Dark matter bound to the Solar System: consequences for annihilation searches

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dc.creatorPeter, Annika H. G.
dc.date2009-05-15
dc.date.accessioned2026-07-07T13:15:51Z
dc.date.available2026-07-07T13:15:51Z
dc.descriptionOne method to search for particle dark matter is to hunt down its annihilation products. In the Solar System, three potential types of signals of annihilation have been identified: neutrinos and gamma-rays from the Sun, and neutrinos from the Earth. Each of these signals depends sensitively on the orbital evolution of dark matter once it becomes bound to the Solar System. I will review progress on characterizing these signals based on recent improvements in the determination of the properties of the bound dark matter population.
dc.description8 pages, 4 figures, invited talk at XLIV Rencontres de Moriond: Electroweak Interactions and Unified Theories, La Thuile, March 7-14, 2009
dc.identifierhttps://arxiv.org/abs/0905.2456
dc.identifierhttp://arxiv.org/abs/0905.2456
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/230602
dc.subjectHigh Energy Astrophysical Phenomena
dc.subjectHigh Energy Physics - Experiment
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDark matter bound to the Solar System: consequences for annihilation searches
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