Published December 24, 2008 | Version v1
Journal article

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

  • 1. IRFU/DSM/CEA, CE Saclay, F-91191 Gif-sur-Yvette, Cedex (France)
  • 2. Laboratoire de Physique Theorique et Astroparticules, CNRS/IN2P3, Universite Montpellier II, CC70, Place Eugene Bataillon, F-34095 Montpellier cedex 5 (France)
  • 3. LPNHE, Universite Pierre et Marie Curie Paris 6, Universite Denis Diderot Paris 7, CNRS/IN2P3, 4 Place Jussieu, F-75252 Paris Cedex (France)
  • 4. Laboratoire d'Annecy-le-Vieux de Physique des Particules, CNRS/IN2P3, 9 Chemin de Bellevue, BP110, F-74941 Annecy-le-Vieux Cedex (France)
  • 5. Universitaet Hamburg, Institut fuer Experimentalphysik, Luruper Chaussee 149, D 22761 Hamburg (Germany)

Description

WIMP pair annihilations produce high energy gamma-rays in the final state, which can be detected by Imaging Atmospheric Cherenkov Telescopes such as the H.E.S.S. array. We focus in this contribution on searches towards dwarf galaxies and mini-spikes around intermediate mass black holes (IMBHs) in the Galactic halo. H.E.S.S. observations towards the nearby dwarf galaxies Sagittarius and Canis Major are presented. Using realistic modellings for the dark matter (DM) density profiles, constraints on the velocity-weighted annihilation cross section σv of DM particles are derived in the framework of Supersymmetric and Kaluza-Klein models. A search for DM mini-spikes around IMBHs is described as well as constraints on the particle physics parameters.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1085
Journal Issue
1
Journal Page Range
p. 685-688
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
4. international meeting on high energy gamma-ray astronomy
Dates
7-11 Jul 2008
Place
Heidelberg (Germany)

Optional Information

Notes
(c) 2009 American Institute of Physics
Collaborations
H.E.S.S. Collaboration