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The Gerasimov-Drell-Hearn Sum Rule and the

Spin Struture of the Proton

G.Krein

Instituto deFsiaTeoria,UniversidadeEstadual Paulista,

RuaPamplona145, 01405-900,S~aoPaulo,SP

Reeivedon22February,2001

We present an overview of the present theoretial status of the Gerasimov-Drell-Hearn (GDH)

sumrule. Itisemphasizedtheimportaneofnearthresholds-wavephotoprodutionontributions

to the sumrule. We also disuss the experimental veriationof the sum rule, with partiular

emphasisonthereentexperimentattheMainzMirotron(MAMI).Thespinpolarizabilities and

thegeneralizedGDHsumrule,whihare ofinteresttoissuesrelated tothespinoftheprotonas

measuredathighenergies,aredisussed.

I Introdution

The responseof theinternal degreesof freedomof the

nuleontoanexternaleletromagnetieldanbe

de-sribed in terms of polarizabilities. Forreal photons,

polarizabilities and other ground-state properties an

berelated to integralsoverphotoabsorptionross

se-tionsby sumrules. Oneof themostprominent

exam-plesistheGerasimov-Drell-Hearn(GDH)sumrule[1℄,

whih provides a relationship between the anomalous

magneti moment

N

of the nuleon and the

pho-toabsorptionrosssetionsforparallelandantiparallel

alignments of the nuleon and photon heliities,

3=2

and

1=2

2

N

4 =

M 2

8 2

I

N

; (1)

where I

N

is theGDH integral,givenby

I

N =

Z

1

!

th

1=2 (!)

3=2 (!)

!

d!: (2)

The importane of the sum rule stems from the fat

that it is basedon generalpriniples of physis, suh

as Lorentz and gauge invariane, rossing symmetry,

ausalityandunitarity.

CloselyrelatedtotheGDHsumruleistheforward

spinpolarizability[2℄

= 1

4 2

Z

1

!th

1=2 (!)

3=2 (!)

! 3

d!: (3)

This quantity is related to the Ragusa

polarizabili-ties[3℄

i

; i=14,as

=

1

2 2

4

: (4)

The Ragusapolarizabilitiesappear aslow-energy

on-tantsofthetermsO(! 3

)intheexpansionofthe

Comp-Theuseofvirtualphotonsfromeletronsattering

proessesprovidesuswithevenmoredetailed

informa-tionon theinternaldegreesoffreedomofthenuleon.

Inpartiular,asweinreasethefour-momentumQ 2

of

thevirtualphotonfromthereal-photonpoint(Q 2

=0)

tolargevaluesofQ 2

,weaninvestigatethetransition

fromthenonperturbativetotheperturbativeregimeof

quantumhromodynamis(QCD).Thegeneralizations

ofreal-photonsumrulestovirtualphotonsprovidean

interestingpossibility to study this transition and the

varyingroleoftherelevantdegreesoffreedom.

In this ontribution we present an overview of the

presenttheoretialandexperimentalstatusoftheGDH

sumrule. Wealsodisussgeneralisationsofthespin

po-larizabilityand GDH sum rule. These generalizations

areofinteresttoissuesrelatedtothespinoftheproton

asmeasuredat high energies. Atthe end ofthis

on-tribution,wealsodisussageneralizationoftheBaldin

sumruleasafuntion of Q 2

and omparepreditions

basedonhiralperturbationtheoryanda

phenomeno-logialresonanemodel.

II The GDH sum rule

Untilreently,there wasnodiret measurementofthe

rosssetions

3=2 and

1=2

intheintegrandsofthe

in-tegralsabove. The situation hangedwith the reent

experiment at MAMI [4℄, whih measured the

ross-setion dierene = N

1=2

N

3=2

for photon lab.

energiesintherange200 800MeV.Beforethis

experi-ment,onehadtorelyonestimatesusingpion

(2)

The deomposition of in Eqs. (2) and (3) in

termsofphotoprodutionmultipolesisgivenas[6℄

= 8

q

k

jE

0+ j

2

+3jE

1+ j

2

+6E

1+ M

1+ jM

1+ j

2

+ jM

1 j

2

+

; (5)

whereqisthe.m. momentumofthepionandkinthe

.m. momentumofthephoton. Beauseofthe

weight-ingfator1=!inI

GDH

,itistobeexpetedthatalarge

frationofthethesumruleissaturatedbys-wave

near-threshold pion photoprodution and by (1232)

reso-nane prodution. This seemspartiularly true for ,

beauseofthe1=! 3

in theintegrandofEq.(3).

