Dark Matter searches with imaging atmospheric Cherenkov telescopes
E. Moulin
TL;DR
This paper reviews recent results from imaging atmospheric Cherenkov telescopes in the search for dark matter through gamma-ray detection from WIMP annihilations in various astrophysical targets.
Contribution
It provides an overview of recent observational results and discusses the potential of IACTs in dark matter detection efforts.
Findings
Detection limits set by current IACT observations
Constraints on WIMP properties from gamma-ray data
Future prospects for dark matter searches with IACTs
Abstract
The annihilations of WIMPs produce high energy gamma-rays in the final state. These high energy gamma-rays may be detected by imaging atmospheric Cherenkov telescopes (IACTs). Amongst the plausible targets are the Galactic Center, the centre of galaxy clusters, dwarf Sphreroidal galaxies and substructures in Galactic haloes. I will review on the recent results from observations of ongoing IACTs.
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