2000/08/30 by R. Arnowitt, Arnowitt, R., B. Dutta +4
Engineering · Physics and Astronomy · #CCD and CMOS Imaging Sensors #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0008320
5 pages, latex, 3 figures, talk at ICHEP 2000, Osaka, Japan, July 27-Aug. 2, 2000, change in title, no change in content
openalex publication_date 2000/08/30 · arxiv created 2000/08/31 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We consider here the spin independent neutralino-proton cross section for a variety of SUGRA and D-brane models with R-parity invariance. The minimum cross section generally is >~ 1× 10-(9-10) pb (and hence accessible to future detectors) except for special regions of parameter space where it may drop to =~ 10-12 pb. In the latter case the gluino and squarks will be heavy (>~ 1 TeV).