alessandro bravar s u m m a r y xi th advanced research workshop spin-05, dubna, september...

90
Alessandro Bravar S U M M A R Y S U M M A R Y XI XI th th Advanced Research Workshop Advanced Research Workshop Spin-05, Dubna, Spin-05, Dubna, September 27-October 1, 2005 September 27-October 1, 2005

Post on 15-Jan-2016

215 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Alessandro Bravar

S U M M A R YS U M M A R Y

XIXIthth Advanced Research Workshop Advanced Research Workshop

Spin-05, Dubna, Spin-05, Dubna,

September 27-October 1, 2005September 27-October 1, 2005

Page 2: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

SPIN at High Energies: Workshops in SPIN at High Energies: Workshops in DubnaDubna

First – 1981 under the Chair of Lev Iosifovich Lapidus (1927-1986), prominent scientist who laid down the fundamentals of high energy spin physics Biannual workshops (in odd

years, between Spin Symposia) in Protvino and (1997, 2001, 2003) Dubna

Page 3: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

SOME DUE WORDS …SOME DUE WORDS …Workshop supported by- Russian Foundation for Basic Research- International Committee of Spin Physics Symposia - JINR

Many thanks to Anatoli Efremov, and the organizing committeefor organizing this very interesting and stimulating meetingand also for the very good weather

85 talks: experiments and new results, future, theory,spin technology

Page 4: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

This workshopThis workshopdedicated to the memory ofdedicated to the memory ofProf. Mikhail Petrovich Rekalo (1938-2004)Prof. Mikhail Petrovich Rekalo (1938-2004)

Prominent scientist who made important contributions to the spin physics (talk by I.M. Sitnik)

In particular – early studies of T-odd spin asymmetries : currently popular subject to be much discussed at this Workshop

Page 5: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

GENERAL OUTLINE …GENERAL OUTLINE …

proton spininclusive, semi-inclusive, gluon polarization, transversity

transverse spin -> SSATMD, Sivers, Collins, Cahn, … effectsSivers in Drell-Yan ?

Generalized Parton DistributionsDVCS, DVMP, … -> Lq

elastic scatteringHigh Energy, Medium and Lowbinary reactions

spin technologyAcceleartion, sources, targets, polarimeters, …

future

Page 6: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Proton Spin “puzzle”Proton Spin “puzzle”

The Spin of the nucleon made of:

|p = ½ = ½ + G + Lq + Lg

= u + d + s Spin of Quarks

G Spin of Gluons

Lq, Lg Orbital angular momentum

Naïve expectations: quarks carry all the nucleon spin = 1+ relativistic effects = 0.6, Lq = 0.4

but … EMC (’89): = 0.12 ± 0.09 ± 0.014 s = 0.19 ± 0.03 ± 0.05 consisten with 0 “Spin crisis”

s < 0 generated by axial anomaly large G > 0 curiosity: existence of proton spin first deduce from specific heats of H2

Page 7: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

q(x)

q(x)

Tq(x)

momentum distribution

helicity distribution

transversity distribution

Parton Distribution Parton Distribution FunctionsFunctions3 distribution functions are necessary to describe

the structure of the nucleon at LO:

all of equal importance !

h1(x) decouples from leading twist DISbecause helicity of quark must flip

NO MIXTURE WITH GLUON

g(x,Q2)=

g(x,Q2)=

and of course Gluons

Page 8: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

inclusiveinclusive

Page 9: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Precision DIS data Precision DIS data PDFs PDFs

Un

po

lari

zed

DIS

Str

uct

ure

Fu

nct

ion

(x,Q

2 )

Parton Model F2

p(x,Q2) = ½ ei2[qi (x,Q2) + qi (x,Q2)]

Only half the integral momentum of a high-energy proton comes from q and q;

scaling violations constrain the gluon (x,Q2)-dependence.

however, still big uncertaintyfor G(x) at large x !

