Searching for supersymmetry in high-energy cosmic-ray interactions

Details Searching for supersymmetry in high-energy cosmic-ray interactions Searching for supersymmetry in high-energy cosmic-ray interactions

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phrvd..33.1239r&link_type=abstract

Physical Review D (Particles and Fields), Volume 33, Issue 5, 1 March 1986, pp.1239-1246

Physics

4

Supersymmetric Partners Of Known Particles, Cosmic-Ray Interactions

Scientific paper

We survey the prospects for producing and detecting supersymmetric particles in high-energy cosmic-ray interactions. We find that the production and subsequent decay of light (~3 GeV) gluinos can lead to fluxes of neutral, weakly interacting superparticles, photinos or scalar neutrinos, which might be detected in large, underwater neutrino detectors. We identify several reactions, γ~N-->g~qX in the 10-100-TeV region and the resonant process ν~ee--->W~-, which can lead to measurable reaction rates in the discussed 105-kiloton DUMAND-type detector.

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