Indirect Detection of Neutralino Dark Matter with Neutrino Telescopes

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dc.creatorNezri, E.
dc.date2002-11-06
dc.date.accessioned2026-07-07T03:48:28Z
dc.date.available2026-07-07T03:48:28Z
dc.descriptionPrinciple of neutralino dark matter detection with neutrino telescopes and predictions are reviewed. The future Antares detector is described. Prospection in the CMSSM is exposed including comparison with experiment sensitivities of both neutrino indirect detection and direct detection experiments. Results in other frameworks are shortly surveyed. Models with a non negligible neutralino higgsino fraction are promising for neutrino telescopes detection.
dc.descriptionTalk given at SUSY02, Desy, Hambourg, Germany June 17-23
dc.identifierhttps://arxiv.org/abs/hep-ph/0211082
dc.identifierhttp://arxiv.org/abs/hep-ph/0211082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/42021
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.titleIndirect Detection of Neutralino Dark Matter with Neutrino Telescopes
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