Neutralino Dark Matter in Minimal Supergravity: Direct Detection vs. Collider Searches

dc.creatorBaer, Howard
dc.creatorBrhlik, Michal
dc.date1997-06-25
dc.date.accessioned2026-07-07T10:33:32Z
dc.date.available2026-07-07T10:33:32Z
dc.descriptionWe calculate expected event rates for direct detection of relic neutralinos as a function of parameter space of the minimal supergravity model. Numerical results are presented for the specific case of a $^{73}$Ge detector. We find significant detection rates ($R> 0.01$ events/kg/day) in regions of parameter space most favored by constraints from $B\to X_sγ$ and the cosmological relic density of neutralinos. The detection rates are especially large in regions of large $\tanβ$, where many conventional signals for supersymmetry at collider experiments are difficult to detect. If the parameter $\tanβ$ is large, then there is a significant probability that the first direct evidence for supersymmetry could come from direct detection experiments, rather than from collider searches for sparticles.
dc.description25 page REVTEX file including 9 PS figures
dc.identifierhttps://arxiv.org/abs/hep-ph/9706509
dc.identifierhttp://arxiv.org/abs/hep-ph/9706509
dc.identifierPhys.Rev.D57:567-577,1998
dc.identifierdoi:10.1103/PhysRevD.57.567
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179146
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutralino Dark Matter in Minimal Supergravity: Direct Detection vs. Collider Searches
dc.typetext

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