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(1)

High Density QCD

M.B. Gay Duati

InstitutodeFsia,UniversidadeFederaldoRioGrande doSul

CaixaPostal 15051,CEP91501-970, PortoAlegre,RS,Brazil

Reeivedon19April,2001

ThedynamisofhighpartonidensityQCDispresentedonsidering, inthedoublelogarithm

ap-proximation,thepartonreombinationmehanismbuiltintheAGLformalism,developedinluding

unitarityorretionsforthenuleonaswellfornuleus. Itisshownthattheseorretionsare

un-der theoretial ontrol. The resulting non linear evolution equation is solved inthe asymptoti

regime,andaomprehensivephenomenologyonerningDeepInelastiSatteringlikeF2,FL,F

2 .

F

2 =lnQ

2

,F A

2 =lnQ

2

,et,ispresented. TheonnetionofourformalismwiththeDGLAPand

BFKLdynamis,andwithotherperurbative(K)andnonperturbative(MV-JKLW)approahesis

analisedindetail. Thephenomenaofsaturationduetoshadowingorretionsandtherelevaneof

thiseetinionphysisandheavyquarkprodutionisemphasized. Theimpliationstoe-RHIC,

HERA-A,andLHCphysisandsomeopenquestionsarementioned.

I Introdution

ThedynamisofthehighdensityQuantum

Chromody-namis (hdQCD)isoneofthepresentmosthalleging

openquestionsinhighenergyphysis. Theintense

the-oretial and experimental ativity towardsthe

under-standingofsmallx(smallfrationofprotonmomentum

arried by the struk parton) QCD takes plae from

Deep InelastiSattering(DIS)at HERA[1℄to heavy

ions ollisions (HIC) at RHIC [2℄. This kinematial

regime willalsobetestedatLHC inanearfuture[3℄.

Important ontribution to the interest of the eld

is due to the puzzling result obtained by HERA at

small-x (x 10 2

) [4℄ for the proton struture

fun-tionF

2 (x;Q

2

). Thisfuntion was observedto inrease

dramatially as x gets smaller (Fig. 1). In the

re-gion of moderate Bjorken x (x 10 2

) the

Opera-tor Produt Expansion (OPE)methods aswell asthe

Renormalization Group Equations (RGE) have been

applied suessfully [5℄. The evolution of quark and

gluondistributionfuntionsgivenbytheDGLAP

equa-tions[6℄isbasedonthesummingoftheleadingpowers

of

s lnQ

2

1,

s

ln(1=x)<<1,

s

<<1,where

s is

thestrongouplingonstant. Theleadingln(1=x)

on-tributions is thease forthe BFKLequation [7℄. The

proedureknownasthedoubleleadinglogarithmi

ap-proximation(DLA)orrespondsinaxialgaugesto

gen-eratethelogarithmsbyladderdiagrams,whoseemitted

gluonshavestronglyorderedtransverseand

longitudi-nal momenta, summing the logs

s lnQ

2

ln(1=x). It

wasshown that the DLA is a ommon limit between

thelineardynamis[8℄.

Theinreasingofthepartondensitiesrequiresa

for-mulationof the QCD at high partoni density, where

unitarity orretions (UC), notonsidered in the

pre-viousdynamisalreadymentioned, areproperlytaken

into aount. In this sense,the small x region, where

thegluondistributionsetsthebehaviorofthemain

ob-servables, providesthe interfae between perturbative

andnonperturbativeQCD,orinotherwords,between

hard and soft physis. Clearly, both experimentalists

and theoretiians are hallenged to desentangle,

mea-sureandformulatethedynamialolletiveeetsthat

aresubjaenttotheobservedresultofinreasingF

2 and

therosssetion

tot

atDIS,asxgetssmaller[4℄. Both

evolutionequations, DGLAP (evolutionin lnQ 2

) and

BFKL (evolutionin ln(1=x)) as representativesof

lin-eardynamis,needontrolinordertorestoreunitarity,

sinetheFroissartlimitrequires

tot

Cteln 2

s[9℄.

Aomprehensivetreatmentshouldenvolveboth

lin-ear and non linear regimes. The main attempts to

develop a formalism for hdQCD are the approahes

of M.Lerran andollaborators (MVJKLW)[10℄, by

Kovhegov (K) [11℄ and by Ayala, Gay Duati and

Levin(AGL)[12,13℄. Derivedindependently,thethree

methods obtainnonlinear evolutionequations forthe

gluondistribution,atthesmallxregion,desribingthe

onsetofhdQCD,althoughonsideringdierentdegrees

offreedom.

InwhatfollowsIwillpresentanintrodutoryreview

ofthesubjetofhdQCD,themainaspetsofthe

formu-lationsto thesubjet,theonnetionsamong themin

theasymptotiregion(x!0), presentthestateofart

of the phenomenology of small x physis and address

(2)

someopenquestions.

II The Evolution Equations

ItwillbebrieypresentedtheDGLAPandBFKL

dy-namisand theirpreditionsforthesmall xregime at

DIS. TheDIS is theproess of interation ofalepton

andanuleonexhanginganeletroweakboson

produ-ingmanypartilesatthenalstate,whihisahadroni

stateX. Theproessis

l(k)N(p)!l 0

(k 0

)X ; (1)

wherek,k 0

,pandp 0

arethefourmomentaoftheinitial

and nal lepton, inident nuleon and nal hadroni

system, respetively. Themain variables forthis

pro-ess are Q 2

= q

2

= (k k 0

) 2

, whih is the square

ofthe transferedmomentum, s=(k+p) 2

, thesquare

of the enter of mass energy, W 2

= (q+p) 2

= (p 0

) 2

,

the square of theenter of massenergy of the virtual

boson-nuleon system. The hard sale is given by q 2

(< 0), orresponding to the proess resolution, and

x = Q 2

=2p:q, meaning the virtual boson resolvesthe

hadronistruture,orthepartons,sinex1= p

Q 2

. Arealsouseful thevariables y =q:p=k:p, measuring

theproessinelastiityand=q:p=m

N

,theenergyof

thevirtualbosononetakeninthetargetrestframe.

Intermsofthepartoniontentofthenuleonthe

struturefuntion,whihreetsitsoveralldistribution,

isgivenby

F

2 (x;Q

2

)= X

f e

2

f [q

f

(x;Q 2

)℄; (2)

wherethesumisoveravoursweightedbythe

respe-tivesquaredharges(e 2

f

). Itisthisfuntionthatis

ob-jetof main experimental studies,speially atHERA,

at the small longitudinal nuleon fration of

momen-tum,orsmallx (seeFig. 1)[14℄.

0

0.5

1

1.5

2

2.5

3

3.5

4

10

-3

10

-2

10

-1

1

x

F

2

(x,Q

2

)

0

0.5

1

1.5

2

2.5

3

3.5

4

10

-3

10

-2

10

-1

1

x

F

2

(x,Q

2

)

Figure1

The quark distribution funtion an be shown to

evolveas

q f

(x;Q 2

)

lnQ 2

=

s

2 Z

dx

1

x P

qq (

x

x )q

f

(x;Q 2

); (3)

where P

qq = C

F 1+z

2

1 z j

+

(with self-energy orretions

overthekpropagator)is oneofthesplittingfuntions

P

ij (P

gq =C

F 1+(1 z)

2

z

, et),desribingthetransition

between the quarkstate i to the quark state j, from

fration of momentum x

1

to x. The aboveevolution

refersto thenonsinglet quarksdistributionwheresea

quarksand gluondistributionareunoupled

q

NS (x;Q

2

)q

i (x;Q

2

) q

j (x;q

2

): (4)

Thesinglet quarkdistributionisgivenby

q

S (x;q

2

) X

f

q f

(x;Q 2

)+q f

(x;Q 2

)

; (5)

where the gluon distribution is oupled to the quark

one.

Now theevolutionequations, in thelinear regime,

readforthequarks

q

S (x;Q

2

)

lnQ 2

=

s (Q

2

)

2 Z

1

x

P

qq (

x

x

1 )q

s (x

1 ;Q

2

)

+ P

qg (

x

x

1 )g(x;Q

2

)

; (6)

andforthegluondistribution

g(x;Q 2

)

lnQ 2

=

s (Q

2

)

2 Z

1

x

P

gq (

x

x

1 )q

s (x

1 ;Q

2

)

+ P

gg (

x

x

1 )g(x;Q

2

) : (7)

TheEqs. (6)and(7)wereindependentlyderivedby

Dokshitzer, Gribov and Lipatov, and by Altarelliand

Parisi, known as DGLAP equations in leading order.

