Collider Signatures of SuperWIMP Warm Dark Matter

Details Collider Signatures of SuperWIMP Warm Dark Matter Collider Signatures of SuperWIMP Warm Dark Matter

2006-03-09

arxiv.org/abs/hep-ph/0603067v1

ECONFC0508141:ALCPG0334,2005

Physics

High Energy Physics

High Energy Physics - Phenomenology

Contributed to the 2005 International Linear Collider Physics and Detector Workshop and 2nd ILC Accelerator Workshop, Snowmass

Scientific paper

SuperWeakly-Interacting Massive Particles (superWIMPs) produced in the late decays of other particles are well-motivated dark matter candidates and may be favored over standard Weakly-Interacting Massive Particles (WIMPs) by small scale structure observations. Among the most promising frameworks that incorporate superWIMPs are R-parity conserving supersymmetry models in which the lightest supersymmetric particle (LSP) is the gravitino or the axino. In these well-defined particle models, astrophysical observations have direct implications for possible measurements at future colliders.

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