Detecting supersymmetric dark matter in M31 with CELESTE ?
Astrophysics
2007-05-23 v1
Abstract
It is widely believed that dark matter exists within galaxies and clusters of galaxies. Under the assumption that this dark matter is composed of the lightest, stable supersymmetric particle, assumed to be the neutralino, the feasibility of its indirect detection via observations of a diffuse gamma-ray signal due to neutralino annihilation within M31 is examined.
Cite
@article{arxiv.astro-ph/0212560,
title = {Detecting supersymmetric dark matter in M31 with CELESTE ?},
author = {E. Nuss and G. Moultaka and A. Falvard and E. Giraud and A. Jacholkowska and K. Jedamzik and J. Lavalle and F. Piron and M. Sapinski and P. Salati and R. Taillet},
journal= {arXiv preprint arXiv:astro-ph/0212560},
year = {2007}
}
Comments
Latex, 5 pages, 3 figures, to appear in the proceedings of the French Astrophysical Society, 2002