Neutrino dark matter and the Higgs portal: improved freeze-in analysis

Abstract Sterile neutrinos are one of the leading dark matter candidates. Their masses may originate from a vacuum expectation value of a scalar field. If the sterile neutrino couplings are very small and their direct coupling to the inflaton is forbidden by the lepton number symmetry, the leading d...

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Main Authors: Valentina De Romeri, Dimitrios Karamitros, Oleg Lebedev, Takashi Toma
Format: Article
Language:English
Published: SpringerOpen 2020-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP10(2020)137
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spelling doaj-80d90bda80324db0a32d3469f06b143e2020-11-25T03:59:13ZengSpringerOpenJournal of High Energy Physics1029-84792020-10-0120201014110.1007/JHEP10(2020)137Neutrino dark matter and the Higgs portal: improved freeze-in analysisValentina De Romeri0Dimitrios Karamitros1Oleg Lebedev2Takashi Toma3Institut de Física Corpuscular CSIC/Universitat de València, Parc Científic de PaternaNational Centre for Nuclear ResearchDepartment of Physics, University of HelsinkiDepartment of Physics, McGill UniversityAbstract Sterile neutrinos are one of the leading dark matter candidates. Their masses may originate from a vacuum expectation value of a scalar field. If the sterile neutrino couplings are very small and their direct coupling to the inflaton is forbidden by the lepton number symmetry, the leading dark matter production mechanism is the freeze-in scenario. We study this possibility in the neutrino mass range up to 1 GeV, taking into account relativistic production rates based on the Bose-Einstein statistics, thermal masses and phase transition effects. The specifics of the production mechanism and the dominant mode depend on the relation between the scalar and sterile neutrino masses as well as on whether or not the scalar is thermalized. We find that the observed dark matter abundance can be produced in all of the cases considered. We also revisit the freeze-in production of a Higgs portal scalar, pointing out the importance of a fusion mode, as well as the thermalization constraints.http://link.springer.com/article/10.1007/JHEP10(2020)137Beyond Standard ModelCosmology of Theories beyond the SM
collection DOAJ
language English
format Article
sources DOAJ
author Valentina De Romeri
Dimitrios Karamitros
Oleg Lebedev
Takashi Toma
spellingShingle Valentina De Romeri
Dimitrios Karamitros
Oleg Lebedev
Takashi Toma
Neutrino dark matter and the Higgs portal: improved freeze-in analysis
Journal of High Energy Physics
Beyond Standard Model
Cosmology of Theories beyond the SM
author_facet Valentina De Romeri
Dimitrios Karamitros
Oleg Lebedev
Takashi Toma
author_sort Valentina De Romeri
title Neutrino dark matter and the Higgs portal: improved freeze-in analysis
title_short Neutrino dark matter and the Higgs portal: improved freeze-in analysis
title_full Neutrino dark matter and the Higgs portal: improved freeze-in analysis
title_fullStr Neutrino dark matter and the Higgs portal: improved freeze-in analysis
title_full_unstemmed Neutrino dark matter and the Higgs portal: improved freeze-in analysis
title_sort neutrino dark matter and the higgs portal: improved freeze-in analysis
publisher SpringerOpen
series Journal of High Energy Physics
issn 1029-8479
publishDate 2020-10-01
description Abstract Sterile neutrinos are one of the leading dark matter candidates. Their masses may originate from a vacuum expectation value of a scalar field. If the sterile neutrino couplings are very small and their direct coupling to the inflaton is forbidden by the lepton number symmetry, the leading dark matter production mechanism is the freeze-in scenario. We study this possibility in the neutrino mass range up to 1 GeV, taking into account relativistic production rates based on the Bose-Einstein statistics, thermal masses and phase transition effects. The specifics of the production mechanism and the dominant mode depend on the relation between the scalar and sterile neutrino masses as well as on whether or not the scalar is thermalized. We find that the observed dark matter abundance can be produced in all of the cases considered. We also revisit the freeze-in production of a Higgs portal scalar, pointing out the importance of a fusion mode, as well as the thermalization constraints.
topic Beyond Standard Model
Cosmology of Theories beyond the SM
url http://link.springer.com/article/10.1007/JHEP10(2020)137
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AT dimitrioskaramitros neutrinodarkmatterandthehiggsportalimprovedfreezeinanalysis
AT oleglebedev neutrinodarkmatterandthehiggsportalimprovedfreezeinanalysis
AT takashitoma neutrinodarkmatterandthehiggsportalimprovedfreezeinanalysis
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