2001/12/03 by D. G. Cerdeño, D. G. Cerdeno, Cerdeno, D. G. +6
Physics and Astronomy · #Astronomy and Astrophysical Research #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0112033
Talk given at COSMO-01, Rovaniemi, Finland, August 29-September 4, 2001. Latex, 13 pages, 7 figures
arxiv created 2001/12/03 · arxiv updated 2009/11/30
We study the direct detection of supersymmetric dark matter in the light of recent experimental results. In particular, we show that regions in the parameter space of several scenarios with a neutralino-nucleon cross section of the order of 10-6 pb, i.e., where current dark matter detectors are sensitive, can be obtained. These are supergravity scenarios with intermediate unification scale, and superstring scenarios with D-branes.