On the detectability of gamma-rays from Dark Matter annihilation in the Local Group with ground-based experiments

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dc.creatorPieri, Lidia
dc.creatorBranchini, Enzo
dc.date2003-07-02
dc.date.accessioned2026-07-07T02:08:54Z
dc.date.available2026-07-07T02:08:54Z
dc.descriptionRecent studies have suggested the possibility that the lightest supersymmetric particle is a suitable dark matter candidate. In this theoretical framework, annihilations in high density environments like the center of dark matter haloes may produce an intense flux of gamma-rays. In this paper we discuss the possibility of detecting the signatures of neutralino annihilation in nearby galaxies with next generation ground-based detectors.
dc.descriptionto appear in Proceedings of ICRC 2003
dc.identifierhttps://arxiv.org/abs/astro-ph/0307042
dc.identifierhttp://arxiv.org/abs/astro-ph/0307042
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6237
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleOn the detectability of gamma-rays from Dark Matter annihilation in the Local Group with ground-based experiments
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