Q^2 Dependence of the azimuthal Asymmetry in Unpolarized Drell-Yan

a r X i v :h e p -p h /0407208v 1 19 J u l 2004

GEF-Th-8/2004

Q 2Dependence

of the Azimuthal Asymmetry in Unpolarized Drell-Yan

Elvio Di Salvo

Dipartimento di Fisica and I.N.F.N.-Sez.Genova,Via Dodecaneso,33

-16146Genova,Italy

Abstract

We study the azimuthal asymmetry of the unpolarized Drell-Yan in the framework of the T-odd functions.We ?nd,on the basis of quite general arguments,that for |q ⊥|<

experimental results support this conclusion.

PACS numbers:13.85.Qk,13.88.+e

1Introduction

As is well-known,unpolarized Drell-Yan(DY)presents an azimuthal asymmetry. This was seen,for example,in reactions of the type[1-3]

π?N→μ+μ?X,(1)

where N is an unpolarized tungsten or deuterium target,which scatters a negative pion beam.Such an asymmetry was originally explained as a?rst order QCD correc-tion e?ect[1].Recently,however,it has been attributed[4,5]to the quark polarization in unpolarized(or spinless)hadrons[6,7].Such a polarization reads

p⊥×P

Π=

naive parton model.Sect.3is dedicated to the quark correlation matrix,containing ”soft”information for the inclusive cross sections at high momentum transfers.In sect.4we determine the parameterμ0,either by comparison between the correlation matrix and the density matrix,or starting from a simple model.In sect.5we calculate the azimuthal asymmetry parameterν(see formula(4)below)in terms of the polarizationsΠof the active https://www.360docs.net/doc/5d15284809.html,ing the result of sect.4,we obtain the Q2 dependence of this asymmetry,which we compare with experimental https://www.360docs.net/doc/5d15284809.html,stly we draw a short conclusion.

2The unpolarized Drell-Yan cross section

The DY angular di?erential cross section is conventionally expressed as

1

d?=

3

λ+3

(1+λcos2θ+μsin2θcosφ+

1

d?→

them,as far as possible,as an e?ect of the quark transverse momentum,essential in the polarization(2).In particular,such an interpretation of the azimuthal asymmetry accounts rather well[4]for the observed large size ofνand small size ofμ[1,2].

3The quark correlation matrix

The correlation matrix is a very important tool for calculating inclusive reaction cross sections at high momentum transfers.Indeeed,in the framework of factorization[11], this matrix contains all information concerning the”soft”functions entering the the-oretical expressions of such cross sections.For example,the DY cross section,which we are interested in,has the following convolutive expression:

α2

(x a+x b)s

kν+kνk,(7) k and

6 d2p⊥T r[ΦA(x a,p⊥)γμΦB(x b,q⊥?p⊥)γν].(8)ΦA andΦB are the correlation matrices of the active quark and antiquark,which belong to the two initial hadrons,denoted here respectively as A and B.?The corre-lation matrix may be parametrized according to the Dirac algebra,taking into account Lorentz and parity invariance.On the contrary,we do not consider restrictions due to time reversal,since we admit the so-called T-odd functions,i.e.,some particular interference terms,which,without violating any symmetry,change their sign under that transformation.Obviously,not all the Dirac components will contribute to a single process.

In order to determineμ0,it is necessary to consider a polarized nucleon,e.g.,a transversely polarized one.In this case the correlation matrix is parametrized as

Φ=Φ⊥?Φ0a+Φ0b+Φ1+ΦO,(9) where

Φ0a=1

2

h1Tγ5[/S,/n+]

+1

2

λ⊥h⊥1Tγ5[/p⊥,/n+],(10)

