Matière noire et rayons cosmiques galactiques

Abstract : Dark matter is one of the major problems encountered by modern cosmology and astrophysics, resisting the efforts of both theoreticians and experimentalists. The problem itself is easy to state : many indirect astrophysical measurements indicate that the mass contained in the Universe seems to be dominated by a new type of matter which has never been directly seen yet, this is what is called dark matter. This hypothesis of dark matter being made of new particles is of great interest for particle physicists, whose theories provide many candidates : dark matter is one of the major topics of astroparticle physics. This "habilitation à diriger des recherches" focuses on searching dark matter in the form of new particles, more precisely to indirect detection, i.e. the search of particles produced by dark matter annihilation rather than dark matter particles themselves. In this framework, I will present the studies I have been doing in the field of cosmic rays physics, in several collaborations. In particular, the study of its antimatter component can give invaluable information about dark matter.
Document type :
Habilitation à diriger des recherches
Cosmologie et astrophysique extra-galactique [astro-ph.CO]. Université de Savoie, 2010
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  • HAL Id : tel-00633127, version 1



Richard Taillet. Matière noire et rayons cosmiques galactiques. Cosmologie et astrophysique extra-galactique [astro-ph.CO]. Université de Savoie, 2010. 〈tel-00633127〉



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