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Evolution Kernels for Light-Ray Operators Twist 2 and Twist 3 Contributions
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Evolution Kernels for Light-Ray
Operators :
Twist 2 and Twist 3 Contributions
Johannes Blu?mlein?, Bodo Geyer? and Dieter Robaschik?
?DESY – Zeuthen, Platanenallee 6, D – 15735 Zeuthen, Germany
? Naturwissenschaftlich–Theoretisches Zentrum der Universita?t Leipzig,
Augustusplatz 10, D–04109 Leipzig, Germany
Abstract. The general evolution kernels of the twist 2 light–ray operators for
unpolarized and polarized deep inelastic scattering are calculated inO(αs). From
these evolution kernels a series of special evolution equations can be derived,
among them the Altarelli-Parisi equations and the evolution equation for the
meson wave function. In the case of twist 3 the results of Balitzki and Braun are
confirmed.
INTRODUCTION
The study of the Compton amplitude for scattering of a virtual photon off
a hadron is one of the basic tools in QCD to understand the short–distance
behavior of the theory. The Compton amplitude for the general case of non–
forward scattering is given by
Tμν(p+, p?, Q) = i
∫
d4xeiqx〈p2|T (Jμ(x/2)Jν(?x/2))|p1〉, (1)
where p+ = p2 + p1, p? = p2 ? p1 = q1 ? q2 and q = (q1 + q2)/2. The time–
ordered product in eq. (1) can be represented in terms of the operator product
expansion. Here we use the representation derived in ref. [1,2]
T (Jμ(x/2)Jν(?x/2)) ≈
∫ +∞
?∞
dκ?
∫ +∞
?∞
dκ+[Ca(x
2, κi, μ
2)Sμν
ρσx?ρO
a
σ(κix?, μ
2)
+Ca,5(x
2, κi, μ
2)εμν
ρσx?ρO
a
5,σ(κix?, μ
2)], (2)
with Sμνρσ = gμνgρσ ? gμρgνσ ? gμσgνρ and εμνρσ denoting the Levi–Civita
symbol. The light–like vector x? = x + r(x.r/r.r)
[√
1? x.xr.r/(x.r)2 ? 1
]
is
c? 1997 American Institute of Physics 1
2related to x and a subsidiary four–vector r, Ca and Ca5 denote the respec-
tive coefficient functions. Different kinematic situations in the Bjorken region
are described by different matrix–elements of the involved light–ray operators
Oaσ(κ+x?, κ?x?, μ
2) and Oa5,σ(κ+x?, κ?x?, μ
2). Let us illustrate this with the help
of the non–si
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