A further look at particle annihilation in dark matter caustics

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dc.creatorNatarajan, Aravind
dc.creatorSikivie, Pierre
dc.date2007-11-08
dc.date2008-01-28
dc.date.accessioned2026-07-07T12:13:52Z
dc.date.available2026-07-07T12:13:52Z
dc.descriptionDark matter caustics are small scale, high density structures believed to exist in galaxies like ours. If the dark matter consists of Weakly Interacting Massive Particles, these caustics may be detected by means of the gamma rays produced by dark matter particle annihilation. We discuss particle annihilation in outer and inner caustics and provide sky maps of the expected gamma ray distribution.
dc.descriptionMinor changes, Introduction expanded, references added, accepted for publication in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/0711.1297
dc.identifierhttp://arxiv.org/abs/0711.1297
dc.identifierPhys.Rev.D77:043531,2008
dc.identifierdoi:10.1103/PhysRevD.77.043531
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/210998
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleA further look at particle annihilation in dark matter caustics
dc.typetext

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