Cosmological constraints on dark scalar

Abstract We discuss cosmological constraints on a dark scalar particle mixing with the Standard Model Higgs boson. We pay particular attention to the dark scalar production process when the reheating temperature of the Universe is very low, which allows us to give a conservative limit on the low-mas...

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Main Authors: Masahiro Ibe, Shin Kobayashi, Yuhei Nakayama, Satoshi Shirai
Format: Article
Language:English
Published: SpringerOpen 2022-03-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP03(2022)198
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author Masahiro Ibe
Shin Kobayashi
Yuhei Nakayama
Satoshi Shirai
author_facet Masahiro Ibe
Shin Kobayashi
Yuhei Nakayama
Satoshi Shirai
author_sort Masahiro Ibe
collection DOAJ
description Abstract We discuss cosmological constraints on a dark scalar particle mixing with the Standard Model Higgs boson. We pay particular attention to the dark scalar production process when the reheating temperature of the Universe is very low, which allows us to give a conservative limit on the low-mass scalar particle. We also study the effect of the self-interaction of the dark scalars and find this has a significant impact on the cosmological constraints. We obtain the most conservative cosmological constraint on the dark scalar, which is complementary to accelerator experiments and astrophysical observations.
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spelling doaj.art-00a4968751c94794b15ef70208afebf82022-12-21T23:33:30ZengSpringerOpenJournal of High Energy Physics1029-84792022-03-012022314010.1007/JHEP03(2022)198Cosmological constraints on dark scalarMasahiro Ibe0Shin Kobayashi1Yuhei Nakayama2Satoshi Shirai3ICRR, The University of TokyoICRR, The University of TokyoICRR, The University of TokyoKavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, The University of TokyoAbstract We discuss cosmological constraints on a dark scalar particle mixing with the Standard Model Higgs boson. We pay particular attention to the dark scalar production process when the reheating temperature of the Universe is very low, which allows us to give a conservative limit on the low-mass scalar particle. We also study the effect of the self-interaction of the dark scalars and find this has a significant impact on the cosmological constraints. We obtain the most conservative cosmological constraint on the dark scalar, which is complementary to accelerator experiments and astrophysical observations.https://doi.org/10.1007/JHEP03(2022)198Cosmology of Theories BSMNew Light Particles
spellingShingle Masahiro Ibe
Shin Kobayashi
Yuhei Nakayama
Satoshi Shirai
Cosmological constraints on dark scalar
Journal of High Energy Physics
Cosmology of Theories BSM
New Light Particles
title Cosmological constraints on dark scalar
title_full Cosmological constraints on dark scalar
title_fullStr Cosmological constraints on dark scalar
title_full_unstemmed Cosmological constraints on dark scalar
title_short Cosmological constraints on dark scalar
title_sort cosmological constraints on dark scalar
topic Cosmology of Theories BSM
New Light Particles
url https://doi.org/10.1007/JHEP03(2022)198
work_keys_str_mv AT masahiroibe cosmologicalconstraintsondarkscalar
AT shinkobayashi cosmologicalconstraintsondarkscalar
AT yuheinakayama cosmologicalconstraintsondarkscalar
AT satoshishirai cosmologicalconstraintsondarkscalar