Jul 26 – 30, 2010
Montpellier 2 University
Europe/Paris timezone

Cosmic Ray propagation uncertainties and Dark Matter

Jul 26, 2010, 11:45 AM
Amphithéatre Dumontet (Montpellier 2 University)

Amphithéatre Dumontet

Montpellier 2 University

Place Eugene Bataillon, 34095 Montpellier Cedex 5 FRANCE
Talk Dark Matter Indirect Searches Plenary session : Indirect Searches 1


Mr Richard Taillet (Université de Savoie/LAPTH)


Some of the antimatter (antiprotons or positrons) present in cosmic rays could be due to the annihilation of dark matter particles. Indirect searches based on these signals require to be able to model the propagation process, from the annihilation location to the Solar System. The physical processes are well known : diffusion, convection, energy losses and reacceleration. The physical parameters describing these effect (diffusion coefficient, convection velocity, etc) can be constrained by studying secondary-to-primary ratios of nuclei in cosmic rays. I will present the uncertainties related to this procedure and the importance for indirect searches or dark matter.

Primary author

Mr Richard Taillet (Université de Savoie/LAPTH)


Mr David Maurin (LPNHE) Ms Fiorenza Donato (INFN) Mr Pierre Salati (Université de Savoie/LAPTH)

Presentation materials