Page 10: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Polarized DIS dataPolarized DIS data

Only ~20-30% of proton spin arises from q and q helicity preferences

(); limited info on scaling violations, on shape or integral of gluon helicity preference g(x,Q2).

g1p = ½ ei

2 [qi (x,Q2) + qi (x,Q2)] Parton Model

Page 11: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

THE COMPASS THE COMPASS SPECTROMETERSPECTROMETER

Scifi, Silicon

SM1

SM2RICH1

Polarised Target

E/HCAL1

Muon Wall 1

Muon Wall 2,MWPC

SPS 160 GeV beam

Micromegas, SDC, Scifi

Straws, Gems

MWPC, Gems, Scifi, W45 (not shown)

E/HCAL2Hodoscopes

Page 12: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

A1 and g1 deuteronA1 and g1 deuteron Windmolders

Page 13: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Windmolders

Page 14: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

New analysis of g1 dataNew analysis of g1 data Stamenov

Page 15: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Stamenov

Page 16: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Although both our and DGLAP formulae lead to x- asymptotisc ofRegge type, they predict different Q2 -asymptotics: our predictionIs the scaling

2/222 1 /~g

xQwhereas DGLAP predicts the steeper x-behavior and the flatter Q2 -behavior:

)(21 )(ln(1/x) ~ Qg DGLAP

x-asymptotics is checked with extrapolating available exp data to x 0.

Agrees with our values of Contradicts DGLAP

Q2 –asymptotics has not been checked yet.

our calculations

DGLAP fit

Conclusion: Small x behaves as perturbative !

ErmolaevSStructure of standard DGLAP inputs for initial tructure of standard DGLAP inputs for initial

parton densities and the role of the singular termsparton densities and the role of the singular terms

Page 17: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Gluon Polarization Gluon Polarization GG

Page 18: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

RHIC: the “Polarized” ColliderRHIC: the “Polarized” Collider

BRAHMS & PP2PP

STARPHENIX

AGS

LINACBOOSTER

Pol. Proton Source

Spin Rotators

Strong Snake

Siberian Snakes

200 MeV polarimeter

AGS inelastic polarimeter

Rf Dipoles

RHIC pC “CNI” polarimeters

PHOBOS

RHIC

absolute pHpolarimeter

SiberianSnakes

During 2005 run:~ 50% Polarization Lmax = 1031 s-1cm-2 @ s 200 GeV

AGS pC “CNI” polarimeter

Partial Snake

Page 19: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

The RHIC ExperimentsThe RHIC Experiments

STAR

BRAHMS

pp2pppolarimeters

Page 20: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Hadron – Hadron CollisionsHadron – Hadron Collisions

ˆˆˆ LLa

factorization !D(z)

P1

P2

S1

S2

qgqgge ̂:..for most processesNLO calculations / predictions available

ALL a

ab

b ˆ (

a

b c X)

Page 21: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

00 and prompt- and prompt- -section @ -section @ = = 00

prelim

inar

y

-section result consistent withNLO pQCD calculationsover 8 orders of magnitudefavors a larger gluon-to-pion FF

pp+Xppo+X

important confirmation of theoretical foundations for spin program

pQCD describes result very well !

Kawall & Okada

Page 22: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

First First AALLLL measurement inclusive measurement inclusive

p + p o + X, ~ 0

gqgq

qqqq

gggg

o

pT (GeV/c)

● `03 + `04 combined

inclusive o production:mixture of gg / gq / qqscatteringspT dependence

expect much more precise data andlarger pT range (`05 run)

prelim

inar

y

Page 23: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

G from Incl. JetsG from Incl. JetsMixture of gg / gq / qq scatterings

– sensitive to gluon polarization

– large -section high statistics with low L

– reconstruct JETS via TPC pT for charged

hadrons + EMC ET for EM showers

p+p, s=200 GeV STARSTAR

jet cone=0.4, 0.2<jet<0.8

prelim

inar

y

gggg

gqgq

qqqq

G

G

G

G

q

q

q

q

G

G

q

q

Hallman

Page 24: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Prompt Photon ProductionPrompt Photon Production