The perturbative QCD evolution, in the linear setor

isgovernedbyDGLAPequations,moreoverasuitable

non perturbativeiniial ondition, extrated from the

experimentforagivenbosonvirtuality.

It an be shown by suessive derivations that

q

NS

(x;") P

n (

s ")

n

, " = lnQ 2

, whih orresponds

to theemissionofn gluons,showingthat theDGLAP

equations resum the leading lnQ 2

. This an be

un-derstoodasladderdiagrams withastrongordering in

transverse momenta k

?

, i.e., Q 2

0 << k

2

1

<< ::: <<

k 2

n <<Q

2

. ThesaleQ 2

0

istheut,ortransitionvalue

betweenperturbativeandnonperturbativephysis. It

wasshownby Gribov [15℄ thatthis resultis gauge

in-dependentoneoneonsiderstheleadinglogarithm

(3)

At small-x the gluons dominate, sine P (0)

gg (z)

2N

z

,andtheparton distributionshavethegeneral

be-havior xp

i (x;Q

2

) x

, > 0. More likely for

ini-tial ondition xp

i (x;Q

2

0

) Const and xp

i (x;Q

2

)

exp p

ln(lnQ 2

)ln1=x, known as double leading

loga-rithm approximation (DLA). From that is lear that

DGLAPpreditstheinreaseofthegluondistribution

funtion,andofthestruturefuntion F

2

withthe

de-reasingofx,whoserelationinthiskinematialregime

isgivenby

F

2 (x;Q

2

)

lnQ 2

=

s (Q

2

)

2 X

f e

2

f

xg(x;Q 2

) (8)

beingequalto 2

s

9

xg(x;Q 2

)forn

f =3.

The DLA implies strong ordering in x and k

T , i.

e., x

1 >> x

2

>> :::: >> x

i 1 >> x

i

>> x and

k

T

1 << k

T

2

<< :::k

T

i 1 << k

T

i

<< Q 2

, the resum

of logs of

s

ln (1=x)lnQ 2

, havingasregionof validity

s

<<1,

s

ln(1=x)<<1and

s

ln(1=x)lnQ 2

1.

The resum of all leading logarithms of Bjorken x,

or the energy, is harateristi of the

Balitsky-Fadin-Kuraev-Lipatov(BFKL)equation. Forverylowx

val-ues the lns beomes largeand

s

ln1=x 1and the

DLA is not valid. The BFKL evolution equation is

proposed for an unintegrated gluon distribution

fun-tioninthetransversemomentumvariable. Itssolution

growsas apower of the enter of mass energy s with

the onsequent violationof the unitaritybound [9℄ at

veryhighenergies. Theurefor thisproblem was not

reahed in the next to leading order alulation [16℄,

andisstillunderresearhforinstane,throughthe

re-summingof allBFKL Pomeronexhanges[17℄,forthe

rosssetionaswellasforthestruturefuntion.

Theamplitudeforthesatteringquark-quark with

one gluon exhange in the t hannel at lowest order

is given by A

0

(s;t) s=t, and for the next order

in

s

the leading terms are given by lns, resulting

A

1

(s;t) A

0

(s;t)lns. One one goes to higher

or-dersthenumberofontributingdiagramsinreasesand

the alulation gains enormously in omplexity [18℄,

and the usual proedure is to introdue an eetive

vertex (Lipatov vertex). It results that the general

termisA

n

(s;t)A

0 (s;t)

n

(t)ln n

(s)=n,where(t)isa

suitable funtion to takeare ofinfrared divergenies,

doile under regularization, for instane, dimensional

regularization.

Clearlythe BFKL evolutionis summing theterms

n

s ln

n

(s), wherelowerorder logarithmsare negleted.

Theresultfortheamplitudeis

A(s;t)=A

0 (s;t)

1

X

n=0

n

(t)ln n

(s)

n!

s (t)

; (9)

with (t)=1+(t). Inthisase,thereisstill the(t)

infrared divergeniestobeured.

Whenjust thesingletontribution inthet-hannel

only Pomeron exhange diagrams are taken into

a-ount,theamplitudeisgivenby

ImA(s;t)

s

= G

2 2

Z

d 2

k

1 d

2

k

2

A (k

1 ;q)

F(y;k

1 ;k

2 ;q)

k 2

2 (k q)

2

B (k

2

;q); (10)

whereG istheolorfatorfortheproessand qisthe

transfered momentum in the t-hannel; the funtions

i

arethe impatfatorssetting theoupling ofF to

theexternalpartilesandnally thefuntion F isthe

perturbativegluonladder. Atleadingorder itonsists

intotheexhangeoftwogluonsbutthesumofallterms

impliesanintegralequationforF,thatisinfrarednite

forareggeizedgluonladder. Thisbehaviorofthe

ker-nelof theBFKL equationis onnetedwith theQCD

Pomeron anditistheresum oftheleadinglogarithms

lns.

The solution of the BFKL equation predits the

steepgrowthofthegluondistribution withdereasing

xaswellasthediusionofthetransversemomenta. As

wellasDGLAPequations,theBFKLequationpredits

thegrowingof theross setionin thesmall-xregime

sinethedynamisofthisobservableisrelatedwiththe

gluondistribution funtion.

From this verybrief disussion on the main issues

ofthelinearformalismsforthedynamisoftheparton

distributions,itgetsleartheneedofformalimproving

inordertoinlude theunitarityorretionspreserving

theFroissartlimit.

This important aspet of high energy physis was

pointed out many years ago by Gribov, Levin and

Ryskin (GLR) in Ref. [19℄. I will present in the

fol-lowingthemainattemptsdevelopedinthereentyears

towardsanon linear dynamis forhigh density QCD,

aswellasthehigh energyphenomenologyprovided.

III The Question

The main question that is addressed one treating

hdQCDishowtoanalytiallyseparatesmallandlarge

distane ontributions to high energy amplitudes in a

properlygaugeinvariantformalism. This orresponds

toestablishthehard andsoft salesfortheproess of

interestanddevelopthephysialmeaningfulmethodto

introduetheunitaryorretions(UC) intotheparton

dynamis.

One thetheoretialneedfor UCis establishedwe

shouldlook fortheirsignaturesanalysing dierent

ob-servables. Besidesomparingthepreditionsofthe

dis-tintformalismsitisrequiredaommonlimitbetween

them, probably to be set by a saturation sale, Q 2

S .

(4)

ap-Although someprogress hasbeen made towardstheir

onnetionthereisnoommonanalytisolutionforthe

gluondistributiong(x;Q 2

)forallkinematialrange.

ThephysisofhdQCDshakesthepartonmodeland

theherishedoneptofinoherenethatisbehindthe

standardalulations. Itseemsthatinordertoontrol

theinreasingofthegluonfuntion somegluon

reom-binationmehanismhastotakeplaeastheenergygets

higherandhigher.

This isagoodpointtoremindthat theanalysisof

thestruture funtionshasalreadygivenussome

sur-prises, and the previousimportant one was the EMC

eet[20℄,thathasasamainresultF A

2 =AF

n

2

6=1. This

diereneis not preditedifonerequires omplete

in-oherene of the partons, and reveals the presene of

nulear eets in the struture funtions where they

werenotexpeted. Alargeliteratureisdevotedtothis

phenomena, but it isinterestingto pointoutthat the

shadowing behavior notied in J= prodution ould

benielydesribed[21℄,aswellastheomparisonwith

Drell-Yan proesses [22℄, for the rst data at small-x,

onsidering the reombination approah developed by

Muellerand Qiu [23℄whih is basedonthe GLR

pro-posals.

Twomain aspets are in order, the ontrol of the

inreasingofthegluondistributionfuntionasan

uni-tarityimperativeandtheappearaneofnuleareets

in high energy proesses. Ifthis aspet is relevantfor

xedtargetquarkoniaprodution,itisstrongly

impor-tantforphysisofHERA-A,RHICandLHC with

nu-lei.

