Dark Matter and the Scale of SUSY Breaking

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dc.creatorBorgani, Stefano
dc.creatorMasiero, Antonio
dc.date1997-01-30
dc.date.accessioned2026-07-07T04:01:14Z
dc.date.available2026-07-07T04:01:14Z
dc.descriptionWe review the prospects for dark matter (DM) in two classes of supersymmetric (SUSY) models which are characterized by the different mechanism of SUSY breaking, namely the more common supergravity models with very large scale of SUSY breaking and the recent schemes where SUSY is broken at a relatively low scale and gravitinos are likely to be the lightest SUSY particle. We point out that the former scheme is in general associated with the cold dark matter (CDM) scenario, while the latter predicts a warm dark matter (WDM) dominated Universe.
dc.description11 pages plus one postscript figure, LaTeX used; Invited talk at the XII International Conference of the Italian Society of General Relativity and Physics of Gravitation, Rome, Sept.23-27, 1996
dc.identifierhttps://arxiv.org/abs/hep-ph/9701417
dc.identifierhttp://arxiv.org/abs/hep-ph/9701417
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/46821
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleDark Matter and the Scale of SUSY Breaking
dc.typetext

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