Gluon Compton dominates Small Background from

Annihilation No fragmentation contribution at

LO)(

)(

)(

)(

)(

22

22

1

1 qgqaxqe

xqe

xg

xgA LL

ii

i

ii

i

LL

large quark polarization for x > 0.2 large analyzing power

A1

Hallman

Page 25: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

BedferG

Page 26: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Bedfer

Page 27: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Bedfer

Page 28: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

semi – inclusivesemi – inclusiveandand

quark polarizationquark polarization

Page 29: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

B. Dressler et al. Predictions

s = 500 GeV

s = 500 GeV

SIDIS sensitivity reduced by fragment- ation functions and eq

2 weighting

qq (flavor) Sea Polarizationqq (flavor) Sea Polarization

Semi-Inclusive DIS: e + N e’ + h + X

W ± Production at RHIC

{

{

Page 30: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

27.6 GeV e+/e-

The HERMES experimentThe HERMES experiment

0.002 < x < 0.9 0.1 < Q2 < 15 GeV2

p/p ~ 1-2% < 0.6 mrad

Lepton ID with ~98%Hadron contamination <0.5%

Contalbrigo

Page 31: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

)Q,(q

q

(z)Ddz)Q(x,q'e

(z)Ddz)Qq(x,e)Q(x,A 2

qq'

hq'

22q'

hq

22q2h

1 x

In semi-inclusive deep inelastic

scattering the hadron tags

the flavour of struck quark

Derive purity of tag from unpolarized data (fragmentation functions)

Hadron asymmetries (measured)

Known quantities(from other data)

Polarized Parton Distribution Functions

!

QPA

Flavour decomposition of spinFlavour decomposition of spinKey issue: role of sea quarks in nucleon spin

Page 32: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

results perfectly consistent with inclusive fits: 2/dof =0.6…1.6 for BB(SU3-sym) and GRSV-valence

Quark polarisationsQuark polarisations

first 5-flavour extraction

[PRL92, 012005, 2004; PRD71, 012003, 2005]

• no significant sea quark polarisation

• in measured x-range (0.023-0.6):

0.0430.002 u -

0.0350.054 d -

0.0340.028 s

Contalbrigo

Page 33: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Difference Asymmetry in SIDISDifference Asymmetry in SIDISChristova

Page 34: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Christova

Page 35: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Flavor-Tagged Quark Polarizations via Flavor-Tagged Quark Polarizations via WW PV in W production

W produced through pure V-Achirality is fixed !

+ no fragmentation ambiguity limited x range

AL~u/u(x) ~ 0.7-0.9 at large-x

Requires large luminosity ands = 500 GeV

)()()()(

)()()()(

baba

babaWL xuxdxdxu

xuxdxdxuA

Page 36: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Transverse SpinTransverse Spinin hadronic interactionsin hadronic interactions

Page 37: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Transverse Single Spin Transverse Single Spin AsymmetriesAsymmetries

Fermilab E-704 reported Large Asymmetries AN Could be explained as

– Transversity X Spin-dependent fragmentation (Collins effect),

– Intrinsic-kT imbalance + Lq (Sivers effect)

GeV 4.19at sXpp

Page 38: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Sivers vs. CollinsSivers vs. Collins

Sivers effect [Phys Rev D41 (1990) 83; 43 (1991) 261]:Correlation between the proton spin (Sp), momentum (Pp) and transverse momentum (kT) of the unpolarized partons inside. The unpolarized parton distribution function fq(x,kT) is modified to:

Collins effect [Nucl Phys B396 (1993) 161]:

Correlation between the quark spin (sq), momentum (pq) and transverse momentum (kT) of the pion. The fragmentation

function of transversely polarized quark q takes the form:

qPP

qpPqq

NqqqPqq

)()k(x,ƒΔ

21

)k(x,ƒ),(x,ƒkPS

kPSSk

πq

πqqNqπ

kp

kpssk

)()k(z,D)k(z,D),(z,D /q/q/q 2

Page 39: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Melis

Page 40: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Melis

Page 41: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Melis

Page 42: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

• pQCD calculations consistent with measured large- cross sections

• transverse single-spin effects observed for s = 200 GeV pp collisions large xF

Collins effect transversity Sivers effect orbital angular momentum

Forward Forward 00 Production p Production p+p +p oo+X+XSTARSTAR

prelim

inary

Morozov

prelim

inary

Page 43: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

AANN(p(pTT) in run3+run5 at ) in run3+run5 at √s=200 GeV√s=200 GeV

Combined statistics from run3 and run5 allowed to distinguish nonzero effect in AN(pT) plot

There is an evidence that analyzing power at xF>0.4 decreases with increasing pT

Theoretical prediction’s needed to compare – constrain on Sivers function?

