Dark Matter and Detector Cross Sections
| dc.creator | Arnowitt, R. | |
| dc.creator | Dutta, B. | |
| dc.creator | Santoso, Y. | |
| dc.date | 2000-08-30 | |
| dc.date | 2000-08-31 | |
| dc.date.accessioned | 2026-07-07T03:42:25Z | |
| dc.date.available | 2026-07-07T03:42:25Z | |
| dc.description | 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\times 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). | |
| dc.description | 5 pages, latex, 3 figures, talk at ICHEP 2000, Osaka, Japan, July 27-Aug. 2, 2000, change in title, no change in content | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0008320 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0008320 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/39895 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Dark Matter and Detector Cross Sections | |
| dc.type | text |