TL;DR
This paper discusses WIMPless dark matter, a candidate in hidden sectors with suitable relic density and diverse masses, arising naturally from gauge-mediated supersymmetry breaking.
Contribution
It introduces the WIMPless dark matter scenario, showing it can naturally produce the correct relic density across a wide mass range.
Findings
Dark matter candidate in hidden sector matches observed relic density
Wide range of possible masses for WIMPless dark matter
Natural emergence from gauge-mediated supersymmetry breaking
Abstract
We describe the scenario of WIMPless dark matter. In this scenario of gauge-mediated supersymmetry breaking, a dark matter candidate in the hidden sector is found to naturally have approximately the right relic density to explain astronomical dark matter observations, but with a wide range of possible masses.
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