# Fermionic triplet dark matter in an $SO(10)$-inspired left right model

**Authors:** Carolina Arbel\'aez, Martin Hirsch, Diego Restrepo

arXiv: 1703.08148 · 2017-06-07

## TL;DR

This paper investigates fermionic triplet dark matter within an $SO(10)$-inspired left-right model, exploring scenarios that achieve gauge unification and satisfy relic density and detection constraints.

## Contribution

It introduces two novel fermionic triplet dark matter scenarios compatible with gauge unification and phenomenological constraints in a left-right symmetric framework.

## Key findings

- One scenario's dark matter is nearly unconstrained by current direct detection.
- The second scenario's detection constraints are comparable to collider limits.
- Both scenarios can achieve gauge coupling unification within an $SO(10)$ framework.

## Abstract

We study a left right (LR) extension of the Standard Model (SM) where the Dark Matter (DM) candidate is composed of a set of fermionic Majorana triplets. The DM is stabilized by a remnant $Z_{2}$ symmetry from the breaking of the LR group to the SM. Two simple scenarios where the DM particles plus a certain set of extra fields lead to gauge coupling unification with a low LR scale are explored. The constraints from relic density and predictions for direct detection are discussed for both scenarios. The first scenario with a $SU(2)_R$ vectorlike fermion triplet contains a DM candidate which is almost unconstrained by current direct detection experiments. The second scenario, with an additional $SU(2)_R$ triplet, opens up a scalar portal leading to direct detection constraints which are similar to collider limits for right gauge bosons. The DM parameter space consistent with phenomenological requirements can also lead to successful gauge coupling unification in a $SO(10)$ setup.

## Full text

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## Figures

17 figures with captions in the complete paper: https://tomesphere.com/paper/1703.08148/full.md

## References

47 references — full list in the complete paper: https://tomesphere.com/paper/1703.08148/full.md

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Source: https://tomesphere.com/paper/1703.08148