TL;DR
This paper reviews the evidence for dark matter in the universe, discusses astrophysical methods to probe its nature through multi-frequency analysis, and explores strategies for multi-messenger searches to uncover its properties.
Contribution
It provides a comprehensive overview of current astrophysical probes and strategies for detecting and understanding dark matter using multi-frequency and multi-messenger approaches.
Findings
Evidence accumulation supports dark matter's existence
Multi-frequency analysis constrains dark matter scenarios
Multi-messenger strategies enhance detection prospects
Abstract
The presence of Dark Matter (DM) is required in the universe regulated by the standard general relativistic theory of gravitation. The nature of DM is however still elusive to any experimental search. We discuss here the process of accumulation of evidence for the presence of DM in the universe, the astrophysical probes for the leading DM scenarios that can be obtained through a multi-frequency analysis of cosmic structures on large scales, and the strategies related to the multi-messenger and multi-experiment astrophysical search for the nature of the DM.
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