Neutrino Indirect Detection of Neutralino Dark Matter in the CMSSM

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dc.creatorBertin, V.
dc.creatorNezri, E.
dc.creatorOrloff, J.
dc.date2002-04-12
dc.date2002-07-15
dc.date.accessioned2026-07-07T12:02:53Z
dc.date.available2026-07-07T12:02:53Z
dc.descriptionWe study potential signals of neutralino dark matter indirect detection by neutrino telescopes in a wide range of CMSSM parameters. We also compare with direct detection potential signals taking into account in both cases present and future experiment sensitivities. Only models with neutralino annihilation into gauge bosons can satisfy cosmological constraints and current neutrino indirect detection sensitivities. For both direct and indirect detection, only next generation experiments will be able to really test this kind of models.
dc.description16 pages, 19 figures; v4: a few clarifications and significant improvement of references
dc.identifierhttps://arxiv.org/abs/hep-ph/0204135
dc.identifierhttp://arxiv.org/abs/hep-ph/0204135
dc.identifierEur.Phys.J.C26:111-124,2002
dc.identifierdoi:10.1140/epjc/s2002-01043-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207591
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleNeutrino Indirect Detection of Neutralino Dark Matter in the CMSSM
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