Dark matter searches with H.E.S.S: nearby dwarf galaxies and IMBH mini-spikes

Astronomy and Astrophysics – Astrophysics

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Scientific paper

WIMP pair annihilations produce high energy gamma-rays, which can be detected by IACTs such as the H.E.S.S. array of Imaging Atmospheric Cherenkov telescopes.
Nearby dwarf galaxies and mini-spikes around intermediate-mass black holes (IMBHs) in the Galactic halo are possible targets for the observation of these annihilations. H.E.S.S. observations on the nearby dwarf galaxy candidate Canis Major is reported. Using a modelling of the unknown dark matter density profile, constraints on the velocity-weighted annihilation cross section of DM particles are derived in the framework of Supersymmetric (pMSSM) and Kaluza-Klein (KK) models. Next, a search for DM mini-spikes around IMBHs is described and constraints on the particle physics parameters in various scenarios are given.

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