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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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 |
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DataCite Metadata Store (German National Library of Science and Technology) |
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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 |
_version_ |
1766201533805887488 |