Supersymmetric Dark Matter Candidates - The Lightest Neutralino, the Gravitino, and the Axino

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dc.creatorSteffen, Frank Daniel
dc.date2007-11-08
dc.date2007-11-28
dc.date.accessioned2026-07-07T08:45:15Z
dc.date.available2026-07-07T08:45:15Z
dc.descriptionIn supersymmetric extensions of the Standard Model, the lightest neutralino, the gravitino, and the axino can appear as the lightest supersymmetric particle and as such provide a compelling explanation of the non-baryonic dark matter in our Universe. For each of these dark matter candidates, I review the present status of primordial production mechanisms, cosmological constraints, and prospects of experimental identification.
dc.description13 pages, 8 figures; Submitted for the SUSY07 proceedings; revised version (comments and references added, typos corrected)
dc.identifierhttps://arxiv.org/abs/0711.1240
dc.identifierhttp://arxiv.org/abs/0711.1240
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142909
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.titleSupersymmetric Dark Matter Candidates - The Lightest Neutralino, the Gravitino, and the Axino
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