Dark Matter production from relativistic bubble walls
Abstract In this paper we present a novel mechanism for producing the observed Dark Matter (DM) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show that the bubble expansion with ultra-relativistic velocities can lead to the abundance of DM particles with ma...
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Online Access: | https://doi.org/10.1007/JHEP03(2021)288 |
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doaj-c4a8b74dfb2641b2af6ad5d467015c0d2021-04-04T11:07:06ZengSpringerOpenJournal of High Energy Physics1029-84792021-03-012021313110.1007/JHEP03(2021)288Dark Matter production from relativistic bubble wallsAleksandr Azatov0Miguel Vanvlasselaer1Wen Yin2SISSA International School for Advanced StudiesSISSA International School for Advanced StudiesDepartment of Physics, The University of TokyoAbstract In this paper we present a novel mechanism for producing the observed Dark Matter (DM) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show that the bubble expansion with ultra-relativistic velocities can lead to the abundance of DM particles with masses much larger than the scale of the transition. We study this non-thermal production mechanism in the context of a generic phase transition and the electroweak phase transition. The application of the mechanism to the Higgs portal DM as well as the signal in the Stochastic Gravitational Background are discussed.https://doi.org/10.1007/JHEP03(2021)288Cosmology of Theories beyond the SMSpontaneous Symmetry BreakingBeyond Standard ModelThermal Field Theory |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Aleksandr Azatov Miguel Vanvlasselaer Wen Yin |
spellingShingle |
Aleksandr Azatov Miguel Vanvlasselaer Wen Yin Dark Matter production from relativistic bubble walls Journal of High Energy Physics Cosmology of Theories beyond the SM Spontaneous Symmetry Breaking Beyond Standard Model Thermal Field Theory |
author_facet |
Aleksandr Azatov Miguel Vanvlasselaer Wen Yin |
author_sort |
Aleksandr Azatov |
title |
Dark Matter production from relativistic bubble walls |
title_short |
Dark Matter production from relativistic bubble walls |
title_full |
Dark Matter production from relativistic bubble walls |
title_fullStr |
Dark Matter production from relativistic bubble walls |
title_full_unstemmed |
Dark Matter production from relativistic bubble walls |
title_sort |
dark matter production from relativistic bubble walls |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2021-03-01 |
description |
Abstract In this paper we present a novel mechanism for producing the observed Dark Matter (DM) relic abundance during the First Order Phase Transition (FOPT) in the early universe. We show that the bubble expansion with ultra-relativistic velocities can lead to the abundance of DM particles with masses much larger than the scale of the transition. We study this non-thermal production mechanism in the context of a generic phase transition and the electroweak phase transition. The application of the mechanism to the Higgs portal DM as well as the signal in the Stochastic Gravitational Background are discussed. |
topic |
Cosmology of Theories beyond the SM Spontaneous Symmetry Breaking Beyond Standard Model Thermal Field Theory |
url |
https://doi.org/10.1007/JHEP03(2021)288 |
work_keys_str_mv |
AT aleksandrazatov darkmatterproductionfromrelativisticbubblewalls AT miguelvanvlasselaer darkmatterproductionfromrelativisticbubblewalls AT wenyin darkmatterproductionfromrelativisticbubblewalls |
_version_ |
1721543133675651072 |