Dark matter in the fully flipped 3-3-1-1 model

TL;DR

This paper explores a specific particle physics model, the fully flipped 3-3-1-1, which naturally provides dark matter candidates and analyzes their viability based on relic density and detection constraints.

Contribution

It introduces the fully flipped 3-3-1-1 model and identifies dark matter candidates within it, analyzing their parameter space and experimental constraints.

Findings

Dark matter candidates are naturally generated in the model.

Viable parameter regions are constrained by relic density data.

Direct detection experiments further restrict the model's parameter space.

Abstract

We present the features of the fully flipped 3-3-1-1 model and show that this model leads to dark matter candidates naturally. We study two dark matter scenarios corresponding to the triplet fermion and singlet scalar candidates, and we determine the viable parameter regimes constrained from the observed relic density and direct detection experiments.