STARSTAR

Morozov

Page 44: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

AANN of Jet k of Jet kTT

STAR projections for 30 pb1 (4pb-1), Pbeam=70% (50%)

pp di-jet + X s = 200 GeV 8 pT(1,2) 12 GeV |(1,2)| 1.0

D.

Bo

er

& W

. V

og

els

an

g

pre

dic

tion

s

Search for spin-dependent transverse motion preferences inside proton (related to parton

Lorbit ) via predicted spin-dependent deviation (not power-suppressed) from back-to-back

alignment of di-jet axes study unique to RHIC spin: Access Sivers function

0

2

h

A probe to access to Sivers functions (=left/right asymmetry in the kT of the partons ).

Hallman

Page 45: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

What about What about polarization … polarization …E 704

Page 46: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Transversity andTransversity andTransverse SpinTransverse Spin

in leptoproductionin leptoproduction

Page 47: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Tensor charge (’91 – ’92):

in analogy with:

Soffer inequality (95):

Leader sum rule (04):

in analogy with:

TransversityTransversity

In the last ten years: great development in

the theory of transversity remarkable role of

ΔTq(x), notably complementary to Δq(x)

In the last few years: role of the kt structure

functions clarified (Cahn and Sivers effects, …) )()(

2

1)( xqxqxq TT

)()( xqxqdxg TTT

)()( xqxqdxg A

gqq

zqq

T Lxqdx,,,

)(2

1

2

1

zz LGS 2

1

Key features of transversity:• probes relativistic nature of quarks• no gluon analog for spin-1/2 nucleon• different Q2 evolution and sum rule

than Δq(x)• sensitive to valence quark

polarization

Page 48: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Measuring Measuring ΔΔTTq(x)q(x)

Hard scattering (e.g. GSI)

–Drell-Yan

Hard scattering (e.g. RHIC)

–Drell-Yan

–Single Spin Asym (e.g. p↑p→X)

SIDIS(e.g. COMPASS and HERMES )

Chiral-odd: requires another chiral-odd partner

FF (x) qΔT

q Δ qΔ TT NN NN

q Δ qΔ TT

Inclusive DIS ppl+l-X

lpl’hX

impossible direct measurementΣΔTq(x) ·ΔTq(x)

convolution withspin dependentfragment. func.

lpl’h1h2X

Bradamante

Page 49: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Transversity MeasurementTransversity Measurement

Drell-Yan production of lepton pairs– clean, but requires high

luminosity

– combination of q and q

– large analyzing power aTT

but q small

* / Z

l+

l

ii

ii

TTTT xqxqe

xqxqeaA

)()(

)()(

21

2

21

2

Page 50: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Efremov

Page 51: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Prokudin

Page 52: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Efremov

Page 53: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

COLLINS and SIVERS COLLINS and SIVERS

ASYMMETRIESASYMMETRIES2002 data only

systematic errors are smaller than the quoted statistical errors

Collins

Sivers

Bradamante

Deuteron target

Page 54: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Collins and Sivers MomentsCollins and Sivers MomentsKorotkov

proton target

Page 55: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Prokudin

Page 56: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

SIVERS ASYMMETRIESSIVERS ASYMMETRIESCOMPASS2002 data

M. Anselmino, M. Boglione, U. D'Alesio, A. Kotzinian, F. Murgia and A. ProkudinExtracting the Sivers function from polarized SIDIS data and making predictionsarXiv:hep-ph/0507181

Bradamante

Page 57: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Efremov

Page 58: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Sissakian

Page 59: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Prokudin, Efremov,Sissakian

Page 60: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Efremov

Page 61: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

G P D sG P D sand Land Lqq

Page 62: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Kroll

Page 63: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Kroll

t 0

Page 64: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Kroll

Page 65: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

uV quarksdV quarks

Kroll

Page 66: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Experimental access to GPDsExperimental access to GPDs

Exclusive meson electroproduction:

– Vector mesons (0):

– Pseudoscalar mesons ():

Deeply virtual Compton scattering (DVCS):

