Peer-reviewedCC BY 4.0The European Physical Journal C
Right-handed neutrino dark matter consistent with the generation of baryon number asymmetry
- 1Kanazawa University
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.
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BibTeX
@article{suematsu2026righthanded,
title = {{Right-handed neutrino dark matter consistent with the generation of baryon number asymmetry}},
author = {Daijiro Suematsu},
journal = {The European Physical Journal C},
year = {2026},
month = oct,
doi = {10.1140/epjc/s10052-026-16425-1},
url = {https://link.springer.com/10.1140/epjc/s10052-026-16425-1},
note = {CC BY 4.0},
}
RIS
TY - JOUR
TI - Right-handed neutrino dark matter consistent with the generation of baryon number asymmetry
AU - Daijiro Suematsu
PY - 2026
DA - 2026/10/07
JO - The European Physical Journal C
DO - 10.1140/epjc/s10052-026-16425-1
UR - https://link.springer.com/10.1140/epjc/s10052-026-16425-1
AB - 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.
SN - 1434-6044
SN - 1434-6052
ER -