ThestatusoftheGDHsumruleuntilreentlywas,

asdisussed in Refs.[7℄ and [8℄, that there seemed to

bea severe disrepany betweenthe preditionof the

sumruleandthesaturationoftheintegralwith

photo-produtiondata. Fortheproton,forexample,thesum

rulepredits

I

p

= 204b; (6)

while the SAID multipoles, together with an old

esti-mate [9℄ of the NN ontribution, predited[7℄ I

p =

289b. AmorereentSAID analysis,SAID-SP97K,

gave[8℄

I SAID

p

= 281b: (7)

Thedisrepanybetweenthepreditionofthesumrule

andtheSAIDmultipoleswasontheorderof30%.

Veryreently, thepresentauthor together with D.

Drehsel[10℄showedthatthedisrepanyisdrastially

redued when using the HDT [11℄ multipoles, instead

oftheSAIDmultipoles. TheHDTmultipolesarebased

on xed-t dispersion relations and unitarity. In the

HDT dispersive approah the threshold region is not

inludedinthettingoffreeparameters;thethreshold

values for the s-wave amplitudes are genuine

predi-tions. The HDTanalysis islimitedto photonenergies

upto400MeV,s, p,andd wavesfor isospin1/2,and

sandpwavesforisospin3/2. Althoughthedierenes

betweentheSAID-SP97KandHDTmultipolesarevery

smallforenergiesabove400MeV,largedierenes

o-ur for the E

0+

multipole for +

prodution lose to

threshold. In Fig.1 we show the results for the

inte-grandofthesumruleusingtheHDT(solid)andSAID

(dashed)multipoles.

Figure 1. Multipole ontributions to the integrand of Ip:

(a)E

0

+,(b)M

1

+,and()all(uptoL=5)partialwaves.

Thesolidlinesorrespondto theHDTmultipoles andthe

dottedtotheSP97K-SAIDmultipoles.

The HDT multipoles lead to I

p

(1) = 196b.

Thisimpliesinahangeof20b,omparedtoSAID.If

weuse the(very)old estimateestimateofKarliner [9℄

for the two-pion ontribution, I

p

(2) = 65b, the

earlier disrepany [7℄ redues from 38 % to 28 %.

Moreover, if one uses the estimate of Ref. [12℄ of the

ontributionsbeyondone-pionprodution, 32b,

to-gether with the single-pion HDT predition, the

dis-repanyfallstoonly12%.

ThisvalueisnottoofartheresultofthereentGDH

experiment at Mainz [4℄, for energies upto 800 MeV.

Conerningtheremainingdisrepany,itwillbe

inter-esting to see the outome of the GDH experiment at

ELSAathigherenergies.

Regardingthe spinpolarizability, Eq. (3), beause

ofthe1=! 3

in thedenominator,oneexpetsthat

near-threshold s-wave pion photoprodution and (1232)

resonaneprodutionsaturate the aboveintegraleven

morerapidlythantheGDHintegral. Thiswasatually

veriedinRef.[13℄: theintegrandisalreadynegligible

at!' 500MeV.

TheHDT multipolesleadfortheproton

HDT

p

= 0:610 4

fm 4

; (8)

whiletheSP97K-SAIDgive

SAID

= 1:310 4

fm 4

(3)

The reentMainz experiment[4℄ of =

1=2

3=2

forenergieslargerthan200MeVgivesavalueof

p 1:710 4 fm 4

. TheHDTmultipolespreditthatthe

region very lose to threshold, !

th

< ! < 200 MeV,

ontributesto

p

with apositive value equalto +0:9.

Therefore,to theextentthattheHDT multipoles

pro-videanaurantedesriptionofthelow-energyregion,

one anpreditthat

p

= 0:810 4

fm 4

.

Itisinstrutivetoompare[13℄thesenumberswith

preditions of hiral perturbation theory. Two reent

alulations, Refs. [14℄and [15℄, in O(p 4

)of HBChPT

nd

p

= 3:910 4

fm 4

. Anotherreent O(p 4

)

al-ulation [16℄, whih diers from the previous two in

the waythe single-partilereduible ontributions are

treated, leads to

p

= 1:010 4

fm 4

. A

alula-tion [17℄using dispersionrelationstogetherwith large

N

argumentsleadsto

p

= 0:110 4

fm 4

.

