# Multimessenger TeV Dark Matter: a mini review

## TL;DR

This paper reviews multimessenger indirect detection methods for multi-TeV dark matter, discussing key equations, uncertainties, and current experimental status in the context of gamma rays, neutrinos, and antiprotons.

## Contribution

It provides a concise overview of the multimessenger approach to dark matter detection, highlighting recent developments and open challenges in the field.

## Key findings

- Current multimessenger techniques constrain multi-TeV dark matter models.
- Uncertainties in dark matter distribution and cosmic rays impact detection sensitivity.
- Experimental limitations hinder definitive conclusions in dark matter searches.

## Abstract

We briefly review the general insight into the indirect searches of dark matter. We discuss the primary equation in a three-level multimessenger approach (gamma rays, neutrinos and antiprotons), and we introduce the reader to the main topics and related uncertainties (e.g. dark matter density distribution, cosmic rays, particle physics). As an application of the general concept, we focus on the multi-TeV dark matter candidate among other weak interactive massive particles. We present the state-of-the-art on this sub-field, and we discuss open questions and experimental limitations.