# Cornering pseudoscalar-mediated dark matter with the LHC and cosmology

**Authors:** Shankha Banerjee, Daniele Barducci, Genevi\`eve B\'elanger, Benjamin, Fuks, Andreas Goudelis, Bryan Zaldivar

arXiv: 1705.02327 · 2017-07-25

## TL;DR

This paper analyzes pseudoscalar-mediated dark matter models, showing that LHC collider searches strongly constrain mediator masses above 100-200 GeV, especially with large top quark couplings, and future data will tighten these bounds.

## Contribution

It provides a comprehensive collider and cosmological analysis of pseudoscalar-mediated dark matter, highlighting the importance of LHC searches beyond traditional methods.

## Key findings

- Mediator masses above 100-200 GeV are excluded for large top couplings.
- LHC searches can surpass direct detection in constraining these models.
- Future collider and astrophysical data will further restrict parameter space.

## Abstract

Models in which dark matter particles communicate with the visible sector through a pseudoscalar mediator are well-motivated both from a theoretical and from a phenomenological standpoint. With direct detection bounds being typically subleading in such scenarios, the main constraints stem either from collider searches for dark matter, or from indirect detection experiments. However, LHC searches for the mediator particles themselves can not only compete with -- or even supersede -- the reach of direct collider dark matter probes, but they can also test scenarios in which traditional monojet searches become irrelevant, especially when the mediator cannot decay on-shell into dark matter particles or its decay is suppressed. In this work we perform a detailed analysis of a pseudoscalar-mediated dark matter simplified model, taking into account a large set of collider constraints and concentrating on the parameter space regions favoured by cosmological and astrophysical data. We find that mediator masses above 100-200~GeV are essentially excluded by LHC searches in the case of large couplings to the top quark, while forthcoming collider and astrophysical measurements will further constrain the available parameter space.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1705.02327/full.md

## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1705.02327/full.md

## References

116 references — full list in the complete paper: https://tomesphere.com/paper/1705.02327/full.md

---
Source: https://tomesphere.com/paper/1705.02327