III Generalized GDH integral

and spin polarizability

One of themany possiblegeneralizations of theGDH

sumrule[18℄tovirtualphotonsistheexpression

I 1 (Q 2 ) = M 2 8 2 Z 1 0 1 x 1+ 2 1=2 ( ;Q

2

)

3=2 ( ;Q

2

)

2 0

LT ( ;Q

2 ) d ; (10) where 0 =m +(m 2 +Q 2

)=2m is the thresholdlab

energyof one-pionprodution. Here,x

0

is the

thresh-oldvalueofx=Q 2

=2M,x

0 =Q 2 =(Mm +m 2 +Q 2 ),

and = Q=. Also,

3=2 and

1=2

are the ross

se-tionsforthesatteringof polarizedeletronson

polar-izednuleonswithparalleland antiparallelalignments

of the eletron and nuleon heliities, and 0

LT is the

longitudinal-transverserosssetion.

Contatwith deep inelastisattering experiments

an bemadebyexpressingI

1 (Q

2

)in termsofan

inte-graloverthespinstruturefuntiong

1 (x;Q 2 ) I 1 (Q 2 ) = 2M 2 Q 2 Z x 0 0 g 1 (x;Q 2 )dx = 2M 2 Q 2 1 (Q 2 ): (11)

A generalized polarizability an also be dened in

termsofeletroprodutionrosssetions

3=2 and 1=2 as[19℄ (Q 2 )= 1 4 2 Z 1 0 1=2 ( ;Q

2

)

3=2 ( ;Q

2

)

3

d : (12)

Thereisverylittleexperimentalinformationonthe

eletroprodution ross-setions in the resonane

re-gion. Thesituationwillhangein thenearfuture with

being, one has to rely on phenomenologial models.

Here, we review our reent work [20℄ [21℄ on

general-izedGDH sumrule and spinpolarizabilities. In these

worksweusedthereentlydevelopedisobarmodelfor

eletroprodution,knownasMAID. Themodeliswell

doumentedand aessible viathe Internet [22℄. It is

basedonaneetivephenomenologialLagrangianfor

Born terms (\bakground") and resonanes up to the

thirdresonaneregion. Foreah partialwavethe

mul-tipoles satisfy the onstraints of gaugeinvariane and

unitarity,andin thereal photonasetheresultsagree

wellwiththepreditionsofdispersiontheory[11℄. The

modelisabletodesribetheorretenergydependene

ofthemultipolesforphotonenergiesupto!'1GeV,

anditprovidesagooddesriptionofallexperimentally

measureddierentialrosssetionsandpolarization

ob-servables.

Figure2. Comparisonof resultsfor

1

from MAID(solid)

andHBChPT(dashed).

The preditionof MAID isshowm in Fig.??. We

ompareresultswithareentHBChPTalulation[23℄

at O(p 4

). For the proton, the result obtained in

Ref.[23℄for

1

isgivenby

1 (Q 2 )= p 4

+6:85Q 2

(GeV 2

): (13)

Beingthis aresultof aHBChPT alulation,it is

ex-peted to bevalid onlyfor small valuesof Q 2

. Inthe

FigureweomparethepreditionsofMAID(solidline)

andEq. (13)(dashed line). Is is woth mentioningthe

theMAIDresultisverylosetoreentSLACdata[20℄

atQ 2

=0:5GeV 2

. Fromthegure, itisseenthat for

Q 2

>0:05GeV 2

,theHBChPTresultbeomes

onsid-erablydierentfromtheMAIDpredition.

Forthegeneralizedspinpolizability,areent

alu-lation[19℄hasbeenmadeintheframeworkofthe

one-loopapproximationto(relativisti)hiralperturbation

theory (ChPT), supplemented by tree graphs for the

(4)

Figure3. Comparisonof resultsfor p fromMAID(solid)

andrelativistiChPT(dashed).

InFig.3weompareresultsagainwithMAID[21℄.

