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Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies

Weakly interacting massive particles (WIMPs) constitute one of very few probes of cosmology before big bang nucleosynthesis (BBN). We point out that in scenarios in which the Universe evolves in a non-standard manner during and after WIMP kinetic decoupling, the horizon mass scale at decoupling can...

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Detalles Bibliográficos
Autores principales: Gelmini, Graciela B., Gondolo, Paolo
Lenguaje:eng
Publicado: 2008
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2008/10/002
http://cds.cern.ch/record/1094678
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author Gelmini, Graciela B.
Gondolo, Paolo
author_facet Gelmini, Graciela B.
Gondolo, Paolo
author_sort Gelmini, Graciela B.
collection CERN
description Weakly interacting massive particles (WIMPs) constitute one of very few probes of cosmology before big bang nucleosynthesis (BBN). We point out that in scenarios in which the Universe evolves in a non-standard manner during and after WIMP kinetic decoupling, the horizon mass scale at decoupling can be smaller and the dark matter WIMPs can be colder than in standard cosmology. This would lead to much smaller first objects in hierarchical structure formation. In low reheating temperature scenarios the effect may be large enough to noticeably enhance indirect detection signals in GLAST and other detectors, by up to two orders of magnitude.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2008
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spelling cern-10946782023-03-14T19:02:17Zdoi:10.1088/1475-7516/2008/10/002http://cds.cern.ch/record/1094678engGelmini, Graciela B.Gondolo, PaoloUltra-cold WIMPs: relics of non-standard pre-BBN cosmologiesAstrophysics and AstronomyWeakly interacting massive particles (WIMPs) constitute one of very few probes of cosmology before big bang nucleosynthesis (BBN). We point out that in scenarios in which the Universe evolves in a non-standard manner during and after WIMP kinetic decoupling, the horizon mass scale at decoupling can be smaller and the dark matter WIMPs can be colder than in standard cosmology. This would lead to much smaller first objects in hierarchical structure formation. In low reheating temperature scenarios the effect may be large enough to noticeably enhance indirect detection signals in GLAST and other detectors, by up to two orders of magnitude.We point out that in scenarios in which the Universe evolves in a non-standard manner during and after the kinetic decoupling of weakly interacting massive particles (WIMPs), these relics can be much colder than in standard cosmological scenarios (i.e. can be ultra-cold), possibly leading to the formation of smaller first objects in hierarchical structure formation scenarios.arXiv:0803.2349CERN-PH-TH-2008-052CERN-PH-TH-2008-052oai:cds.cern.ch:10946782008
spellingShingle Astrophysics and Astronomy
Gelmini, Graciela B.
Gondolo, Paolo
Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies
title Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies
title_full Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies
title_fullStr Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies
title_full_unstemmed Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies
title_short Ultra-cold WIMPs: relics of non-standard pre-BBN cosmologies
title_sort ultra-cold wimps: relics of non-standard pre-bbn cosmologies
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1088/1475-7516/2008/10/002
http://cds.cern.ch/record/1094678
work_keys_str_mv AT gelminigracielab ultracoldwimpsrelicsofnonstandardprebbncosmologies
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