Saturation and Wilson Line Distributions
Abstract
We introduce a Wilson line distribution function barWtau(v) to study gluon saturation at small Feynman xF, or large tau=ln(1/xF). This new distribution can be obtained from the distribution Wtau(alpha) of the Color Glass Condensate model and the JIMWLK renormalization group equation. barWtau(v) is physically more relevant, and mathematically simpler to deal with because of unitarity of the Wilson line v. A JIMWLK equation is derived for barWtau(v); its properties are studied. These properties are used to complete Mueller's derivation of the JIMWLK equation, though for barWtau(v) and not Wtau(alpha). They are used to derive a generalized Balitsky-Kovchegov equation for higher multipole amplitudes. They are also used to compute the unintegrated gluon distribution at xF=0, yielding a completely flat spectrum in transverse momentum squared k2, with a known height. This is similar but not identical to the mean field result at small k2.
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