Maximum And Minimum Dark Matter Detection Cross Sections

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dc.creatorArnowitt, R.
dc.creatorDutta, B.
dc.creatorSantoso, Y.
dc.date2000-08-31
dc.date.accessioned2026-07-07T03:42:26Z
dc.date.available2026-07-07T03:42:26Z
dc.descriptionThe range of neutralino-proton cross sections for R-parity preserving supergravity models with GUT scale unification of the gauge coupling constants is examined. The models considered here are mSUGRA, models with non universal soft breaking and D-brane models. It is found that the current dark matter detectors are sampling significant parts of the SUSY parameter space and future detectors could sample almost the entire space. The special regions of parameter space that may be inaccessible to future detectors are seen to have a squark/gluino spectra beyond 1 TeV, but observable at the LHC.
dc.description11 pages, latex, 8 figures, based on invited talk at Workshop on the Next Generation U.S. Underground Facility, Carlsbad, NM, June, 2000
dc.identifierhttps://arxiv.org/abs/hep-ph/0008336
dc.identifierhttp://arxiv.org/abs/hep-ph/0008336
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/39899
dc.subjectHigh Energy Physics - Phenomenology
dc.titleMaximum And Minimum Dark Matter Detection Cross Sections
dc.typetext

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