IV The High Density QCD

Ap-proahes

TheleadinglogarithmapproximationDLA(relatedto

DGLAP) and LL(1/x) (related to BFKL) result both

into linear evolutionequations for the gluon

distribu-tionfuntion. Theeet ofsumminglargelogsinhigh

energyregimeimpliestheinreaseofthegluon

distribu-tionfuntion g(x;Q 2

)aswellastherosssetionone

xdereases. However,thisresultviolatestheunitarity

of the sattering matrix, a main theorem of

relativis-ti Quantum Field Theory, the Froissart theorem [9℄,

whihstatestherosssetion annotgrowfasterthan

ln 2

s. TranslatedtotheDIS,thisimpliesinreasing

re-stritions to thestruture funtion and/or totalross

setion,saylowerthanln 2

(1=x)andprovidesa

limita-tioninthexrangetotheappliationoflinearevolutions

inorder togetsuitableresults.

Intuitively we an assoiate xg(x;Q 2

) to the

num-berof gluonsinto the nuleon, n

g

, per rapidityunity,

y = ln(1=x), with transverse size of order 1=Q. In

the hadron-nuleon interation it is the virtual gluon

that probesthenuleonstruture,in analogywiththe

rosssetionis

G

N (x;Q

2

)=

0

xg(x;Q 2

); (11)

where

0 =

G

g!X = Cte

s(Q 2

)

Q 2

, is the total ross

setionofthevirtualgluon,withvirtualityQ 2

,and

nu-leon gluoninteration. Assuming

0

=R

2

HAD ,then

0 xg(x;Q

2

) orresponds to the area oupied by the

gluonsinanuleon. Asx!0,thistransverseareamay

beomparable,orevenbigger,thanR 2

HAD

,following

DGLAPorBFKLpreditionsforsmallx orsmall Q 2

.

Approahing this regime the gluons may begin to

su-perposespatially inthetransversediretionand to

in-terat, behaving not anymore asfree partons. These

interations should slower, or even stop, the intense

growing of the ross setion, xing the limit R 2

HAD

in thesmallx regime.

Introduingthefuntion,withprobabilisti

inter-pretation

=

0

xg(x;Q 2

)

R 2

; (12)

itispossibletoestimateinwhihkinematialregionone

an expet modiationsin the usual evolution

equa-tions. So to say, for << 1 the system stays at x

andQ 2

wheretheusualevolutionequations(linear)are

appliable, governed by individual partoni asades,

withoutinterationsamongtheasades.

As

s

,partons fromdistintasades beginto

interatduetospatialsuperposition.Thisspei

kine-matialregimeortheonsetofthereombination

meh-anism was rst studied by Gribov, Levin and Ryskin

[19℄ almost twentyyears ago, proposing the

introdu-tionofnonlineartermsintotheevolutionequation.

Theregion of ! 1 was addressedmore reently

[12, 13℄ (see Fig. 2) and experiened onsiderable

de-velopment on the theoretial side [10, 11℄, also

moti-vatedbyHERAresultsandthegreatinterestonRHIC

and LHC future data. This is the kinematial regime

that requirestheQCDdynamisforhighpartons

den-sity. Although theoupling onstant

s

is still small,

allowing in priniplethe useof perturbativemethods,

thesystemissodensethatmanifestationofnon-linear

eets are expeted, and theyare required to be

on-sideredinaompleteformalism.

The region of ! 1 orresponds to partons in a

(5)

-1.0

0.0

1.0

2.0

3.0

4.0

0.0

5.0

10.0

15.0

20.0

Contour for

κ

= cte for Nucleon

R

2

= 5 GeV

-2

κ = 0.6

= 0.8

= 1.0

= 1.2

= 1.4

HERA 96

ln(1/x)

ln(Q

2

/GeV

2

)

HERA

Figure2

IVI The GLR Formulation

Gribov, Levin and Ryskin [19℄ introdued the

meha-nismofpartonreombinationinperturbativeQCDfor

high density systems,expressing this asunitarity

or-retions inluded in a new evolution equation known

as GLR equation. In terms of diagrams it onsiders

thedominantnon-ladderontributions,ormulti-ladder

graphs,alsodenotedfan diagrams.

The standard QCD evolution is represented by a

asadeof partonideaysinthenuleon. Thephoton

interats with aparton with fration of momentum x

andvirtualityQ 2

,whihisthelastoneofahainwhere

the partonsgetslowerand withbiggervirtuality. The

saleQ

0

setstheinitialvirtualityandatthesametime,

thelimitforperturbativeQCDappliability,andQ 2

is

the higher virtuality of the hain. In the transverse

planethepartonswithlowfrationofmomentumstay

inthelowerpartoftheladderandhavelargetransverse

size;thosewithbiggervirtualityareontheupperpart

oftheladderandtransversallysmaller.

Following DGLAP, the number of partons of low

frationofmomentuminreasesveryrapidly,whih

pi-torially orresponds to bigger density of individuals

in the sameallowedarea, in ontrastwith a more

di-lutedsystematintermediatevaluesofx,farawayfrom

thepossibilityofsuperposition.Thetransitionbetween

theseregimesshouldbeharaterizedbyaritialvalue

x =x

CRIT

. Thesame an be argued throughBFKL

formalism,with thedierenethat in thisasethe

in-reasingof thepartoni distributions,takesplaeat a

xed transverse sale, although theevolution presents

theutuationsinthetransverseplaneduetothe

har-ateristidiusion inBFKL.

Itisimportanttoemphasizethatinbothlinear

dy-namis only thedeayproessesare onsidered in the

partonievolution,howeverweexpetthatthe

anihila-tionmehanismshouldontributeinthelowxregime,

distribution funtion. In the linearapproah we

on-sider one inident and two emergent partons to

on-strut the splitting funtions for the deay proesses.

Nowitistheasetoonsidertwoinidentpartonsand

one emergent one, and to express the reombination

mehanism it is needed a formulationin terms of the

probabilitytoreombinetwoinidentpartons.

As arst approximationoneonsiders the

anihila-tion probability as proportional to the square of the

probability to nd oneinident parton, introduing a

non-linearbehavior.

Taking = xg(x;Q

2

)

R 2

as the gluon density in the

transverseplane,onehasthegeneralbehavior:for

split-ting1!2,theprobabilityisproportionalto

s ,for

anihilation 2 ! 1, the probability is proportional to

2

s

2

=Q 2

; where 1=Q 2

stands for the size of the

pro-dued parton. For x ! 0, inreases and the

anihi-lation proess beomes relevant. Consideringaell of

volumelnQ 2

ln(1=x)in thephasespaeallowsone

towritethemodiationofthepartoni densityas

2

lnQ 2

ln1=x =

s N

2

s

Q 2

2

; (13)

where the oupling in the proess is given by .

Ex-pressing in terms of the gluon distribution the above

equationis

2

xg(x;Q 2

)

lnQ 2

ln1=x =

s N

xg

2

s

Q 2

R 2

[xg℄ 2

: (14)

This equation is the GLR equation [19℄. The

al-ready mentioned work of Mueller and Qiu [23℄ gives

=81=16forN

=3.

Thenon-linearorretions orrespondto alass of

QCDFeynmandiagrams,alled fan diagrams,formed

byagluonladderwithsubsequentsubdivisionsingluon

ladders, where the three ladders vertex is assoiated

withthedeayandonsistsofasumofseveralnon

pla-nardiagrams. Theoverall resultarriesaminus sign,

whih is important in order to ontrol the growing of

theparton distribution onethe fan diagramsbeome

relevant,i.e.,atlowx. Thelowestpartofthediagrams

ouplestothenuleonandtheEq. (14)resumsalllass

ofthediagramsrepresentedinFig. 3.

As is lear from Eq. (14), the non-linearterm

re-duesthegrowingofxg(x;Q 2

)atlowx,inomparison

with the linearequations. It is also predited for the

asymptoti region x ! 0 the saturation of the gluon

distribution,witharitialline betweenthe

perturba-tiveregion and saturationregion, setting its region of

validity (meaning independene of the gluon funtion

with the energy). The subjet of saturation is very

appealing andthere areseveralattempts in the

(6)

γ

N

N

G(Q

2

,x)

γ

γ

γ

d)

Figure3

In the asymptoti limit one obtains

xg(x;Q 2

)

GLR

SAT =

16

27

s Q

2

R 2

. Sine the GLR only

inludes therst non-linearterm,although it predits

saturationin theasymptotiregimeitsregionof

valid-itydoesnot extendto veryhigh density wherehigher

ordertermsshouldontributesigniantly.

