# MeV scale model of SIMP dark matter, neutrino mass and leptogenesis

**Authors:** Subhendra Mohanty, Ayon Patra, Tripurari Srivastava

arXiv: 1908.00909 · 2020-03-18

## TL;DR

This paper proposes a minimal extension of the Standard Model introducing scalar fields and right-handed neutrinos to explain MeV-scale dark matter, neutrino masses, and baryogenesis via leptogenesis.

## Contribution

It introduces a simple model with scalar fields and right-handed neutrinos that simultaneously addresses dark matter stability, neutrino mass generation, and leptogenesis.

## Key findings

- Scalar field serves as stable MeV-scale dark matter.
- Model successfully explains neutrino masses via Type-I seesaw.
- Leptogenesis mechanism generates observed baryon asymmetry.

## Abstract

We consider a simple extension of the Standard Model with two singlet scalar fields and three heavy right-handed neutrinos. One of the scalar fields serves as an MeV scale dark matter and its stability is ensured by the introduction of an extra $Z_2$ symmetry. The second scalar (which is even under the $Z_2$ symmetry) generates the mass term of the scalar, contributes to the $3 \rightarrow 2$ annihilation process required for the correct relic density of the dark matter and it also contributes to the leptogenesis. The right-handed neutrinos are responsible for the generation of light neutrino masses through Type-I seesaw mechanism. The decay of the heavy right-handed neutrino can generate the lepton asymmetry which can then be converted to baryon asymmetry through sphaleron transitions.

## Full text

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## Figures

23 figures with captions in the complete paper: https://tomesphere.com/paper/1908.00909/full.md

## References

73 references — full list in the complete paper: https://tomesphere.com/paper/1908.00909/full.md

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Source: https://tomesphere.com/paper/1908.00909