Light relic neutralinos in Dark Matter direct and indirect searches and at the Large Hadron Collider

Details Light relic neutralinos in Dark Matter direct and indirect searches and at the Large Hadron Collider Light relic neutralinos in Dark Matter direct and indirect searches and at the Large Hadron Collider

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1115..111s&link_type=abstract

THE DARK SIDE OF THE UNIVERSE: 4th International Workshop on the Dark Side of the Universe. AIP Conference Proceedings, Volume

Physics

Dark Matter, Supersymmetric Models, Neutrino Interactions

Scientific paper

We show that light relic neutralinos which arise in R-parity conserving Susy models where gaugino masses are not unified at a Grand Unified (GUT) scale can explain the new DAMA annual modulation result. The same configurations are also discussed in connection to indirect signals from galactic antiprotons. Prospects of detection of these light relic neutralinos at the Large Hadron Collider are also analyzed and look promising.

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