Neutrinos from WIMP annihilations

dc.creatorBlennow, Mattias
dc.date2007-10-08
dc.date.accessioned2026-07-07T08:34:43Z
dc.date.available2026-07-07T08:34:43Z
dc.descriptionWe make an improved analysis on the flow of neutrinos originating from WIMP annihilations inside the Sun and the Earth. We treat both neutrino interaction and oscillation effects in a consistent framework. Our numerical simulations are performed in an event based setting, which is useful for both theoretical studies and for creating neutrino telescope Monte Carlos. We find that the flow of muon-type neutrinos is enhanced or suppressed depending on the dominant WIMP annihilation channel.
dc.descriptionSubmitted for the SUSY07 proceedings, 4 pages, LaTeX, 5 figures
dc.identifierhttps://arxiv.org/abs/0710.1493
dc.identifierhttp://arxiv.org/abs/0710.1493
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/139536
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrinos from WIMP annihilations
dc.typetext

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