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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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Lenguaje: | eng |
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2008
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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. |
id | cern-1094678 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2008 |
record_format | invenio |
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 AT gondolopaolo ultracoldwimpsrelicsofnonstandardprebbncosmologies |