Dark Matter from Early Decays

dc.creatorKaplinghat, Manoj
dc.date2005-07-13
dc.date2005-09-09
dc.date.accessioned2026-07-07T11:24:35Z
dc.date.available2026-07-07T11:24:35Z
dc.descriptionTwo leading dark matter candidates from supersymmetry and other theories of physics beyond the standard model are WIMPs and weak scale gravitinos. If the lightest stable particle is a gravitino, then a WIMP will decay into it with a natural lifetime of order a month ~ M_{pl}^2/M_{weak}^3. We show that if the bulk of dark matter today came from decays of neutral particles with lifetimes of order a year or smaller, then it could lead to a reduction in the amount of small scale substructure, less concentrated halos and constant density cores in the smallest mass halos. Such beneficial effects may therefore be realized naturally, as discussed by Cembranos, Feng, Rajaraman, and Takayama, in the case of supersymmetry.
dc.descriptionMatches version accepted for publication in PRD. Added a paragraph to Sec V. 9 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0507300
dc.identifierhttp://arxiv.org/abs/astro-ph/0507300
dc.identifierPhys.Rev.D72:063510,2005
dc.identifierdoi:10.1103/PhysRevD.72.063510
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195240
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDark Matter from Early Decays
dc.typetext

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