Confinement of Cosmic Rays in Dark Matter clumps

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dc.creatorde Boer, W.
dc.creatorZhukov, V.
dc.date2007-09-28
dc.date.accessioned2026-07-07T08:32:52Z
dc.date.available2026-07-07T08:32:52Z
dc.descriptionSome part of the relic Dark Matter is distributed in small-scale clumps which survived structure formation in inflation cosmological scenario. The annihilation of DM inside these clumps is a strong source of stable charged particles which can have a substantial density near the clump core. The streaming of the annihilation products from the clump can enhance irregularities in the galactic magnetic field. This can produce small scale variations in diffusion coefficient affecting propagation of Cosmic Rays.
dc.descriptionContribution to the 30 ICRC, July 2007, Merida, Mexico
dc.identifierhttps://arxiv.org/abs/0709.4576
dc.identifierhttp://arxiv.org/abs/0709.4576
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/138935
dc.subjectAstrophysics
dc.titleConfinement of Cosmic Rays in Dark Matter clumps
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