2009/05/15 by Annika H. G. Peter, Peter, Annika H. G. · 1 citation
Physics and Astronomy · #Atomic and Subatomic Physics Research #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Experiment (hep-ex) #High Energy Physics - Phenomenology (hep-ph) #Quantum Mechanics and Applications #astro-ph.HE #hep-ex #hep-ph
paper · pdf · doi:10.48550/arxiv.0905.2456
8 pages, 4 figures, invited talk at XLIV Rencontres de Moriond: Electroweak Interactions and Unified Theories, La Thuile, March 7-14, 2009
arxiv created 2009/05/15 · openalex publication_date 2009/05/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
One 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.