Dark matter indirect signatures

Julien Lavalle; Pierre Salati

doi:10.1016/j.crhy.2012.05.001

Dark matter indirect signatures
[Signatures indirectes des particules de matière noire]

Julien Lavalle ¹ ; Pierre Salati ²

¹ Laboratoire univers & particules de Montpellier (LUPM), CNRS-IN2P3 & université Montpellier II (UMR-5299), place Eugène-Bataillon, 34095 Montpellier cedex 05, France
² LAPTh, CNRS & université de Savoie, 9, chemin de Bellevue, B.P. 110, 74941 Annecy-le-Vieux cedex, France

Comptes Rendus. Physique, Volume 13 (2012) no. 6-7, pp. 740-782.

Résumé
Abstract

La matière noire astronomique pourrait être constituée de particules massives aux interactions évanescentes. Si tel était le cas, ces particules se retrouveraient en abondance au sein de la Voie Lactée où elles sʼannihileraient en permanence, produisant de multiples radiations cosmiques. Celles-ci sont éventuellement visibles de la Terre et constituent dès lors des sortes dʼempreintes spectrales, véritables signatures indirectes des candidats potentiels à la matière noire galactique. Dans cet article, nous passons en revue les différentes espèces cosmiques susceptibles dʼêtre produites, et comparons leur flux avec celui des radiations engendrées par les processus astrophysiques conventionnels. Lʼexistence de condensations de matière noire est brièvement discutée. Le taux dʼannihilation pourrait être amplifié au sein de telles structures, conduisant à des signatures indirectes plus intenses que dans le cas dʼun halo galactique lisse.

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.

Publié le : 2012-07-01

DOI : 10.1016/j.crhy.2012.05.001

Keywords: Astronomical dark matter, Cosmic rays, Galactic antimatter, Gamma-rays, Neutrinos
Mot clés : Matière noire astronomique, Rayons cosmiques, Anti-matière galactique, Rayons gamma, Neutrinos

Affiliations des auteurs :

Julien Lavalle ¹ ; Pierre Salati ²

¹ Laboratoire univers & particules de Montpellier (LUPM), CNRS-IN2P3 & université Montpellier II (UMR-5299), place Eugène-Bataillon, 34095 Montpellier cedex 05, France
² LAPTh, CNRS & université de Savoie, 9, chemin de Bellevue, B.P. 110, 74941 Annecy-le-Vieux cedex, France

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     title = {Dark matter indirect signatures},
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Julien Lavalle; Pierre Salati. Dark matter indirect signatures. Comptes Rendus. Physique, Volume 13 (2012) no. 6-7, pp. 740-782. doi : 10.1016/j.crhy.2012.05.001. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2012.05.001/

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