),,( and ),,( txEtxH ),,(

~ and ),,(

~txEtxH

DVCS Bethe-Heitler

)()( 22BH

*DVCSDVCS

*BHDVCSBH ττττ||τ||τeNeNdσ

Page 67: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Experimental access to DVCSExperimental access to DVCS)()( 22

BH*DVCSDVCS

*BHDVCSBH ττττ||τ||τeNeNdσ

Page 68: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Beam-Spin Asymmetries in DVCSBeam-Spin Asymmetries in DVCS

Proton Deuteron

Contalbrigo

Page 69: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Transverse Target-Spin Asymmetries in DVCSTransverse Target-Spin Asymmetries in DVCS

Sensitive to Ju

Contalbrigo

Page 70: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

elastic scatteringelastic scattering

Page 71: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

AANN for for ppp p pp pp @ 100 GeV @ 100 GeV

prel

imin

ary Im r5 = 0.002 0.029

Re r5 = -0.006 0.007

2/ndf = 10 / 12

uncertainty on the( = 0.03) parametercan change at the same level

hadhad

p

had

m

tsr 3155 2)(

with hadronic

spin-flip

stat + sys errors used in fits

hadronic spin – flip contribution consistent with zero (1 level)

in the simplest assumption:spin-flip prop. to non-flip ampli.

Bravar

4321*52 Im

4),(

sdtd

tsAN

NA

Page 72: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

AANNNN for for pppp pp pp @ 100 GeV @ 100 GeV

prel

imin

ary

source ofsystematic errors:

1 PT2 = 3 %

2 from backgrounds and event selections

~ 0.0013 rel. luminosity ~ 0.001

similar to stat. errors

NNB

T

TBTNN PPP

A

2

11

ANN basically 0 double spin – flip amplitudes (2 and 4)

are very small / do not contribute in this region

statistical errors only

Bravar

Page 73: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Elastic Elastic pppp Scattering Scattering s = 200 GeVs = 200 GeV

Preliminary

r5 e5 im5 m5

t Im

Kanavets

Page 74: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

spin technology:spin technology:

acceleration of polarized proton beamsacceleration of polarized proton beams

polarized sources and targetspolarized sources and targets

polarimeterspolarimeters

Page 75: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Spin Precession in Laboratory Frame:(Thomas [1927], Bargmann, Michel, Telegdi [1959])

dS/dt = (e/m) [(GB + (1+G) B] S G = 1.91 E

Lorentz Force

dv/dt = (e/m) [ B ] v

For pure vertical field Spin rotates Gtimes faster than motion, sp = G

Spin depolarization resonances due to transverse magnetic fields:

Imperfection resonance (magnet errors and misalignments, closed orbit errors, …):G = sp = n

Intrinsic resonance (vertical focusing fields - quadrupoles, finite beam emittance, …):

G = sp = Pn ±y

Spin DynamicsSpin Dynamics

B

S

v

Shatunov

Page 76: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Siberian Snake OperationSiberian Snake Operation

Partial Snake (AGS)– rotate around beam direction

– compensate for imperfections

– use an RF dipole to compensate forintrinsic resonances

Full Snake (with 2 rotators - RHIC)– rotate around two orthogonal

axes in the accelerator plane(i.e. x and y comp. separately)

– compensate for imperfectionsand intrinsic resonances

Page 77: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Siberian “ Snake ”Siberian “ Snake ”

Invented in 1974 by Derbenev and Kondratenko

Beam Trajectory while rotating Spin Direction~ 3D image of “snake”

Page 78: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

AGS Polarization during AGS Polarization during accelerationacceleration

raw

asy

mm

etry

= A

N

PB

12+ 36- 36+G = 1.91 Ebeam

depolarizing

resonances:

intrinsic: G =

imperfection: G = n

each point = 50 MeV step

48-

red line: simulation of polarizationlosses assuming constant AN

Page 79: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Imperfection Resonances: Imperfection Resonances: GG = n = npartial snake (AGS) =imperfection resoance

if snake sufficiently strong (5% enough in AGS) spin is fully flippedwhen crossing an imperfection resonance with no polarization loss

for G n, spin “oscillates” around stable direction, which is tilted from the vertical

