Leptogenesis in fast expanding Universe
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Publication:5068405
DOI10.1088/1475-7516/2020/03/009zbMath1490.83074arXiv1912.07185OpenAlexW3099055703MaRDI QIDQ5068405
Amit Dutta Banik, Shao-Long Chen, Ze-Kun Liu
Publication date: 6 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1912.07185
Unified quantum theories (81V22) Nuclear physics (81V35) Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Weak interaction in quantum theory (81V15) Galactic and stellar structure (85A15)
Related Items (3)
FIMP Dark Matter from Leptogenesis in Fast Expanding Universe ⋮ Baryon asymmetry and lower bound on right handed neutrino mass in fast expanding Universe: an analytical approach ⋮ WIMPs during reheating
Cites Work
- Leptogenesis as a common origin for matter and dark matter
- Asymmetric dark matter from leptogenesis
- Leptogenesis for pedestrians
- Dark matter assisted Dirac leptogenesis and neutrino mass
- Stability, reheating, and leptogenesis
- Relic Density of Asymmetric Dark Matter in Modified Cosmological Scenarios
- Flavor effects in leptogenesis
- Neutrino Mass and Spontaneous Parity Nonconservation
- Establishing the dark matter relic density in an era of particle decays
- Fermion dark matter with N2 leptogenesis in minimal scotogenic model
- Oscillating neutrinos and \(\mu\rightarrow e,\gamma\)
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