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Light dark photon dark matter from inflation
We discuss the possibility of producing a light dark photon dark matter through a coupling between the dark photon field and the inflaton. The dark photon with a large wavelength is efficiently produced due to the inflaton motion during inflation and becomes non-relativistic before the time of matte...
Autores principales: | , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Berlin Heidelberg
2020
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7768992/ https://www.ncbi.nlm.nih.gov/pubmed/33390726 http://dx.doi.org/10.1007/JHEP12(2020)170 |
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author | Nakai, Yuichiro Namba, Ryo Wang, Ziwei |
author_facet | Nakai, Yuichiro Namba, Ryo Wang, Ziwei |
author_sort | Nakai, Yuichiro |
collection | PubMed |
description | We discuss the possibility of producing a light dark photon dark matter through a coupling between the dark photon field and the inflaton. The dark photon with a large wavelength is efficiently produced due to the inflaton motion during inflation and becomes non-relativistic before the time of matter-radiation equality. We compute the amount of production analytically. The correct relic abundance is realized with a dark photon mass extending down to 10(−21) eV. |
format | Online Article Text |
id | pubmed-7768992 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2020 |
publisher | Springer Berlin Heidelberg |
record_format | MEDLINE/PubMed |
spelling | pubmed-77689922020-12-28 Light dark photon dark matter from inflation Nakai, Yuichiro Namba, Ryo Wang, Ziwei J High Energy Phys Regular Article - Theoretical Physics We discuss the possibility of producing a light dark photon dark matter through a coupling between the dark photon field and the inflaton. The dark photon with a large wavelength is efficiently produced due to the inflaton motion during inflation and becomes non-relativistic before the time of matter-radiation equality. We compute the amount of production analytically. The correct relic abundance is realized with a dark photon mass extending down to 10(−21) eV. Springer Berlin Heidelberg 2020-12-28 2020 /pmc/articles/PMC7768992/ /pubmed/33390726 http://dx.doi.org/10.1007/JHEP12(2020)170 Text en © The Author(s) 2020 https://creativecommons.org/licenses/by/4.0/Open Access. This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0 (https://creativecommons.org/licenses/by/4.0/) ), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited. |
spellingShingle | Regular Article - Theoretical Physics Nakai, Yuichiro Namba, Ryo Wang, Ziwei Light dark photon dark matter from inflation |
title | Light dark photon dark matter from inflation |
title_full | Light dark photon dark matter from inflation |
title_fullStr | Light dark photon dark matter from inflation |
title_full_unstemmed | Light dark photon dark matter from inflation |
title_short | Light dark photon dark matter from inflation |
title_sort | light dark photon dark matter from inflation |
topic | Regular Article - Theoretical Physics |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7768992/ https://www.ncbi.nlm.nih.gov/pubmed/33390726 http://dx.doi.org/10.1007/JHEP12(2020)170 |
work_keys_str_mv | AT nakaiyuichiro lightdarkphotondarkmatterfrominflation AT nambaryo lightdarkphotondarkmatterfrominflation AT wangziwei lightdarkphotondarkmatterfrominflation |