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Right-handed neutrino dark matter consistent with the generation of baryon number asymmetry

Daijiro Suematsu iD

DOI10.1140/epjc/s10052-026-16425-1
PublisherSpringer Science and Business Media LLC
Journal / SourceThe European Physical Journal C
Published2026-10
Metadata Deposited2026-10-07 (updated: 2026-10-07)
Subject—
Languageen
ISSN1434-6044, 1434-6052
Typejournal-article
Volume / Issue / Pages86 / 10 / —
Citations0
References deposited66
Access / license metadataOpen license identified License 1 ↗A reuse license does not by itself establish whether the full text is freely readable.

Abstract

Abstract A right-handed neutrino is a promising candidate for dark matter (DM) which has no interaction with nuclei. Since two right-handed neutrinos explain neutrino oscillation data and baryon number asymmetry through both the seesaw mechanism and leptogenesis based on the out-of-equilibrium decay of the lighter one, the lightest third right-handed neutrino could be free from them and stable to be DM. It suggests a possibility that the right-handed neutrinos could be common key particles for the explanation of three problems in the standard model (SM). We study this possibility by analyzing the structure of a neutrino mass matrix in the scotogenic model for neutrino mass.