Asymmetric dark matter models in SO(10)
From MaRDI portal
Publication:5024129
DOI10.1088/1475-7516/2017/02/016OpenAlexW2593339496MaRDI QIDQ5024129
Keith A. Olive, Natsumi Nagata, Jia-Ming Zheng
Publication date: 28 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1611.04693
Related Items (2)
Direct neutralino searches in the NMSSM with gravitino LSP in the degenerate scenario ⋮ Gravitino dark matter in the constrained next-to-minimal supersymmetric standard model with neutralino next-to-lightest superpartner
Cites Work
- Leptogenesis as a common origin for matter and dark matter
- Asymmetric dark matter from leptogenesis
- Emergent dark matter, baryon, and lepton numbers
- Minimal dark matter and leptogenesis
- Asymmetric dark matter: theories, signatures, and constraints
- Asymmetric inelastic inert doublet dark matter from triplet scalar leptogenesis
- Dark matter from the vector of \(\mathrm{SO}(10)\)
- Weakly-interacting massive particles in non-supersymmetric \(\mathrm{SO}(10)\) grand unified models
- Neutrino Mass and Spontaneous Parity Nonconservation
- On relating the genesis of cosmic baryons and dark matter
This page was built for publication: Asymmetric dark matter models in SO(10)