Neutralino spectrum in top-down models of UHECR

Details Neutralino spectrum in top-down models of UHECR Neutralino spectrum in top-down models of UHECR

2002-02-12

arxiv.org/abs/hep-ph/0202111v2

JHEP 0206 (2002) 006

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, revtex, 3 eps figures. Difference between the present work and Montecarlo simulations clarified

Scientific paper

10.1088/1126-6708/2002/06/006

We calculate the cosmic ray spectrum of ultra high energy neutralinos that one should expect provided that the observed ultra high energy cosmic rays are produced by the decay of superheavy particles X, M_X>10^{12} GeV, in supersymmetric models. Our calculation uses an extended DGLAP formalism. Forthcoming cosmic ray observatories should be able to detect these neutralinos.

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