Skip to content
DraconiticResearch
Search Sources API
197,693 studies31 sourcesUpdated 37 min ago
Peer-reviewedCC BY 4.0The European Physical Journal C

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

  1. 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.

Related

  1. Majorana Neutrino Physics and Matter-Antimatter Asymmetry in Type IIA String Theory
    Yang Liu
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXiv
  2. Distinguishing the origin of cosmic birefringence: dark energy, dark matter, and neutrino asymmetry
    Lu Yin, Eiichiro Komatsu
    arXivPreprintCC BY 4.0Full textCosmologyHigh-energy astrophysicsarXiv
  3. Natural Saturation Of The Sterile Neutrino Dark Matter Resonant Production By a High Lepton Flavor Asymmetry In Primordial Plasma
    Dmitry Gorbunov, Dmitry Kalashnikov
    arXivPreprintCC BY 4.0Full textCosmologyHigh-energy & particle physicsarXiv
  4. Generation-separated hypercharges and dark charges: origin of flavor, neutrino masses, and dark matter
    Duong Van Loi
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXiv
  5. A massive right-handed sterile neutrino in three-body B̅→ D*ℓ-N̅R decays - a Monte Carlo simulation study
    Bhubanjyoti Bhattacharya, Thomas E Browder, Lucien M Cremaldi +6
    HALPreprintarXiv licenceFull textHigh-energy & particle physicsHALarXiv
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  -