The Inflaton Field as Self-Interacting Dark Matter in the Braneworld Scenario

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dc.creatorLidsey, James E.
dc.creatorMatos, Tonatiuh
dc.creatorUrena-Lopez, L. Arturo
dc.date2001-11-14
dc.date2002-04-23
dc.date.accessioned2026-07-07T11:28:50Z
dc.date.available2026-07-07T11:28:50Z
dc.descriptionA unified model is developed within the context of the braneworld paradigm, where a single scalar field can act as both the inflaton field in the very early universe and also as strong, self-interacting dark matter in the post-inflationary universe. Reheating proceeds due to the overproduction and subsequent evaporation of primordial black holes. Observational constraints, most notably from gravitational waves, are satisfied if the probability of PBH formation is sufficiently high.
dc.description5 pages, no figures. Minor changes and references added. To appear in PRD
dc.identifierhttps://arxiv.org/abs/astro-ph/0111292
dc.identifierhttp://arxiv.org/abs/astro-ph/0111292
dc.identifierPhys.Rev.D66:023514,2002
dc.identifierdoi:10.1103/PhysRevD.66.023514
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196523
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleThe Inflaton Field as Self-Interacting Dark Matter in the Braneworld Scenario
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