Dark Matter Candidates of a Very Low Mass
Kathryn M. Zurek

TL;DR
This paper reviews very low mass dark matter candidates, exploring their theoretical motivations, detection methods, and experimental prospects, especially focusing on hidden sectors, astrophysical observations, and condensed matter detection techniques.
Contribution
It provides a comprehensive overview of low mass dark matter candidates and discusses novel detection strategies across astrophysics and condensed matter physics.
Findings
Potential for detection via low-energy colliders with intense beams
Astrophysical observations can constrain small DM interactions
Condensed matter techniques offer new detection avenues
Abstract
We review dark matter (DM) candidates of a very low mass, appearing in the window below the traditional weakly-interacting massive particle GeV and extending down to meV, somewhat below the mass limit where DM becomes wavelike. Such candidates are motivated by hidden sectors such as Hidden Valleys, which feature hidden forces and rich dynamics, but have evaded traditional collider searches looking for New Physics because of their relatively weak coupling to the Standard Model. Such sectors can still be detected through dedicated low-energy colliders which, through their intense beams, can have sensitivity to smaller couplings, or through astrophysical observations of the evolution of DM halos and stellar structures which, through the Universe's epochs, can be sensitive to small DM interactions. We also consider mechanisms where the DM abundance is…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Particle Detector Development and Performance
