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arXiv · 2407.05753

Relic Abundance of Dark Matter with $\Delta$(54) Flavor Symmetry

Hrishi Bora·Ng. K. Francis·Shawan Kumar Jha
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Abstract

In this work we discuss the neutrino phenomenology in a $\Delta(54)$ discrete flavor symmetry and evaluate the relic abundance of dark matter (DM) and active neutrino-DM mixing angle considering various cosmological constraints. We introduced two Standard Model Higgs particles along with vector-like fermions and a new particle (S) which is a gauge singlet in the Standard Model. This modification leads to a mass matrix that diverges from the tribimaximal neutrino mixing pattern resulting in a non-zero reactor angle ($\theta_{13}$). We also incorporated a $ Z_2 \otimes Z_3 \otimes Z_4$ symmetry for the specific interactions in our model. The additional particle S is a sterile neutrino which is considered to be a probable dark matter candidate with mass in keV range.

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Hrishi Bora, Ng. K. Francis, Shawan Kumar Jha. 2024-07-08. Relic Abundance of Dark Matter with $\Delta$(54) Flavor Symmetry. https://arxiv.org/abs/2407.05753

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