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| HAL : hal-00707457, version 1 |
| arXiv : 1205.1004 |
| Fiche détaillée |  Récupérer au format |
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| Dark Matter Indirect Signatures |
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| Julien Lavalle1Pierre Salati2 |
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| (04/05/2012) |
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| The astronomical dark matter could be made of weakly interacting and massive particles. If so, these species would be abundant inside the Milky Way, where they would continuously annihilate and produce cosmic rays. Those annihilation products are potentially detectable at the Earth, and could provide indirect clues for the presence of dark matter species within the Galaxy. We will review here the various cosmic radiations which the dark matter can produce. We will examine how they propagate throughout the Milky Way and compare the dark matter yields with what pure astrophysical processes are expected to generate. The presence of dark matter substructures might enhance the signals and will be briefly discussed. |
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| 1 : | LPTA - Laboratoire de Physique Théorique et Astroparticules |
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| 2 : | LAPTH - Laboratoire d'Annecy-le-Vieux de Physique Théorique |
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| Domaine | : | Physique/Astrophysique/Phénomènes cosmiques de haute energie Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie Physique/Physique des Hautes Energies - Phénoménologie |
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| Lien vers le texte intégral : |
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| http://fr.arXiv.org/abs/1205.1004 |
| hal-00707457, version 1 | |
| http://hal.archives-ouvertes.fr/hal-00707457 | |
| oai:hal.archives-ouvertes.fr:hal-00707457 | |
| Contributeur : Virginie Malaval | |
| Soumis le : Mardi 12 Juin 2012, 16:27:26 | |
| Dernière modification le : Mardi 12 Juin 2012, 16:27:26 | |
