Pierre Auger Observatory and Super Heavy Dark Matter

TL;DR

This paper explores how data from the Pierre Auger Observatory can constrain models of super heavy dark matter particles generated in the early universe, emphasizing the observatory's powerful constraining capabilities.

Contribution

It introduces the use of Pierre Auger Observatory data to test and limit super heavy dark matter models from early universe scenarios.

Findings

Auger data strongly constrains super heavy dark matter models

Observations limit the parameter space of early universe generated particles

The study highlights the observatory's role in dark matter research

Abstract

We briefly discuss the connection of the Pierre Auger Observatory data with a large class of dark matter models based on the early universe generation of super heavy particles, their role in the solution of the dark matter problem, highlighting the remarkable constraining capabilities of the Auger observations.