A TeV scale model for neutrino mass, dark matter and baryon asymmetry
Mayumi Aoki, Shinya Kanemura, Osamu Seto

TL;DR
This paper proposes a TeV-scale model that simultaneously explains neutrino oscillations, dark matter, and baryon asymmetry through an extended Higgs sector and right-handed neutrinos, with testable predictions.
Contribution
It introduces a novel TeV-scale model with an exact Z2 symmetry that accounts for neutrino masses, dark matter, and baryogenesis in a unified framework.
Findings
Neutrino masses generated at three-loop level
Singlet scalar as dark matter candidate
Strong first-order phase transition for baryogenesis
Abstract
We discuss a TeV scale model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the dynamics of the extended Higgs sector and TeV-scale right-handed neutrinos with imposed an exact symmetry. Tiny neutrino masses are generated at the three loop level, a singlet scalar field is a candidate of dark matter, and a strong first order phase transition is realized for successful electroweak baryogenesis. The model provides various discriminative predictions, so that it is testable at the current and future experiments.
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Taxonomy
TopicsComputational Physics and Python Applications · Particle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena
