arXiv · hep-ph/0106326
Susy QCD and High Energy Cosmic Rays 1. Fragmentation functions of Susy QCD
Abstract
The supersymmetric evolution of the fragmentation functions (or timelike evolution) within N=1 $QCD$ is discussed and predictions for the fragmentation functions of the theory (into final protons) are given. We use a backward running of the supersymmetric DGLAP equations, using a method developed in previous works. We start from the usual QCD parameterizations at low energy and run the DGLAP back, up to an intermediate scale -assumed to be supersymmetric- where we switch-on supersymmetry. From there on we assume the applicability of an N=1 supersymmetric evolution (ESAP). We elaborate on possible application of these results to High Energy Cosmic Rays near the GZK cutoff.
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Claudio Coriano', Alon E. Faraggi. 2002-01-07. Susy QCD and High Energy Cosmic Rays 1. Fragmentation functions of Susy QCD. https://doi.org/10.1103/physrevd.65.075001
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