Detecting supersymmetric dark matter in M31 with CELESTE ?

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dc.creatorNuss, E.
dc.creatorMoultaka, G.
dc.creatorFalvard, A.
dc.creatorGiraud, E.
dc.creatorJacholkowska, A.
dc.creatorJedamzik, K.
dc.creatorLavalle, J.
dc.creatorPiron, F.
dc.creatorSapinski, M.
dc.creatorSalati, P.
dc.creatorTaillet, R.
dc.date2002-12-28
dc.date.accessioned2026-07-07T02:07:01Z
dc.date.available2026-07-07T02:07:01Z
dc.descriptionIt is widely believed that dark matter exists within galaxies and clusters of galaxies. Under the assumption that this dark matter is composed of the lightest, stable supersymmetric particle, assumed to be the neutralino, the feasibility of its indirect detection via observations of a diffuse gamma-ray signal due to neutralino annihilation within M31 is examined.
dc.descriptionLatex, 5 pages, 3 figures, to appear in the proceedings of the French Astrophysical Society, 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0212560
dc.identifierhttp://arxiv.org/abs/astro-ph/0212560
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5561
dc.subjectAstrophysics
dc.titleDetecting supersymmetric dark matter in M31 with CELESTE ?
dc.typetext

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