Collider Signatures of SuperWIMP Warm Dark Matter

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dc.creatorCembranos, Jose A. R.
dc.creatorFeng, Jonathan L.
dc.creatorRajaraman, Arvind
dc.creatorSmith, Bryan T.
dc.creatorTakayama, Fumihiro
dc.date2006-03-09
dc.date.accessioned2026-07-07T10:29:52Z
dc.date.available2026-07-07T10:29:52Z
dc.descriptionSuperWeakly-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.
dc.descriptionContributed to the 2005 International Linear Collider Physics and Detector Workshop and 2nd ILC Accelerator Workshop, Snowmass, Colorado, 14-27 Aug 2005. 3 pages, LaTeX, 1 figure
dc.identifierhttps://arxiv.org/abs/hep-ph/0603067
dc.identifierhttp://arxiv.org/abs/hep-ph/0603067
dc.identifierECONFC0508141:ALCPG0334,2005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177961
dc.subjectHigh Energy Physics - Phenomenology
dc.titleCollider Signatures of SuperWIMP Warm Dark Matter
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