Abstract
This is an overview of recent developments and future prospects in the search for dark matter and new physics with astronomical and astro-particle techniques.
Highlights
This is an overview of recent developments and future prospects in the search for dark matter and new physics with astronomical and astro-particle techniques
Indirect detection refers to the exercise of seeking the hopefully unique astronomical, astro-particle, or cosmological signals that probe the particle nature of the Dark Matter (DM)
On largely model-independent grounds, the DM mass is constrained from below by quantum effects having to exist on scales smaller than the size of the smallest gravitationally collapsed objects, and from above from the requirement that macroscopic DM particles not disrupt the stability of long-lived structures in the universe, such as globular clusters and galactic disks
Summary
This is an overview of recent developments and future prospects in the search for dark matter and new physics with astronomical and astro-particle techniques. Indirect detection refers to the exercise of seeking the hopefully unique astronomical, astro-particle, or cosmological signals that probe the particle nature of the Dark Matter (DM).
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