IVII The AGL Formulation

This approah developed by Ayala, Gay Duati and

Levin (AGL) [12, 13℄, intents to extend the

perturba-tivetreatmentofQCDuptotheonsetofhighdensity

partons regime, through the alulation of the gluon

distributionwhihisthesolutionofanon-linear

equa-tionthatresumsthemultipleexhangeofgluonladders,

indouble leadinglogarithmapproximation(DLA).

Itis basedonthe developmentofthe Glauber

for-malismfor perturbativeQCD [25℄, onsideringthe

in-terationofthefastestpartons oftheladderswiththe

target, nuleonor nuleus,sineoneofthemain goals

isto obtainthenuleargluondistributionxg A

(x;Q 2

).

We onsidered a virtual probe G

that interats with

the target in the rest frame, through multiple

resat-terings with the nuleons. In this referene framethe

virtualprobe anbe interpreted following the

deom-positionoftheFokstates,anditsinterationwiththe

target oours by the deay of the omponent gg, as

representedin Fig. (4).

Forsmall-xthispairhasalifetimemuhbiggerthan

thenuleus (nuleon) radius and thepairis separated

bythexedtransverseseparationr

t

duringthe

intera-tion,whih isrepresentedbythe exhange ofaladder

ofgluonsstronglyorderedintransversemomentum.

Therosssetionforthisproessisgivenby

G

A

= Z

1

0 dz

Z

d 2

r

t

j

G

t (Q

2

;r

t ;x;z)j

2

gg+A

;(15)

where G

is a olorless virtual probe with virtuality

Q 2

;z is the probe fration of energy arried by the

gluonand G

t

isthewavefuntionofthetransversely

polarizedgluonin theprobe, gg+A

(z;r 2

)is theross

setion of the pair with the target, whih was proven

forperturbativeQCDbyMuellerinRef. [25,26℄

The lower limit estimation of UC is obtained

throughtheinoherentresatteringsof thegluonpair,

withtheonstraintthatonlythefastestpartonsofthe

laddersinteratwiththetarget. Introduingthe

trans-verseimpatparameterb

t

andaprolefuntionforthe

nuleusS(b

t

)weget

G

A

= Z

1

0 dz

Z

1

0 d

2

r

t

Z

d 2

b

t

j

G

t (Q

2

;r

t ;z)j

2

2[1 e 1

2

g g

N (x

0

;4=r 2

t )S(bt)

℄; (16)

where x 0

= x=(zr

t Q

2

), S(b

t

) may be taken as

A

R 2

A e

b

t =R

2

A

foragaussianprole, gg

N =

CA

CF

qq

N ,where

qq

N =

CF

CA (

3

4

s (4=r

2

t ))

2

r 2

t

xg(x;4=r 2

t

), and 4=r 2

t is a

ut for the nonperturbative region. For the virtual

probe with virtuality Q 2

the relation G

A

(x;Q 2

) =

( 4

2

s

Q 2

)xg

A (x;Q

2

)isvalid.

In this approah the gluon pair emission is

de-sribed in DLA of perturbative QCD and from the

Feynmandiagramsoforder n

s

,itshould beextrated

only the terms that ontribute with a fator of order

(

s

ln1=xlnQ 2

=Q 2

0 )

n

. Theinterationofthegluonpair

withthetargetoperatesthroughtheexhangeofa

lad-der whih satises the DGLAP evolution equation in

theDLAlimit.

It is aworking hypothesis that in high energy the

suessiveresatteringsanbetakenasindependent

al-lowingtheemployofGlauberformalism,insuhaway

using the eikonal proedure for a relativisti partile

propagatingin thetarget.

Our master equation for the interation of the gg

pair with the target is known asthe Glauber-Mueller

formulaandis

xg

A (x;Q

2

)= 4

2

Z

1

x dx

0

x 0

Z

1

4=Q 2

d 2

r

t

r 4

t Z

d 2

b

t

2[1 gg

N (x

0

;4=r 2

t )S(b

t

)℄: (17)

Thepitorial representationof thespae-time

evo-lutionofthis formulaisgivenin Fig. (4).

(7)

Oneweperformtheimpatparameterintegration

usingagaussianprolefuntionweobtain

xg A (x;Q 2 )= 2R 2 A 2 Z 1 x dx 0 x 0 Z 1=Q 2 0 1=Q 2 d 2 r t r 4 t

C+ln(

G (x 0 ;r 2 t ))+E

1 ( G (x 0 ;r 2 t )) ; (18)

where C is the Euler onstant, E

1

is the exponential

funtion andwherethe

G

funtionwasintroduedas

G (x;r 2 t )= 3 s 2R 2 A r 2 t xg(x;1=r 2 t

): (19)

The expansion of Eq. (18) in terms of

G gives

as the Born term the DGLAP equation in the small

x region, the higherorder terms orresponding to the

unitarityorretionsnaturallyimplementedinthis

for-malism.

Theestimationoftheshadowingeetduetogluon

reombinationanbeimmediatelyobtainedstudingthe

ratio R 1 = xg A (x;Q 2 )=Axg GRV N (x;Q 2

) presented in

Fig. (5), wherewealulate forCaandAu,and

anal-ysed thebehaviorof thisfuntion in termsof ln(1=x),

A 1=3

andlnQ 2

. WeusedtheGRVparametrization[27℄

and adapted the alulation in order to have alarger

domain ofvalidityin xusing

xg(x;Q 2

)=xg

A

[Eq:(18)℄+Axg GRV (x;Q 2 ) A s N Z 1 x Z Q 2 Q 2 0 dx 1 x 1 dQ 02 Q 02 x 0 g(x 0 ;Q 2

); (20)

where Axg GRV

(x;Q 2

0

) is the initial ondition. The

same proedure ould be applied for another global

parametrizationbasedonDGLAP.

AsexpetedtheUCinreasewithA,andgetsmaller

asQ 2

inreasesanditisevidenttheimportaneofthe

eet asx goesto small values. This allowsus to say

that theUCshould beinludedinthealulations

re-lated withthenuleargluondistributionfuntion,and

the obtained funtion xg

A (x;Q

2

) may be used to set

the initial onditions for future experiments. For

in-stanein HERA-A,in proessese

A [28℄thefuntion

xg

A

ould beobtained indiretly and employed as an

initialonditionforthehadronihighenergyproesses

at RHICandLHC.

Thequarksand gluonsdistributionwerealso

anal-ysedforthenuleoninthisformulation[13℄,aswellas

thestruturefuntion F

2

[29℄. Themotivation forthis

0.0

2.0

4.0

6.0

8.0

10.0

0.4

0.6

0.8

1.0

ln(Q

2

)

e)

f)

Ca

0.0

2.0

4.0

6.0

0.4

0.6

0.8

1.0

A

1/3

R

1

R

1

0.0

5.0

10.0

15.0

20.0

0.2

0.4

0.6

0.8

1.0

Q

2

=1.0 Gev

2

Ca

=10. Gev

2

=1.0 Gev

2

Au

=10. Gev

2

R

1

ln(1/x)

a)

0.0

2.0

4.0

6.0

8.0

10.0

0.4

0.6

0.8

1.0

x

B

=10

-5

=10

-4

=10

-3

=10

-2

Au

ln(Q

2

)

0.0

2.0

4.0

6.0

0.4

0.6

0.8

1.0

x

B

=10

-5

=10

-4

=10

-3

=10

-2

Q

2

=1 Gev

2

Q

2

=10 Gev

2

A

1/3

R

1

R

1

R

1

0.0

5.0

10.0

15.0

20.0

0.2

0.4

0.6

0.8

1.0

Q

2

=0.5 Gev

2

Au

=1.0 Gev

2

=10. Gev

2

=100. Gev

2

ln(1/x)

b)

c)

d)

Figure5

ThefreeinterpretationoftheFroissarttheoremfor

hadroni proesses requires a limit for the inreasing

of the ross setion

N and F

2

with the energy so

unitarity is not violated. Conentrating the

disus-sion on the value, = xg(x;Q 2 ) gg =(Q 2 R 2 ) = 3 s xg(x;Q 2 )=2Q 2 R 2

, whihistheprobabilityof

glu-onsinterations inside the partoni asade, and R is

theradiusofthenuleonareaoupiedbythegluons,

we were able to obtain R 2

= 5 GeV 2

, and that

reahes1 at HERA,meaning theeets of shadowing

should be onsidered in the analysis [12, 13, 30℄. In

thenuleonase,followingthesamestepsasbeforewe

obtain xg(x;Q 2 )= 4 2 Z 1 x dx 0 x 0 Z 1 4=Q 2 d 2 r t r 4 t Z 1 0 d 2 b t

2[1 e 1 2 g g N (x 0 ;4=r 2 t )S(b t )

