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Implications for minimal supersymmetry from grand unification and the neutralino relic abundance

dc.contributor.authorRoberts, R. G.en_US
dc.contributor.authorRoszkowski, Leszeken_US
dc.date.accessioned2006-04-10T15:40:27Z
dc.date.available2006-04-10T15:40:27Z
dc.date.issued1993-07-15en_US
dc.identifier.citationRoberts, R. G., Roszkowski, Leszek (1993/07/15)."Implications for minimal supersymmetry from grand unification and the neutralino relic abundance." Physics Letters B 309(3-4): 329-336. <http://hdl.handle.net/2027.42/30683>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6TVN-470W21T-3F6/2/d174636d875a9ec5294a9e87234b8f5fen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/30683
dc.description.abstractWe examine various predictions of the minimal supersymmetric standard model coupled to minimal supergravity. The previously considered predictions of the model are now extended to include the bottom quark mass and the neutralino relic density which in turn provide stringent bounds on the scale parameters. We find a remarkable consistency among several different constraints only in the region of low-energy supersymmetry, thus avoiding the use of the fine tuning criterion. We find all supersymmetric particle masses preferably within the reach of future supercolliders (LHC and SSC). The requirement that the neutralino be the dominant component of (dark) matter in the flat Universe provides a lower bound on the spectrum of supersymmetric particles beyond the reach of LEP, and most likely also the Tevatron and LEP 200.en_US
dc.format.extent635745 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleImplications for minimal supersymmetry from grand unification and the neutralino relic abundanceen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbsecondlevelMathematicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumRandall Physics Laboratory, University of Michigan, Ann Arbor, MI 48190, USAen_US
dc.contributor.affiliationotherRutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 OQX, UKen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/30683/1/0000327.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0370-2693(93)90941-Aen_US
dc.identifier.sourcePhysics Letters Ben_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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