Supersymmetric candidates for dark matter

dc.creatorFornengo, N.
dc.date1998-04-28
dc.date.accessioned2026-07-07T02:26:42Z
dc.date.available2026-07-07T02:26:42Z
dc.descriptionDirect and indirect detection rates of relic neutralinos are reviewed in the framework of the Minimal Supersymmetric Standard Model. The theoretical estimates are compared with the most recent experimental limits from low-background detectors and neutrino telescopes. The properties of neutralino under the hypothesis that preliminary experimental results of the DAMA/NaI Collaboration may be indicative of a yearly modulation effect are examined.
dc.description10 pages, 6 figures, LaTeX, uses psfig.sty and dmtrieste.sty (the full paper with high resolution figures is available at http://www.to.infn.it/~fornengo/proclist.html)
dc.identifierhttps://arxiv.org/abs/astro-ph/9804295
dc.identifierhttp://arxiv.org/abs/astro-ph/9804295
dc.identifierProceedings of "DM97", 1997, page 14 (editor P. Salucci)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12381
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleSupersymmetric candidates for dark matter
dc.typetext

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