℄; (21)

and requiring the reovering of DGLAP at DLA we

have gg N (x;4=r 2 t )= 3 2 s 4 r 2 t xg(x;4=r 2 t

): (22)

Forthe quarks,onsideringthe satteringof a

vir-tual photon that deays into a quark-antiquark pair,

whihinteratswiththenuleonthroughtheexhange

ofaladderweget

( )= Z 1 0 dz Z d 2 r t j (z;r

t )j 2 qq+N tot ; (23)

where is the wavefuntion of the qqin the virtual

photon[26℄. Weobtain

tot = Z d 2 b t [1 e 1 2 qq(x;rt;bt)

(8)

Here

qq

is the opaity funtion that in the

Glauber (or eikonal) approah is equivalent to =

4 2

s (Q

2

)

3Q 2

xg(x;Q 2

)S(b

t

). In doing so we are able to

reprodueDGLAP evolutionfor<1,and guarantee

thevalidityoftheformulationalsoforthekinematial

regionwhere>1.

Taking ! 1 and fatorizingthe b

t

dependene

weobtaintheunitaritylimitforthestruturefuntion,

having for the lnQ 2

derivative of F

2 , F

2 =lnQ

2

<

Q 2

R 2

=3 2

. UsingGRV, theunitaritylimitfor HERA

isreahedforQ 2

=Q 2

0

=1 2GeV 2

(y=ln1=x9).

Similarly,forgluonsitisQ 2

=1 2GeV 2

(y=ln1=x

7)forHERA[30℄.

Withtheaimtoobtainanon-linearevolution

equa-tionontainingtheunitarityorretionsthroughthe

in-lusionofalltheinterationsbesidesthefastestparton

from the ladder, wedierentiate our master equation

forthegluonin y=ln1=xand"=lnQ 2

,obtaining

2

xg(y;")

y" =

2Q 2

R 2

[C+ln(

G )+E

1 (

G

)℄; (25)

where DGLAP

G

(x;Q 2

) = Ns

2Q 2

R 2

xg DGLAP

(x;Q 2

) for

alulations.

Intermsof

G

themainevolutionequationis

2

(y;")

y" +

(y;")

y =

N

s

[C+ln(

G )+E

1 (

G )℄:(26)

It should be mentioned that large distane eets are

absorvedin theinitialonditionfortheevolution,and

situating in a onveninet region of Q 2

only short

dis-taneeetsarepresent,meaningaperturbative

alu-lationisreliable.

Equations (25) and (26) were derived in Ref. [12,

13℄, and refered forsimpliity asAGL equation. The

mainpropertiesofthisformulationare:

all ontributions from the diagrams of order

(

s y")

2

areresummed;

in thelimit!0theDGLAPevolutioninDLA

isfullyreovered;

for < 1, and not large, the GLR equation is

reovered;

for

s

y" 1 the equation is equivalent to the

Glauberformalism.

TheUCaredesribedforthe dierentkinematial

regionsof fromstritly perturbativeQCDuptothe

onset of hdQCD. Non-perturbative eets are not

ex-pliitly desribed and this is the objet of a distint

formalismMV JLKM [10℄thatwewillbriey

om-ment in a next subsetion. In Fig. (6) the

ompari-sonbetweenthesolutionsoftheequationsAGL,GLR,

DGLAP and Glauber-Mueller (MOD MF) formula is

presented,wheretheontrolofthegrowingofthegluon

Itwasalsoobtainedtheasymptotisolution>1

oftheAGLequationforxed

s

[12,13℄ aswellasfor

running

s

[31℄. Forhighpartonidensityandy>>y

0

weobtain

asymp

G

(y)=

s N

ylny

s N

y: (27)

0.0

10.0

20.0

30.0

0.0

10.0

20.0

30.0

κ

values

DGLAP

MOD MF

AGL

GLR

Q

2

= 10. GeV

2

κ

y=ln(1/x)

Figure6

Thissolutionisagoodapproximationforverysmall

values of x (O(10 8

)), related with THERA physis

[28℄, regionofaverydensepartonsystem. Intermsof

thegluonfuntiontheasymptotibehavioris

xg(x;Q 2

)= 2N

Q

2

R 2

3 2

ln(1=x); (28)

presentingabehaviorsofterthanpreditedbyDGLAP,

meaningapartial saturation.

Fortherunning

s

theresultis[31℄

xg(x;Q 2

)= "

1+" 2N

Q

2

R 2

3 2

ln(1=x): (29)

where "=lnQ 2

= 2

QCD

. The partial saturationis not

modied, and the main dierene from the previous

resultoours forsmall valuesof". Thisonrms the

expetationthattheUCarealreadyrelevantbeforethe

orretionstoleadingorder[30,32℄.

IVIII The Kovhegov Formulation

The unitarization problem in QCD was addressed as

an extension of the dipoles formalism for the BFKL

equationbyKovhegov[11℄. Thisworkproposesanon

lineargeneralizationofBFKLequation,alsoaddressed

previously in Ref. [33℄ by the use of OPE to QCD

obtainingthe evolutionof Wilson line operators. The

sattering ofadipole(onium - qq)with thenuleonis

desribed byaasade evolutionorrespondingto the

suessivesubdivisionofdipolesfromthefatherdipole.

(9)

resummedinordertoobtaintherosssetionofthe

in-teration ofthedipolewith thenuleus. Asaresultit

isderivedtheevolutionequationhavingtheunitarized

BFKLPomeronassolution,intheLL(1=x)

approxima-tion.

The sattering of the onium qq(dipole) with the

nuleus in the rest frame, takes plae through a

as-ade of softgluons, whih one taken in the N

! 1

limitis simpliedbythe suppressionofnon-planar

di-agrams. The gluonsare replaed byqqpairs and the

dipoleMueller'stehniquefortheperturbativeasade

anbeemployed[34℄.

TheKovhegovformulation,as the AGL,is a

per-turbativeQCD alulationand theonsidered dipoles

from the asade interat independently with the

nu-leus. Theonium-oniumfrontalsatteringhastheross

setion = 2ImA,where theamplitude

A= i Z

d 2

x Z

1

0 dz

Z

d 2

x

1 Z

1

0 dz

1

(~x ;z)F(x~

1 ;z

1 );

where(~x ;z)isthesquareoftheoniumwavefuntion,

~

xisthetransverseseparationoftheqqpair,andzisthe

longitudinal fration of momentum of the quark. For

theexhangeof onlytwogluons,withoutgluonladder

evolutionthefuntionF is[26℄

F (0)

(~x ;x~

1 )=

2

s (N

2

1)

N 2

x

2

<

(1+ln ( x

>

x

<

)); (30)

wherex

> (x

<

)isthebiggest(smaller) betweenj~x jand

jx~

1

j. Thetwogluonsapproximationisenergy

indepen-dent, but for high energy the ontributions of order

(

s Y)

n

shouldbeinluded(Y =lns=M 2

is the

rapid-ityandM istheoniummass),sinetheygeneratethe

perturbativeasadeevolution. Thedipole

approxima-tion introdues an arbitrary number of soft gluons in

thesquareoftheoniawavefuntion,andkeepingF

asan exhange of two gluons avoidsto deal with the

reggeizationofthegluonsandtheeetivevertex. The

transverseoordinatesofthequarkandantiquarkofan

ultrarelativistioniumstate in +diretion arex~

0 =0

and~x,andsuessivelyintheevolutionthenext

emit-ted gluonshould be softer. We have p k and k, as

themomenta for thepair, and z

1 =

k +

1

p +

(in light-one

variables[35℄),havingaswavefuntion

(0)

(x

01 ;z

1 )=

Z

d 2

k

1

(2) 2

e i

~

k

1 ~ x

01 (0)

(k

1 ;z

1

); (31)

wherex~

01 =x~

1 ~ x

0

, and (0)

=j (0)

j 2

, keeping

fa-torizationin thisproedure. This allowstoobtainthe

dipoledensity,n,onsideringx

02 >;x

12

>,where

isanultravioletutalsoimpliedbyCintheexpression

below

n (x

01

;x;Y)=xÆ(x x

01 )exp

2

s N

Y ln( x

01

)

+

s N

2

Z

C x

2

01 d

2

x

2

x 2

02 x

2

12 Z

Y

0

dyexp

2

s N

(Y y)ln ( x

01

)

n(x

12

;x;y); (32)

forY =lns=M 2

,whihis representedinFig. (7).

