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arxiv: hep-ph/0302215 · v2 · submitted 2003-02-25 · ✦ hep-ph · astro-ph

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Superweakly Interacting Massive Particles

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classification ✦ hep-ph astro-ph
keywords darkmattersuperwimpsconventionalmassiveparticleswimpsappear
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We investigate a new class of dark matter: superweakly-interacting massive particles (superWIMPs). As with conventional WIMPs, superWIMPs appear in well-motivated particle theories with naturally the correct relic density. In contrast to WIMPs, however, superWIMPs are impossible to detect in all conventional dark matter searches. We consider the concrete examples of gravitino and graviton cold dark matter in models with supersymmetry and universal extra dimensions, respectively, and show that superWIMP dark matter satisfies stringent constraints from Big Bang nucleosynthesis and the cosmic microwave background.

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  1. Can LLP detectors probe the reheating temperature? A case study of vector dark matter

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    In a vector dark matter extension of the Higgs portal, far detectors at colliders can probe otherwise inaccessible parameter space and set novel bounds on the reheating temperature.