pith. sign in

arxiv: hep-ph/0603067 · v1 · submitted 2006-03-09 · ✦ hep-ph

Collider Signatures of SuperWIMP Warm Dark Matter

classification ✦ hep-ph
keywords particlesdarkmassivemattermodelsobservationsparticlesuperwimps
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.