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arXiv · 1305.0302

Prospects for Indirect Detection of Dark Matter with CTA

Matthew Wood·Jim Buckley·Seth Digel·Stefan Funk·Daniel Nieto·Miguel A. Sanchez-Conde
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Abstract

We discuss the prospects for indirect detection of dark matter (DM) with the Cherenkov Telescope Array (CTA), a future ground-based gamma-ray observatory that will be sensitive to gamma rays in the energy range from a few tens of GeV to 100 TeV. We consider the detectability of DM annihilation in different astrophysical targets with a focus on the Galactic Center (GC) region. With a deep observation of the GC, CTA will be sensitive to DM particles with mass greater than 100 GeV and an annihilation cross section close to the thermal relic value.

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Matthew Wood, Jim Buckley, Seth Digel, Stefan Funk, Daniel Nieto, Miguel A. Sanchez-Conde. 2013-05-01. Prospects for Indirect Detection of Dark Matter with CTA. https://arxiv.org/abs/1305.0302

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