}

x

x

x

+

x

0

}

x

=

x

0

1

0

x

1

1

x

Figure7

Thenextstepistoobtainanevolutionequationforthedipoledensityassumingthepropagationofthedipoles

inthetargetisrepresentedbythefuntion

1 (~x ;

~

b),wherebistheimpatparameter,andwhihshouldbeaddedto

thedensityn

2

,equallyonvolutedwith

2 (x~

1 ;

~

b

1 ;x~

2 ;

~

b

2

),et. Assumingnoorrelationamongthedipoles

n (:::)=

1 (x~

1 ;

~

b

1 ):::

1 (x~

n ;

~

b

n

),therosssetionfortheinterationoniumnuleusN(x~

01 ;

~

b

0

;Y)isthen givenby[11℄

N(x~

01 ;

~

b

0 ;Y)=

1

X

i Z

n

i (x

01 ;Y;

~

b

1 ;x~

1 ;:::;

~

b

i ;x~

i )

(x~

1 ;

~

b

1 )

d 2

x

1

2x 2

1 d

2

b

1

:::

(x~

i ;

~

b

i )

d 2

x

i

2x 2

d 2

b

i

(10)

Finally,omittingsomestepsofthealulation[11℄theevolutionequationforN(x~

01 ;

~

b

0 ;Y)is

N(x~

01 ;

~

b

0

;Y)= (x~

01 ;

~

b

0 )exp

4

s C

F

ln(

x

01

)Y

+

s C

F

2

Z

Y

0

dyexp

4

s C

F

ln(

x

01

)(Y y)

Z

d

2

x

2 x

2

01

x 2

02 x

2

12

2N(x~

02 ;

~

b

0 +

1

2 ~ x

12 ;y)

N(x~

02 ;

~

b

0 +

1

2 ~ x

12

;y)N(x~

12 ;

~

b

0 1

2 ~ x

20 ;y)

; (34)

d

where x

ij = x

i x

j

, the size of the dipole whose

quarkhastransverseoordinatex

i

, andtheantiquark

x

j , (x~

01 ;

~

b

0

)is thepropagatorof thepair qq through

thenuleus,desribingthemultiple resatteringofthe

dipolewiththenuleonswithinthenuleus. Wedenote

thisequationas theK equation.

Thephysialrepresentationisomparablewiththe

approah Glauber-Mueller sine the inident photon

generatesaqqthatsubsequentlyemitsagluonasade

furtherinterating withthenuleus. AtlargeN

limit

thegluonanberepresentedbyaqqpair,andwean

expet in this limit and DLA that the gluon asade

ouldbeinterpretedasadipoleasade. Although

be-guinningtheformulationswithdistintdegreesof

free-dombothKandAGLresumthemultipleresatterings

in their respetives degrees of freedom, whih allows

to onsidertheyshould oinidein asuitableommon

kinematiallimit,whih wewillshowlateron.

InDLA, wherethe photonsale of momentum Q 2

isbiggerthan 2

QCD

,theKequationsimpliesto

N(x~

01 ;

~

b

0 ;Y)

Y

=

s C

F

x

2

01 Z

1= 2

QCD

x 2

01 d

2

x

02

(x 2

02 )

2

h

2N(x~

02 ;

~

b

0

;Y) N(x~

02 ;

~

b

0

;Y)N(x~

02 ;

~

b

0 ;Y)

i

; (35)

whih is the evolution in transverse size of the

dipoles from x

01

up to 1=

QCD

. Now deriving in

ln(1=x 2

01

2

QCD

)results

2

N(x~

01 ;

~

b

0 ;Y)

Yln(1=x 2

01

2

QCD )

=

s C

F

h

2 N(x~

01 ;

~

b

0 ;Y)

i

N(x~

01 ;

~

b

0

;Y):(36)

settingthatthesuessiveemissionofdipolesgenerates

largertransversesizeforeahhighergeneration.

The linear term reprodues BFKL at low density,

andthequadratitermintroduesUCunitaryzingthe

BFKLPomeronandtheequationreproduesGLRone

weassumeN diretlyrelatedtothegluondistribution

funtion.

IVIV The MV-JKWL Formulation

IntheMV-JKWLformulation[10,36℄averydense

sys-tem is treated in the light-one and onsidering the

light-one gauge (A +

0), x q +

Gluon =Q

+

Nuleon . In

Ref. [10℄thegluonsdistributionforsmallxisproposed

foralargenuleuswherethedegreesoffreedomare

vir-tualquantafromalassialeldgeneratedbytheolor

hargeofthevalenepartons(statisoures). The

ap-proah is originally non-perturbative and the nuleus

is onsidered in the innite momentum frame,

trans-fering the sale of the problem to = 1=R 2

dN=dy,

where N is the density of gluons. For small x and a

large nuleus

s

() is small allowing some

perturba-tivealulationinthiseetivelagrangianformulation

forgluonsondensates.

The density of gluons in momentum spae is

ob-tained in terms of theorrelation of thegluons elds,

in thelightonegauge. Theintrinsiquantum

utu-ations are replaedby alassialaverage onthe olor

harge ensemble. Thegluons distributions at agiven

virtualityQ 2

andxisobtainedfromthedensityof

glu-onsin themomentaspaedN=dq +

q 2

~

q,whihisa

fun-tion of the gluon ondensate <A a

i

(x ;~x )A(x 0

; ~

x 0

) >,

being

xg(x;Q 2

) Z

Q 2

d 2

~ qx

dN

dxq 2

~ q

: (37)

Thegluons distributions, in this framework where

alargenumberof olorhargesgeneratesaQCD

ve-torpotential,isobtainedinlowestorderbysolvingthe

lassialYang-Mills equations,D

F

=j

.

Introduingaregulatorin thevalenepartons

ur-rent singularity by onsidering the olor density a

funtion of rapidity, itwasobtained[39℄an analytial

solutionforthelassialorrelations,withtheproperty

that for high transverse momentum the lassial

glu-ons distribution obeys the Weizsaker-Williams form,

and hasitsbehaviorsoftenedasln(k 2

=(y;k 2

(11)

= R 1 y 2 (y;Q 2

)isthesquaredolorhargeperunity

of areaforrapiditybiggerthany.

In the lassial MV the non-linear eets are

in-luded in the harge density solution of Y-M

equa-tions. The quantum orretions areto beonsidered,

andfromRef. [37℄theperturbativeresultforthegluons

distributionuptoseondorderin

s

isgivenby

1 R 2 dN dxd 2 k t = s 1 xk 2 t 1+ 2 s N ln ( k t s

)ln ( 1 x ) ;(38) where = 2 (N 2 1) 2 and 2

is the square ofthe olor

hargeaverage density(perunity of area). The

addi-tional eetofinludingthehardgluonwastreatedin

Ref. [38℄, resultingin thelowdensity limittheBFKL

equation, and for high virtualities the DGLAP

equa-tion. Forhigh densityaompletesolutionwasnotyet

obtained. In Ref. [40℄ JKLW analysed theirevolution

equationin DLAobtainingageneralizationofGLR.

As a summary of the formulations for hdQCD at

present, the Fig. (8) presents their dierent regions

of appliability asfas asin onernedin theln(1=x)

versusQ 2

plane.

Figure8

Themainquestionsatthis pointanbe:

whih isthemost suitableformto introduethe

UC?

anwerelatethedistintformulationsina

om-monlimitanalytially?

whatdowelookattheobservablesasasignature

fortheUC?

