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Detecting supersymmetric dark matter in M31 with CELESTE ?

E. Nuss 1 G. Moultaka 2 Alain Falvard 1 E. Giraud 1 A. Jacholkowska 1 K. Jedamzik 2 J. Lavalle 1 F. Piron 1 M. Sapinski 1 P. Salati 3 Richard Taillet 3 
1 LPTA - Laboratoire de Physique Théorique et Astroparticules
2 PMT - Laboratoire de Physique Mathématique et Théorique
3 LAPTH - Laboratoire d'Annecy-le-Vieux de Physique Théorique
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.
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http://hal.in2p3.fr/in2p3-00087404
Contributor : Dominique Girod Connect in order to contact the contributor
Submitted on : Monday, July 24, 2006 - 11:13:22 AM
Last modification on : Saturday, June 25, 2022 - 9:40:55 AM

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E. Nuss, G. Moultaka, Alain Falvard, E. Giraud, A. Jacholkowska, et al.. Detecting supersymmetric dark matter in M31 with CELESTE ?. The SN factory Consortium - SF2A-2002 - Semaine de l'Astrophysique Française, Jun 2002, Paris, France. ⟨in2p3-00087404⟩

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