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dc.contributor.authorBringmann, Torsten
dc.contributor.authorDepta, Paul Frederik
dc.contributor.authorHufnagel, Marco
dc.contributor.authorKersten, Jörn
dc.contributor.authorRuderman, Joshua T.
dc.contributor.authorSchmidt-Hoberg, Kai
dc.date.accessioned2024-03-12T09:18:03Z
dc.date.available2024-03-12T09:18:03Z
dc.date.created2023-06-13T09:26:56Z
dc.date.issued2023
dc.identifier.issn2470-0010
dc.identifier.urihttps://hdl.handle.net/11250/3121900
dc.description.abstractWe propose a novel mechanism to generate sterile neutrinos νs in the early Universe, by converting ordinary neutrinos να in scattering processes νsνα→νsνs. After initial production by oscillations, this leads to an exponential growth in the νs abundance. We show that such a production regime naturally occurs for self-interacting νs, and that this opens up significant new parameter space where νs make up all of the observed dark matter. Our results provide strong motivation to further push the sensitivity of X-ray line searches, and to improve on constraints from structure formation.en_US
dc.language.isoengen_US
dc.publisherAPSen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.titleMinimal sterile neutrino dark matteren_US
dc.typeJournal articleen_US
dc.typePeer revieweden_US
dc.description.versionpublishedVersionen_US
dc.source.articlenumberL071702en_US
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.doi10.1103/PhysRevD.107.L071702
dc.identifier.cristin2153984
dc.source.journalPhysical Review Den_US
dc.identifier.citationPhysical Review D. 2023, 107 (7), L071702.en_US
dc.source.volume107en_US
dc.source.issue7en_US


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