# Mitigating Direct Detection Bounds in Non-minimal Higgs Portal Scalar   Dark Matter Models

**Authors:** Subhaditya Bhattacharya, Purusottam Ghosh, Tarak Nath Maity, Tirtha, Sankar Ray

arXiv: 1706.04699 · 2017-10-25

## TL;DR

This paper explores non-minimal Higgs portal scalar dark matter models with extended symmetries, demonstrating they can evade current direct detection bounds while still explaining observed dark matter relic density.

## Contribution

It systematically studies how enlarging the stabilizing symmetry and including multipartite features relaxes direct detection constraints in scalar dark matter models.

## Key findings

- Non-minimal models relax direct detection constraints.
- Resonant semi-annihilation opens new parameter space.
- Multi-component frameworks illustrate complex dark matter interactions.

## Abstract

Minimal scalar Higgs portal dark matter model is increasingly in tension with recent results form direct detection experiments like LUX and XENON. In this paper we make a systematic study of minimal extension of the $ \mathbb{Z}_2$ stabilised singlet scalar Higgs portal scenario in terms of their prospects at direct detection experiments. We consider both enlarging the stabilising symmetry to $\mathbb{Z}_3$ and incorporating multipartite features in the dark sector. We demonstrate that in these non-minimal models the interplay of annihilation, co-annihilation and semi-annihilation processes considerably relax constraints from present and proposed direct detection experiments while simultaneously saturating observed dark matter relic density. We explore in particular the resonant semi-annihilation channel within the multipartite $\mathbb{Z}_3$ framework which results in new unexplored regions of parameter space that would be difficult to constrain by direct detection experiments in the near future. The role of dark matter exchange processes within multi-component $\mathbb{Z}_3 \times \mathbb{Z}_3'$ framework is illustrated. We make quantitative estimates to elucidate the role of the various annihilation processes in the different allowed regions of parameter space of these models.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1706.04699/full.md

## Figures

40 figures with captions in the complete paper: https://tomesphere.com/paper/1706.04699/full.md

## References

61 references — full list in the complete paper: https://tomesphere.com/paper/1706.04699/full.md

---
Source: https://tomesphere.com/paper/1706.04699