Non-thermal WIMPs as Dark Radiation

It has been thought that only light species could behave as radiation and account for the dark radiation observed recently by Planck, WMAP9, South Pole and ATACAMA telescopes. In this work we will show that GeV scale WIMPs can plausibly account for the dark radiation as well. Heavy WIMPs might mimic...

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Main Author: Queiroz, Farinaldo S.
Format: Text
Language:unknown
Published: arXiv 2013
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.1310.3026
https://arxiv.org/abs/1310.3026
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spelling ftdatacite:10.48550/arxiv.1310.3026 2023-05-15T18:22:10+02:00 Non-thermal WIMPs as Dark Radiation Queiroz, Farinaldo S. 2013 https://dx.doi.org/10.48550/arxiv.1310.3026 https://arxiv.org/abs/1310.3026 unknown arXiv https://dx.doi.org/10.1063/1.4883415 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Cosmology and Nongalactic Astrophysics astro-ph.CO High Energy Physics - Phenomenology hep-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2013 ftdatacite https://doi.org/10.48550/arxiv.1310.3026 https://doi.org/10.1063/1.4883415 2022-04-01T17:28:00Z It has been thought that only light species could behave as radiation and account for the dark radiation observed recently by Planck, WMAP9, South Pole and ATACAMA telescopes. In this work we will show that GeV scale WIMPs can plausibly account for the dark radiation as well. Heavy WIMPs might mimic the effect of a half neutrino species if some of their fraction were produced non-thermally after the thermal freeze-out. In addition, we will show how BBN, CMB and Structure Formation bounds might be circumvented. : 8 Pages, 2 Figures. Published in the PPC proceedings 2013 Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Cosmology and Nongalactic Astrophysics astro-ph.CO
High Energy Physics - Phenomenology hep-ph
FOS Physical sciences
spellingShingle Cosmology and Nongalactic Astrophysics astro-ph.CO
High Energy Physics - Phenomenology hep-ph
FOS Physical sciences
Queiroz, Farinaldo S.
Non-thermal WIMPs as Dark Radiation
topic_facet Cosmology and Nongalactic Astrophysics astro-ph.CO
High Energy Physics - Phenomenology hep-ph
FOS Physical sciences
description It has been thought that only light species could behave as radiation and account for the dark radiation observed recently by Planck, WMAP9, South Pole and ATACAMA telescopes. In this work we will show that GeV scale WIMPs can plausibly account for the dark radiation as well. Heavy WIMPs might mimic the effect of a half neutrino species if some of their fraction were produced non-thermally after the thermal freeze-out. In addition, we will show how BBN, CMB and Structure Formation bounds might be circumvented. : 8 Pages, 2 Figures. Published in the PPC proceedings 2013
format Text
author Queiroz, Farinaldo S.
author_facet Queiroz, Farinaldo S.
author_sort Queiroz, Farinaldo S.
title Non-thermal WIMPs as Dark Radiation
title_short Non-thermal WIMPs as Dark Radiation
title_full Non-thermal WIMPs as Dark Radiation
title_fullStr Non-thermal WIMPs as Dark Radiation
title_full_unstemmed Non-thermal WIMPs as Dark Radiation
title_sort non-thermal wimps as dark radiation
publisher arXiv
publishDate 2013
url https://dx.doi.org/10.48550/arxiv.1310.3026
https://arxiv.org/abs/1310.3026
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1063/1.4883415
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1310.3026
https://doi.org/10.1063/1.4883415
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