Thelasttwoquestions,I willbriey addressin the

rest of this presentation followingour personal

ontri-V Connetion Among the F

or-mulations

The AGL equation was originally obtained from the

Glauber-Mueller approah, but it an be also derived

from the dipole representation [41℄. We obtained the

ross setion for the virtual probe G

with the

nu-leus G A = R 1 0 dz R d 2 rt j G t j 2 gg+A

, that an be

expressed by meansof the dipoles qqone weremind

gg+A = (C A =C F ) qq+A

. Now in order to estimate

the UC the resatterings of the qq pair into the

nu-leus should be onsidered, having in mind that [30℄

qq N = C F CA (3 s (4=r 2 t )=4) 2 r 2 t xg N (x;4=r 2 t

), where xg

N

is the nuleon gluon distribution. The wave

fun-tion G

alulated in [26, 30℄ is suh that j G t j 2 = 1 z(1 z) [( 2 K 0 (t t ) K 1 (r t )=r t ) 2 + 1=r t (K 1 (r t )) 2 ℄, where 2 = Q 2

z(1 z), and the K

i

are the modied

Besselfuntions. Forsmallz andr

t

<<1weobtain

xg A (x;Q 2 )= 4 C A C F Z 1 x dx 0 x 0 Z 1 4=Q 2 d 2 r t r 4 t 2 h 1 e 1 2 qq N S(b t ) i : (39)

From this equationweanobtainthe AGL

equa-tion in the dipole representation by dierentiating in

y=ln1=xandlnQ 2 = 2 QCD having 2 xg(x;Q 2 )

y lnQ 2 = 2 QCD =C 0 Q 2 Z d 2 b t h 1 e 1 2 qq N S(b t ) i ;(40)

validinDLA,onsideringeahgluonoftheasadeas

aqq inthehigh N

limit,andwhere C 0 =2C A = 2 C F .

For a entral ollision and S

?

= R

2

, and S(0) =

A=R 2 2 xg(x;Q 2 )

ylnQ 2 = 2 QCD =DQ 2 1 e 2 s 2 N S ? Q 2 xg A ; (41) for N

= 3, C

F = N

=2 at high N

, and where

D=

NCFS?

3

.

The GLR for a ylindrial nuleus is immediately

obtained from Eq. (41) by its expansion up to

se-ond order in xg

A

. Again, for small UC only the rst

termontributeswhihreproduesDGLAPintheDLA

limit. ThoseresultsareinRef. [41℄

Now, theEq. (34)is theKequation that in DLA,

wherethesaleofmomentumofthephotonQ 2

ishigher

thanthesaleofmomentumofthenuleus 2

QCD ,

sim-pliesas

N(x~

01 ;

~

b

0 ;Y)

Y = s C F x 2 01 Z 1= 2 QCD x 2 01 dx 2 02 (x 2 02 ) 2 h

2N(x~

02 ;

~

b

0

;Y) N 2

(x~

02 ;

~

b

0 ;Y)

i

(12)

Thisequationonsiderstheevolutionofthedipoles

from x

01

up to 1=

QCD

in the transverse diretion.

NowderivingEq. (42)in ln(1=(x 2

01

2

QCD

))weget

2

N(x~

01 ;

~

b

0 ;Y)

Yln(1=x 2

01

2

QCD )

=

s C

F

[2 N℄N: (43)

We should relate now the funtion N(~x

01 ;

~

b

0 ;Y)

withthegluondistributionfuntion. Forthat we

on-sider the struture funtion F

2

for the nuleus as

ob-tained in [11℄, following [25℄, and analized in [29℄ for

b

t

=0,whihis

F A

2 (x;Q

2

)= Q

2

4 2

em R

2 Z

dz Z

d 2

r

t

j j

2

2 "

1 e

s C

F

2

N 2

S

? r

2

t

Axg(x;1=r 2

t )

#

: (44)

This estimates the UC for the nulear struture

funtion,for entral ollisions in theDLAlimitin the

Glauber-Muellerapproah.

Considering the unitarity orretions due to the

multiple resatteringof the qq pairs with the distint

nuleons into the nuleus, from the just obtained

ex-pressionforF A

2

,itresultstherelation

N(x~

01 ;

~

b

0

=0;Y)=2 "

1 e 2

s C

F

2

N 2

S

? x

2

01

Axg(x;1=x 2

01 )

#

;(45)

where x

01 = x

0 x

1 = r

t

, Y = ln(s=Q 2

) = ln(1=x)

establishing aonnetion between theross-setion of

the qq pair and the gluon struture funtion in DLA

limit.

We are in good terms to verify the onnetion

among the Kand AGL formulations sinewealready

obtainedthe AGL equation in thedipole formulation,

Eq. (40),the Kequation in theDLA limit, Eq. (42),

therosssetionofthepairthroughthedipoledensity

fromKandthenuleargluondistributionfuntion,Eq.

(45).

HavingEq. (45)inEq. (41)andforx

01

2=Q,as

in[10℄,weobtain

2

xg

A (x;Q

2

)

yln(Q 2

= 2

QCD )

=DQ 2

1 e 2s

2

N

s

? Q

2 xga

; (46)

resultalreadyobtained,andthatgivesGLRasalimit.

Our omparison has physial meaning for dipoles

with small transverse sizes and for the above

onne-tionamongN andxg

A

[Eq. (45)℄.

In Refs. [38, 39℄ it was applied the Wilson

renor-malizationgrouptothemodelofMLerranand

Venu-gopalan. The non-linear evolution equation then

ob-taineddealswiththeweightfuntionoftheolorharge

densities,validatleadingorder

s

andfordensitiesup

to 1= . The omplete analytial solution is not yet

obtainedbut somelimits aredisussed. Atlow

densi-tiesBFKL is reovered,and thenat DLA at largeQ 2

DGLAPisreovered. Inthework[40℄is proposed the

equation

2

xg(x;Q 2

;b

t )

y"

=Q 2

1 1

x

exp(1=)E

1 (1=)

;(47)

where =N

(N

1)=2and(x;Q 2

;b

t )=2

s =(N

1)Q 2

xg(x;Q 2

;b

t ).

Forlarge,afatorizedb

t

dependeneand

onsid-eringaentral ollisionweobtainforthisequation

2

xg(x;Q 2

)

y"

=R 2

Q 2

; (48)

whihsolutionis

xg(x;Q 2

)=R 2

Q 2

ln(1=x); (49)

presentingthe sameQ 2

andx behaviorasthe

asymp-toti solution for AGL. The main point is the partial

saturationof the gluon distribution presented in both

formulations in the asymptoti region. A onnetion

among those two formulations in a more broad

kine-matialregionisstillanopenquestion.

Theasymptoti behaviorof the struture funtion

alsorequiredourattention. Consideringtherelationof

qq

andxg(x;Q 2

)weanwrite[29℄

F

2 (x;Q

2

)= 2

s

9 Z

Q 2

Q 2

0 dQ

2

Q 2

xg(x;Q 2

) (50)

whihisaleadingtwistequation,withlimited

applia-tionforhighdensities,duetohighertwisttermsrelated

withtheUC.

UsingthesolutionofAGLintheasymptotiregime

asinput in theaboveequation we obtainF

2 (x;Q

2

)'

s

3

R 2

Q 2

ln(1=x), whih again presents partial

satura-tion, meaning the Froissart limit is not violated [44℄.

Analogous resultwasobtainedby Kovhegov[42℄

em-ploying the solution of the K equation [11℄. We

ob-tainedthat theasymptotibehaviorofF

2

isageneral

harateristithatappearstobeindependentfrom the

approahthatisused[31℄.

Assuming the asymptoti behavior of the gluon

funtion is xg(x;Q 2

) = 2Q 2

R 2

=3

s

, it implies

satu-rationforF

2 (R

2

Q 2

)forverysmallx. Howeverthis

resultshould betakenwith autionsineit isvalid in

akinematialregionwherehigherorderinthepartoni

densityarenotsigniative. Thesubjetofsaturation

isatrikyoneanditseemswearefarfromestablishing

itsfeatures in asolid theoretialbasis[24℄. Important

ontributions to these hallenging aspets of hdQCD

are to befound in Mueller[24℄ forthe theoretial

dis-ussionandGole-BiernatandWustho[24℄fora

(13)

In[43,44℄wewereabletoshowthat

F

2 (x;Q

2

) = R

2

2 2

X

i e

2

i Z

1=Q 2

0

1=Q 2

d 2

r

t

r 4

t [C

+ ln

q +E

1 (

q

)℄ ; (51)

where

q

=4=9

g

. Fromthatwean estimatetheUC

for F

2

in the DLA limit. For large

q

, and using the

asymptotisolutionofAGL,weobtained[31℄

F

2 (x;Q

2

)' R

2

Q 2

3 2

ln[ 4

s

3

ln (1=x)℄; (52)

when highertwisttermsare onsidered in F

2

. Thisis

a softer behavior, but in both asesthere is no

viola-tionoftheFroissartlimit. Thisaboveequationwasnot

studied inKorMV-JKLWapproahes.

