Supersymmetric cosmic accelerators: Fluxes at Earth and companion stability

Details Supersymmetric cosmic accelerators: Fluxes at Earth and companion stability Supersymmetric cosmic accelerators: Fluxes at Earth and companion stability

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987phrvd..36..346c&link_type=abstract

Physical Review D (Particles and Fields), Volume 36, Issue 2, 15 July 1987, pp.346-350

Physics

Cosmic-Ray Interactions, X-Ray Binaries

Scientific paper

We perform a complete calculation of the flux of supersymmetric particles emitted by a binary star such as Cygnus X-3 taking into account production of particles in the interior as well as the atmosphere of the main-sequence star. We calculate fluxes at Earth as well as the contribution to heating of the main-sequence star inside the binary system. Although some supersymmetric models predict observable fluxes in future cosmic-ray telescopes, supersymmetry cannot be the source of underground muons from point sources recently reported by some experiments.

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