Φ0b=

1

4

λ⊥ h⊥Tγ5[/S,/p⊥]+h Tμ0γ5[/n?,/n+] ,(11)Φ1=

1

2μ0 f⊥1T?μνρσγμnν+pρ⊥Sσ+ih⊥112P+ie sγ5p⊥·S.(13) Here we have used the MT notations for the”soft”functions.Moreover we have set λ⊥=?S·p⊥/μ0,p⊥=p?P·p

P

2

h⊥1[/p⊥,/n+],(15) which corresponds to the quark polarizationΠ(eq.(2)),as it is straightforward to check[6,7].It is important to stress that this polarization is due to a coherence e?ect, for example to one gluon exchange between the hadron A and the active parton of the hadron B,or vice-versa[12].This e?ect can be factorized only if the condition(3) is ful?lled[4].Moreover the factorμ0must be the same for all the functions involved,

5

in order to normalize them appropriately.This factor was assumed to be equal to the rest mass of the hadron[8,13].As we shall see in a moment,this is not the most suitable choice,in order to interpret the functions contained in the correlation matrix as probability densities or interference terms.

4

Determining μ0

We follow two di?erent procedures for deriving the correct expression of the parameter μ0.The ?rst procedure consists in comparing the correlation matrix with the density matrix,to which Φreduces for non-interacting quarks.The second procedure is based on a simple,but rather general,model,without any ad hoc assumptions.

4.1The density matrix

The density matrix of a free,on-shell quark in a transversely polarized nucleon reads

ρ⊥=

T =±1/2

q T (x,p ⊥)

1

2

q (x,p 2⊥)(/

p +m )+

1

2

[/S ,/p ]+/p sinθ′

?C 1+mC 2

+O (P ?1).

(17)

Here we have set

q (x,p 2⊥)

=

T =±1/2

q T (x,p ⊥),

δq ⊥(x,p ⊥)=

T =±1/2

2T q T (x,p ⊥),

(18)

C 1=E q

1

C2=/S+1

2

/n′? 1?m√

2x P n++p⊥+O P?1 .(22)

We get,for a free,on-shell quark[14],

f1=f⊥1=q,λ⊥h⊥T=sinθ′δq⊥,(23)λ⊥h⊥1T=(1??1)sinθ′δq⊥,μ0λ⊥h T=(1??1)sinθ′E qδq⊥,(24)λ⊥g1T=(1??2)sinθ′δq⊥,λ⊥g⊥T=(1??3)sinθ′δq⊥.(25) Here?1=m/E q,?2=m/x P and?3=m/2|p|are the correction terms to the chiral limit,which are generally small for light quarks.The terms of order O[(m2+p2⊥)/P2] have been neglected.As regardsμ0,we require the various functions to be normalized, in the chiral limit,likeδq⊥,which is a di?erence between two probability densities. Therefore we assume

λ⊥=sinθ′,(26) which,according to eqs.(21)and(14),implies

μ0=|p|.(27) Two remarks are in order aboutμ0.

?This parameter is frame dependent,as well as the correlation matrix and the density matrix;however,in a speci?c reaction,it can be expressed in terms of

7

Lorentz invariant quantities.In particular,for DY,in the center-of-mass system we have

μ0?Q

Here A l and B l are related to partial wave amplitudes;moreoverθ0andφ0are re-spectively the polar and the azimuthal angle of the quark momentum,assuming the polar axis along P and,as the azimuthal plane,the one through P and s.In the P-frame one has

P l(cosθ0)~1,P1l(cosθ0)~|p⊥|

x P

(Ucosφ0+V sinφ0),(34) where U and V are real functions of x and p2⊥,made up with A l and B l.Since s is an axial vector,parity conservation implies U=0.Therefore

I~|p⊥|x P|p⊥×s|,(35) where the±sign depends on the sign of sinφ0.Therefore the interference term I is T-odd.Moreover,setting s=P/|P|,and comparing eq.(35)with eq.(2),we identify h⊥1with V and we get

μ0=x P.(36) Eqs.(36)predicts that the quark tranverse polarization in an unpolarized(or spinless) hadron decreases as P?1.But in the center-of-mass frame,for Q>>M one has x P?Q/2,therefore we recover the result(28).

