arXiv · hep-ph/0701011
Gravitino and Axino SuperWIMPs
Abstract
Gravitinos and axinos produced in the late decays of other supersymmetric particles are well-motivated dark matter (DM) candidates, whose experimental evidences are very distinctive and different from other standard candidates, as thermal produced neutralinos in similar supersymmetric models. In particular, charged sleptons could appear stable because of the length of its lifetime. The direct production of such particles at both the Large Hadron Collider (LHC) and a future International Linear Collider (ILC) can give not only a clear signature of supersymmetry but also the first non-gravitational evidence of dark matter.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
J. A. R. Cembranos, Jonathan L. Feng, A. Rajaraman, F. Takayama. 2007-01-01. Gravitino and Axino SuperWIMPs. https://doi.org/10.1063/1.2735254
Cite the original work for its findings. Save a collection to share your selection of sources.