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We propose that dark matter is composed of particles that naturally have thecorrect thermal relic density, but have neither weak-scale masses nor weakinteractions. These WIMPless models emerge naturally from gauge-mediatedsupersymmetry breaking, where they elegantly solve the dark matter problem. Theframework accommodates single or multiple component dark matter, dark mattermasses from 10 MeV to 10 TeV, and interaction strengths from gravitational tostrong. These candidates enhance many direct and indirect signals relative toWIMPs and have qualitatively new implications for dark matter searches andcosmological implications for colliders.

The WIMPless Miracle: Dark Matter Particles without Weak-scale Masses or Weak Interactions