5Azimuthal asymmetry

Inserting formulae(7)to(13)into eq.(6),the di?erential cross section reads,under the condition(3),

(x a+x b)s α2

μ20 (37)

Here the sum runs over all the light?avors and anti?avors,u,d,s,d,

where f1A and f1B are the unpolarized densities of the active https://www.360docs.net/doc/5d15284809.html,stly

H= d2p⊥h⊥1A(x a,p2⊥)h⊥1B[x a,(q⊥?p⊥)2]S,(39) where

S=[2p⊥·n(q⊥?p⊥)·n?p⊥·(q⊥?p⊥)](40) and n=q⊥/|q⊥|.But eq.(39)implies that for q⊥→0H∝q2⊥:

H=H0q2⊥,(41) where H0=H0(x a,x b,q2⊥)assumes a?nite value for q⊥=https://www.360docs.net/doc/5d15284809.html,paring eq.(37) with eq.(4)yields

ν=2

f e2f F f.(42)

Inserting eqs.(41)and(28)into eq.(42),we get

ν=A0q2⊥

Appendix

Here we derive formula(17)for the density matrix of a quark.To this end we write formula(16):

ρ⊥= T=±1/2q T(x,p⊥)1

?p⊥·S

|p|,sinφ=

m2+p2.(A.7)

As a result we get

S q=S+ p

√√

References

[1]NA10Coll.,S.Falciano et al.:Z.Phys.C-Particles and Fields31(1986)513

[2]NA10Coll.,M.Guanziroli et al.:Z.Phys.C-Particles and Fields37(1988)

545

[3]J.S.Conway et al.:Phys.Rev.D39(1989)92

[4]D.Boer,S.Brodsky and D.-S.Huang:Phys.Rev.D67(2003)054003

[5]D.Boer:Phys.Rev.D60(1999)014012

[6]D.Boer and P.J.Mulders:Phys.Rev.D57(1998)5780

[7]E.Di Salvo:AIP Conf.Proc.675(2003)494

[8]P.J.Mulders and R.D.Tangerman:Nucl.Phys.B461(1996)197

[9]J.C.Collins:Phys.Lett.B536(2002)43

[10]J.C.Collins and D.E.Soper:Phys.Rev.D16(1977)2219

[11]See,e.g.,J.C.Collins:Phys.Rev.D57(1998)3051;”Perturbative QCD”,A.H.

Mueller ed.,World Scienti?c,Singapore,1989

[12]S.J.Brodsky,D.S.Hwang and I.Schmidt:Nucl.Phys B642(2002)344

[13]J.Ralston and D.E.Soper:Nucl.Phys B152(1979)109

[14]E.Di Salvo:Int.J.Mod.Phys.A18(2003)5277

[15]S.J.Brodsky,D.S.Hwang and I.Schmidt:Phys Lett.B530(2002)99

[16]X.Ji,J.-P.Ma and F.Yuan:Nucl.Phys.B652(2003)383

[17]X.Ji and F.Yuan:Phys.Lett.B543(2002)66

[18]A.V.Belitsky,X.Ji and F.Yuan:Nucl.Phys.B656(2003)165

12

4

6

8

1012

14

16

Q GeV

-0.1

-0.0500.050.10.15Ν

Figure 1:The behaviour of the asymmetry parameter νvs Q ,at constant |q ⊥|<

and

4

5

67

8

Q GeV

-0.05

00.05

0.10.15Ν

Figure 2:Same as ?g.1,

s =19.1

GeV .Data are taken from ref.2and ?tted with formula ν=A 0ρ,A 0=1.35

14

0.1

0.2

0.30.4

0.5

0.6

Ρ

00.10.20.30.4ΝFigure 4:Same as ?g.3,

相关主题
相关文档
最新文档