From the already obtained results it follows the

identity[45℄

F

2 (x;Q

2

)

lnQ 2

=F

2 (x;Q

2

); (53)

as an important signature of the asymptoti regime

of QCD for dense systems. It is relevant to mention

that for thesameenter ofmass energythis regimeis

reahedfor nuleus forsmallerpartonidensities than

in thenuleonase,sine

A =A

1=3

N .

VI Phenomenology

From the Glauber-Mueller formalism for high dense

partoni systemswasdemonstrated theAGL equation

and its asymptotibehavior. It wasalso obtainedthe

nuleonandthenulear gluondistributionfuntion as

well as the respetive struture funtions and

deriva-tives. This formulation inorporates the UC required

bytheFroissartbound,throughanonlineardynamis.

Inthissetionthebehaviorofthemainobservables

obtainedin epollisions,andrelevantforeAollisions,

willbeanalysedwiththegoaltoshedsomelightinthe

subjetofUC.

For epwestudiedthebehavioroftheproton

stru-ture funtion F

2

, its derivative F2

lnQ 2

, the harmed

omponentofthestruturefuntionF

2

,andthe

longi-tudinal distributionfuntion,F

L [43℄.

ThereisalargeamountofdatafromHERAto

mo-tivateadetailedstudyoftheseobservablesdiretly

on-neted with thegluondistributionfuntion. As

previ-ously demonstrated thegluon distribution is modied

inaunitarityorretedformulation,meaningthose

ob-servablesshould beaeted.

Wewere lukytoshowthat the F

2

lnQ 2

,theF

2 are

learlymodied. Also,theeA analysisprovides

strik-ing results for the nulear struture funtion F A

and

itsderivative,asanimportantsignatureoftheUC

or-retions. These resultsare importantsinethey area

preditionbothforHERA-Aandfore-RHIC,inwhih

ahighdensepartonsystemshouldbeformed.

TheinreasingofF

2

inHERAinthesmallxregion

(10 2

>x>10 5

) isobservedevenfor small

virtuali-ties(Q 2

1GeV 2

). TakingF

2 x

,forsmallxdata

is ompatible with =0:15 (Q 2

=0:85 GeV 2

) up to

=0:4(Q 2

=20GeV 2

). ThisisdesribedbyDGLAP

withsuitableinput initial onditionforQ 2

and

distri-butionsbydierentgroups[27, 47℄. Itwill ondut to

theideaUCarenotobservableintheHERA

kinemati-alrange. Wehaveshownthatthestruturefuntionis

tooinlusiveinthegluonfuntiontolearlyexpliitate

theUC.

Wearrivedat adierent onlusionapplying AGL

to F

2

lnQ 2

,F

L andF

2

,allobservablesdiretlyassoiated

withthegluonfuntion.

ThederivativeofF

2 is

F

2

lnQ 2

= R

2

Q 2

2 2

X

i e

2

i

[C+ln(

q )+E

1 (

q

)℄; (54)

that we solvedusing thesame proedure asEq. (20).

Theusual parametrizations[27, 47℄donotinlude the

UCforthegluonsexpliitly. WeuseEq. (20)forA=1

asinput,andweobtaintheorretionsfromboth

se-tors quark and gluons. The last one gains in

impor-taneasQ 2

inreases. InFig. (9)theresultsfor F2

lnQ 2

arepresentedfor R 2

=5GeV 2

. Fortheomplete

dis-ussionwerefer to [48℄. The UC forboth setors are

ableto desribe properlythe datainluding the

turn-over. Our onlusions is this is a good observable to

evidentiatethe preseneof theUC.This questionwas

addressedalso in [49℄ alulating the suppression

fa-torsseparately.

We believe that the UC should be extrated from

datarelatedtoobservablesthatarediretlydependent

ofthegluonfuntion. Thelongitudinalstruture

fun-tion F

L

is a diÆult measurement requiring distint

valuesof the enter of massenergy, meaning dierent

energybeams. An alternativeis toonsider the

radia-tionofahardphotonfromtheinidenteletron,

redu-ing theenter of mass energy. If this should be done

weanstudyF

L (x;Q

2

(14)

10

-4

10

-3

10

-2

10

-1

x

0.0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

dF

2

/dlogQ

2

ZEUS

GRV94(LO)

Quark + Gluon Sector

Gluon Sector

Quark Sector

R

2

= 5 GeV

-2

Figure9

Expressed onsidering the quarks transverse

mo-menta due to gluon radiation, the longitudinal

stru-turefuntionreads

F

L (x;Q

2

)=

s (Q

2

)

2 x

2 Z

1

x dy

y 3

8

3 F

2 (y;Q

2

)

+4 X

f e

2

f (1

x

y

)yg(y;Q 2

) 3

5

; (55)

wherey =Q 2

=sxandthedependeneonthegluon

dis-tribution is expliit, meaning this funtion should be

sensitive to unitarity orretions in HERA

kinemati-al region. Our results for small x region are in Fig.

(10)[43℄omparedwith theH1data [50℄. Althoughit

seems to be a good observable to evidentiate the UC

theavailabledata donotallowanydeniteonlusion

fornow.

0.00010

0.00020

0.00030

0.00040

0.00050

0.0

0.2

0.4

0.6

0.8

1.0

H1

GRV(94)LO

GM

F

L

x

Figure10

A problablymorepromissingobservableistherate

R

F = F

2 (x;Q

2

)=F

2 (x;Q

2

), where F

2

is the harmed

omponentof thestruture funtion. Consideringthe

approah ofboson-gluonin order toreate the pair

weobtainedintheGlauber-Muellerformalismtheratio

R .

This ratiois presented in Fig. (11)[43℄ as a

fun-tionofln(1=x). Thereisstrongmodiationoftheratio

oneUCareinludedin thealulation. Weurgedata

in this observable. The suppression is muh stronger

thanin theF

2

ase,andweexpetalowerprodution

ofquarkharmforsmallx,andthisisrelatedwiththe

produtionof J= whih isproportionaltothesquare

ofthegluonfuntion.

0.0

5.0

10.0

15.0

20.0

0.0

0.1

0.2

0.3

0.4

0.0

5.0

10.0

15.0

20.0

0.0

0.1

0.2

0.3

0.4

0.0

5.0

10.0

15.0

20.0

0.0

0.1

0.2

0.3

0.4

0.0

5.0

10.0

15.0

20.0

0.0

0.1

0.2

0.3

0.4

2.5

5.0

10.0

20.0

ln(1/x)

ln(1/x)

R

F

ln(1/x)

ln(1/x)

R

F

R

F

R

F

Figure11

Finally, one of our most striking results onerns

eAphysis,andisrelatedwiththehighdensepartoni

system in the nulear medium. The nulear

shadow-ing is a hallenge for hdQCD and mainly important

for HERA-A, RHIC and LHC physis. We estimated

how the nulear struture funtion and its derivative

aremodiedbytheeetsofhighpartonidensitiy.

Theshadowingorretionsto F A

2

are assoiatedto

theresatteringsoftheqqin thenuleonsintothe

nu-leus, beingdependenton the nuleongluon

distribu-tion funtion. Here also we separate the two ases:

quarksetor,where thegluondistribution isnot

mod-ied byUC,andquark+gluonsetor,wherenowthe

gluon distribution is modied a la Glauber-Mueller.

The results are presented in Fig. (12)[51℄ as a ratio

R

1 = F

A

2 =AF

N

2

, showing that for small x the gluon

setor ontribution should be inluded, and promote

saturation.

We obtain that the suppression due to the

shad-owing in F A

2

is proportionally smaller than in xg

A in

aperturbativeframework,in adierentresult that in

[19℄ wheresoftphysisisthemain issue. Asanew

re-sultthesaturationoftheratioisattainedat HERA-A

regionwhenthegluonsetorisinluded. Thepresene

ofsaturationintheperturbativeregion(Q 2

>1GeV 2

)

denotes the large shadowing orretions in the gluon

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