Dark Matter Candidates - Axions, Neutralinos, Gravitinos, and Axinos

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dc.creatorSteffen, Frank Daniel
dc.date2008-11-20
dc.date.accessioned2026-07-07T12:42:46Z
dc.date.available2026-07-07T12:42:46Z
dc.descriptionThe existence of dark matter provides strong evidence for physics beyond the Standard Model. Extending the Standard Model with the Peccei-Quinn symmetry and/or supersymmetry, compelling dark matter candidates appear. For the axion, the neutralino, the gravitino, and the axino, I review primordial production mechanisms, cosmological and astrophysical constraints, experimental searches, and prospects for experimental identification.
dc.description31 pages, 14 figures
dc.identifierhttps://arxiv.org/abs/0811.3347
dc.identifierhttp://arxiv.org/abs/0811.3347
dc.identifierEur.Phys.J.C59:557-588,2009
dc.identifierdoi:10.1140/epjc/s10052-008-0830-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/220189
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.titleDark Matter Candidates - Axions, Neutralinos, Gravitinos, and Axinos
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