Dark Matter and Cosmic Rays from Light Gauginos

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dc.creatorFarrar, Glennys R.
dc.date1997-04-13
dc.date.accessioned2026-07-07T04:01:31Z
dc.date.available2026-07-07T04:01:31Z
dc.descriptionAn attractive class of SUSY-breaking mechanisms predicts a photino mass of order 1 GeV. Relic photinos can naturally account for the observed dark matter. Detection of these light photinos is discussed and contrasted with conventional WIMPs. In this scenario the gluino mass is about 100 MeV. The lightest gluino-containing baryon could account for the recently observed ultra-high energy cosmic rays, which violate the GZK bound.
dc.descriptionInvited talk IDM96, Sheffield, England, Sept. 1996. 7 pages with 2 figs, latex
dc.identifierhttps://arxiv.org/abs/hep-ph/9704309
dc.identifierhttp://arxiv.org/abs/hep-ph/9704309
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46925
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDark Matter and Cosmic Rays from Light Gauginos
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