arXiv:astro-ph/0011553·v1·Astrophysics
Annihilations from the Galactic Centre
G.Bertone (1) · G.Sigl (2) · J.Silk (1) ((1) Department of Astrophysics, University of Oxford; (2) Institut d'Astrophysique de Paris)
Abstract
A massive black hole is present at the centre of our galaxy and inevitably accretes dark matter particles, creating a region of very high particle density. The annihilation rate is enhanced with a large number of e+e- pairs produced either directly or by successive decays of mesons. We evaluate the synchrotron emission (and self-absorption) associated with the propagation of these particles through the galactic magnetic field and give constraints on the values of mass and cross section of the dark matter particles.
Comments: 7 pages, 3 figures, contribution to the proceedings of the 3rd International Workshop on the Identification of Dark Matter (IDM2000) in York, in press