TeV Dark Matter detection by Atmospheric Cerenkov Telescopes

Details TeV Dark Matter detection by Atmospheric Cerenkov Telescopes TeV Dark Matter detection by Atmospheric Cerenkov Telescopes

2005-05-19

arxiv.org/abs/astro-ph/0505414v1

Astronomy and Astrophysics

Astrophysics

4 pages, to appear in the proceedings of the 40th Rencontres de Moriond, "Very High Energy Phenomena in the Universe"

Scientific paper

Ground 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.

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