeV/c

4-5 GeV/c

9-12 GeV/c

 s=200 GeV

 s=500 GeV

p

at

s=62 GeV

p

0: PHENIX, PRD79, 012003

Very limited data sample (0.04 pb -1 , compared 2.5 pb -1 from Run2005

 s=200 GeV)

Clear statistical improvement at larger x; extends the range to higher x (0.06<x< 0.4)

Overlap with 200 GeV A

LL provides measurements at the same x but different scale (p

T

  s=500 GeV A

LL or Q 2 ) results will be available soon (from Run2009 with

L~10 pb -1 and P~0.4)

Charged hadrons

25

Forward Calorimetry: MPC

Muon Piston Calorimeter (3.1 < |h| < 3.9) : lower x

10 -3

26

Cluster ( p 0 dominant) A

LL

Decay photon

π 0

Direct photon

P

T

W measurement

A

L

W

 

D u ( x

1

) d ( x u ( x

1

) d ( x

2

2

)  D d ( x

1

) u ( x

)  d ( x

1

) u ( x

2

)

2

)

W   e   e



 



Parity Violation Asymmetry

Clean flavor separation 

W     

A

W

L

A

W

L

D u ( u ( x x

1

,

1

,

M

W

2

M

2

W

)

)

, x

1

D d d (

( x x

1

,

1

,

M

M

2

W

2

W

)

)

, x

1 x

2

( y

W

 x

2

(

 y

W

0 )



0 )

W

e in mid-rapidity

Phys. Rev. Lett. 106, 062001 (2011)

W asymmetry

e +

Run 9 data e -

29

Uncertainty is still large

More data in 2011 and from now

Forward

New Trigger System

Resistive Plate Counter

(RPC) (Φ segmented)

Trigger events with straight track

(e.g.

D strip <= 1)

SG1

30

RPC

FEE

Level 1

Trigger

Board

Trigger

MuTRG

Amp/Discri.

Transmit

Data

Merge

Trigger

5% Optical

MuTRG

ADTX 1.2Gbps

MuTRG

MRG

B

2 planes

95%

MuTr

FEE

Interaction Region

Trigger

RPC / MuTRG data are also recorded on disk.

Rack Room

Trigger efficiency

OK: plateau eff. 92%

31

Run11 data under analysis ー results coming soon

More results ... no time to show them all

Part 2:

Transverse spin physics

32

Transverse spin physics

• Transversity d q : Due to Einstein’s relativity, not the same as

D q

– Unexplored leading twist PDF

33

• A

N

: left-right asymmetry wrt transverse polarization

Left x

F

<0 x

F

>0

L 𝑝

Right

R 𝑝

A

N

L

L

 

 

R

R

Requirements for A

N

• Helicity flip amplitude & relative phase

• In QCD, helicity is conserved if m q

=0.

 A

N

~ a s m q

/p

T

~ O(10 -3 ) in naive collinear picture

Reality

However, large A

N observed in forward pions. WHY??

We need something more

 hot topic

35

(i) Sivers mechanism: correlation between proton spin & parton k

T

S

P

36

Possible mechanisms (ex.)

(ii) Collins mechanism:

Transversity (quark polarization)

× jet fragmentation asymmetry

S

P

S q p k

T,q p p p

S q k

T, π

Phys Rev D41 (1990) 83; 43 (1991) 261 Nucl Phys B396 (1993) 161

(iii) Twist 3: quark-gluon/gluon-gluon correlation

 A source for Sivers function

Expectation: at large p

T

, A

N

~ 1/p

T

– not observed so far

Forward -- MPC

p 0

A

N

37

MPC @ 200 GeV

Cluster ( p 0 dominant) A

N

38

Same tendency with other energies and experiments

Forward

h

A

N

39

Forward

h

A

N

40 same tendency with p 0

Comparison with STAR

Quite different at high x

F

Due to slightly different kinematic conditions?

Need confirmation/ deconfirmation

41

Midrapidity hadrons A

N

42

• A

N is zero within 0.1%  contrast with forward hadrons

IFF and Collins FF

Interference fragmentation function H

1

( ,

 pp

)

J. Collins, S.Heppelmann, G. Ladinsky, Nuclear Physics B, 420 (1994) 565

Quark spin h

1

A

UT

 d q

H

1

□ h

2

 quark

_

 quark h

2 h

1

Collins fragmentation function

J. C. Collins, Nucl. Phys. B396, (1993) 161 h

H

1

A

UT

 d q

H

1

 quark

_

 quark

(courtesy A. Bacchetta) h

FF measurements are ongoing at KEK-BELLE

43

Asymmetry result

44

Still need more data...

• More results ... again, no time to show them all

Part 3:

Future measurements

45

More data!

• Goal:

> 50 pb-1 @ 200 GeV, > 300 pb -1 @ 500 GeV mid rapidity p

0 forward p

0

46

MPC p

0 500 GeV

300 pb -1 P=0.55

W

 

in forward

47

More detectors – (F)VTX

• VTX (from 2011)

• FVTX (from 2012)

• Study of c & b

Gluon polarization via

VTX barrel | h |<1.2

48

• Larger acceptance

 Jet tagging

– q+g  g

+jet

– Theoretically clean channel

– Luminosity hungry

FVTX

More will be discussed by J. Seele this afternoon

Even further upgrade -- sPHENIX

49

Compact, hermetic, EM + hadron calorimetry

Forward region is important for spin physics

- A

N in forward regions

-

D g(x) in small x region

Details will be discussed by J. Seele this afternoon

Summary

• Gluon polarization

– Significant constraints on D g(x) for 0.02<x<0.3

– Extension toward lower x is important

 higher energy, forward region

• Flavor decomposed quark distribution via W

– W  e observed in central arm, muon arm follows

• Transverse spin physics

– Trying to find the mechanism to produce large A

N forward region in

– Access transversity

• More data are still to come

50

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