The most striking dierene refers to the slope of

p (Q

2

)losetotherealphotonpoint. Thepronouned

slope in

p (Q

2

) observed in the MAID result is due

to the interferene between bakground and (1232)

terms,whihhasitsthephysialorigininthe

dynami-aldressingoftheNvertex[24℄.

Insummary,oneofthestrikingfeaturesofthe

gen-eralizedGDH integralisits rapid utuationwith Q 2

andinpartiularahangeofsignat Q 2

'0:5(GeV) 2

,

whihimposessevereonstraintsonanymodelforthe

nuleonstruture. This zero-rossingseparates the

re-giondominatedbyresonane-drivenoherentproesses

fromaregionofessentiallyinoherentsatteringothe

nuleon's onstituents. A similar zero-rossingis

pre-ditedbyChPTforthegeneralizedspinpolarizability,

(Q 2

)[19℄,whilewefoundthatMAIDexludessuha

ross-overforQ 2

(1GeV) 2

.

Aknowledgments Work partially supported

FAPESPandCNPq.

Referenes

[1℄ S.B.Gerasimov,Sov.J.Nul.Phys.2,430(1966);S.D.

DrellandA.C.Hearn,Phys.Rev.Lett.16,908(1966).

[2℄ M.Gell-Mann,M.GoldbergerandW.Thirring,Phys.

Rev.95,1612 (1954).

[3℄ S.Ragusa,Phys.Rev.D47,3757 (1993);Phys.Rev.

[4℄ J. Ahrends er al. (GDH Collaboration), Phys. Rev.

Lett.84,5904 (2000).

[5℄ SAID:TheSatteringAnalysisInterativeDial-in

pro-gram,dataavailableathttp://gwda.phys.gwu.edu .

[6℄ Forareviewsee: D.Drehsel,Prog.Part. Nul.Phys.

34,181(1995).

[7℄ A.M. Sandor, C.S. Whisnant, and M. Khandaker,

Phys.Rev.D50,R6681(1994).

[8℄ R.A. Arndt,I.I. Strakovsky, and R.Workman,Phys.

Rev.C53,430(1996).

[9℄ I.Karliner,Phys.Rev.D7,2717(1973).

[10℄ D. Drehsel and G.Krein, Phys.Rev.D58, 116009,

(1998).

[11℄ O.Hanstein,D.Drehsel,andL.Tiator,Phys.Lett.B

385, 45(1996); Nul. Phys. A 399,13 (1996); Nul.

Phys.A632,561(1998).

[12℄ V.BurkertandZ.Li,Phys.Rev.D47,46(1993).

[13℄ D.Drehsel,G.KreinandO.Hanstein,Phys.Lett. B

420,248(1998).

[14℄ X. Ji, C.-W. Kao and J. Osborne, Phys. Rev.D 61,

074003(2000).

[15℄ K.B.V.Kumar,J.A.MGovernandM.C.Birse,Phys.

Lett.B479,167(2000).

[16℄ G.C.Gellas,T.R.HemmertandUlf-G.Meissner,Phys.

Rev.Lett.85,14(2000).

[17℄ Y. Tanushi, S. Saito, M. Uehara, Phys. Rev. C 60,

065213(1999).

[18℄ R. Pantforder, Investigations on the Foundation

and Possible Modiations of the

Gerasimov-Drell-Hearn Sum Rule, Ph.D. Thesis, Bonn (1997);

hep-ph/9805434.

[19℄ J.Edelmann,N.Kaiser,G.PillerandW.Weise,Nul.

Phys.A641,119(1998).

[20℄ D. Drehsel, S.S. Kamalov, G.Krein, and L. Tiator,

Phys.Rev.D59,094021(1999).

[21℄ D.Drehsel,S.S.Kamalov,G.Krein,B.Pasquini,and

L.Tiator,Nul.Phys.A660,57(1999).

[22℄ D. Drehsel, S.S. Kamalov, and L. Tiator, Nul.

Phys. A 645, 145 (1999). Data available at:

http://www.kph.uni-mainz.de/MAID/.

[23℄ X.Ji,C.-W. Kao,andJ.Osborne,Phys.Lett.B472,

1(2000).

[24℄ S. S.Kamalov and S.N. Yang, Phys.Rev.Lett. 83,

Imagem

Figure 1. Multipole ontributions to the integrand of Ip:
Figure 2. Comparison of results for
Figure 3. Comparison of results for p from MAID (solid)

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