TeV Dark Matter detection by Atmospheric Cerenkov Telescopes

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dc.creatorFerrer, Francesc
dc.date2005-05-19
dc.date.accessioned2026-07-07T02:17:38Z
dc.date.available2026-07-07T02:17:38Z
dc.descriptionGround based Atmospheric Cerenkov Telescopes have recently unveiled a TeV gamma-ray signal from the direction of the Galactic Centre. We examine whether these gamma-rays, observed by the VERITAS, CANGAROO-II and HESS collaborations, may arise from annihilations of dark matter particles. Emission from nearby dwarf spheroidals, such as Sagittarius, could provide a test of this scenario.
dc.description4 pages, to appear in the proceedings of the 40th Rencontres de Moriond, "Very High Energy Phenomena in the Universe"
dc.identifierhttps://arxiv.org/abs/astro-ph/0505414
dc.identifierhttp://arxiv.org/abs/astro-ph/0505414
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9245
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTeV Dark Matter detection by Atmospheric Cerenkov Telescopes
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