Detecting supersymmetric dark matter in M31 with CELESTE ?

Thumbnail Image

Date

Authors

Journal Title

Journal ISSN

Volume Title

Publisher

Abstract

Description

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.
Latex, 5 pages, 3 figures, to appear in the proceedings of the French Astrophysical Society, 2002

Keywords

Astrophysics

Citation

URI

http://salesiana.dossiersoluciones.com/handle/123456789/5561

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0212560
 http://arxiv.org/abs/astro-ph/0212560

Collections

arXiv