Supersymmetry and ultrahigh-energy cosmic rays

Details Supersymmetry and ultrahigh-energy cosmic rays Supersymmetry and ultrahigh-energy cosmic rays

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55..469r&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, July 29, 1985, p. 469-472.

Physics

9

Cosmic Rays, Energetic Particles, High Energy Interactions, Neutrinos, Particle Production, Supersymmetry, Atmospheric Radiation, Elementary Particle Interactions, Pair Production, Particle Energy, Particle Mass

Scientific paper

The production of supersymmetric particles in ultrahigh energy cosmic ray interactions in the atmosphere is investigated. It is found that the pair production and subsequent decay of a light (about 3-5 GeV) gluino can lead to fluxes of neutral, weakly interacting superparticles which can be comparable to neutrino fluxes. Relevant processes for detecting photinos or scalar neutrinos in large neutrino detectors are discussed and several reactions with cross sections as large as those of ordinary nu interactions are examined.

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