S

S

S

SS

S

G = n G = n + 1/2

1

2

3

Page 80: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Intrinsic Resonances: Intrinsic Resonances: GG = n = nPP + +

S

S

N

N

quadrupole

betatron oscillation of frequency

if spin precession “in phase” with

betatron oscillation G = when crossing the quadrupoledepolarizing kicks adddepolarizing resonance condition

Q

Q

Q Q

FODO section

“AGS”

to be in phase with betatron oscillation over a closed orbit spin must precess n + times

in a periodic accelerator spin “in phase” with betatron oscillation when crossing same quadrupole in consecutive FODO section if

G = nP + Polarization losses reduced / avoided by forcing a full spin reversal (flip) usingan RF dipole

Page 81: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

OPPIS High Intensity HOPPIS High Intensity H Source Source

> 80 %polarization

15 1011

protons / pulseat the source(500 A, 300 s)

6 1011

protons/pulseat end of LINAC

Page 82: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

COMPASS OD magnetCOMPASS OD magnet

Solid angle:

from 70 mradto 180 mrad

+30% FOM

2006: new target magnet by OD

Page 83: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

The Atomic H Beam The Atomic H Beam SourceSource

separationmagnets(sextupoles)

H2 dissociator

Breit-Rabipolarimeter

focusingmagnets(sextupoles)

RF transitions

holding field magnet

recoil detectorsrecord beam intensity100% eff. RF transitionsfocusing high intensityB-R polarimeter

OR

Pz+ OR Pz

-

H = p+ + e-

Page 84: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Setup for Setup for ppC scattering – C scattering – the RHIC the RHIC polarimeterspolarimeters

recoil carbon ions scattered around 90o

detected with Silicon strip detectors

polar acceptance± 1.5o around 90o

2 72 channels read out with WFD

very large cross section very fast measurements

statistics per measurement (~ 20 106 events) allows detailed analysis

beamdirection

1

34

5

6

RHIC 2 rings

2

Si strip detectors(ToF, EC)

~36cm

Ultra thin Carbon ribbon Target

(3.5g/cm2 , < 10m)rightleft

rightleft

NB NN

NN

AP

1

recoil

Alekseev

Page 85: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

futurefuture

Page 86: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

J-PARCJ-PARC(Japan-Proton Accelerator Research Complex)(Japan-Proton Accelerator Research Complex)

High intensity proton machine @ 50 GeV

Saito

Page 87: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Spin physics program in the U70 polarized proton beam:Spin physics program in the U70 polarized proton beam:

1. AN and ANN in elastic scattering [high pT2]

2. Precision measurement of single-spin asymmetry in inclusive charged hadron production in pp and pA collisions at different production angles

3. Miscellaneous spin parameters (A,DNN,ALL) in hyperon production

4. Transversity in Drell-Yan muon pairs

5. Double-spin asymmetry ALL in Charmonium production (∆G/G gluon polarization through 2 if gluon-gluon fusion is significant)

Vasiliev

Page 88: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Alessandro Bravar

Facilty for Antiproton and Ion Research (GSI, Darmstadt, Germany)

-Proton linac (injector)-2 synchrotons (30 GeV p)-A number of storage rings Parallel beams operation

Contalbrigo

Page 89: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Principle of spin filter methodPrinciple of spin filter methodP beam polarizationQ target polarizationk || beam direction

σtot = σ0 + σ·P·Q + σ||·(P·k)(Q·k)

transverse case:

Q0tot

longitudinal case:

Q)( ||0tot

For initially equally populated spin states: (m=+½) and (m=-½)

Unpolarized anti-p beam

Polarized H target

Contalbrigo,Nikolaev

Page 90: Alessandro Bravar S U M M A R Y XI th Advanced Research Workshop Spin-05, Dubna, September 27-October 1, 2005

Conclusions ?Conclusions ?Very very exciting “spin” times are ahead of us !

In the next year expect plenty of new data from RHIC, COMPASS, et al.

It has been a very nice week here in Dubna !

Thanks again to Anatoli for organizing this very exciting workshop !

Hope to see each other in Kyoto - Spin06 and again in Dubna in ’07 !

Have a safe trip home !

Thank you for your patience andmy sincere apologies to all that have not been mentioned in my talk

Sandro