Implications for minimal supersymmetry from grand unification and the neutralino relic abundance
dc.contributor.author | Roberts, R. G. | en_US |
dc.contributor.author | Roszkowski, Leszek | en_US |
dc.date.accessioned | 2006-04-10T15:40:27Z | |
dc.date.available | 2006-04-10T15:40:27Z | |
dc.date.issued | 1993-07-15 | en_US |
dc.identifier.citation | Roberts, 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.uri | http://www.sciencedirect.com/science/article/B6TVN-470W21T-3F6/2/d174636d875a9ec5294a9e87234b8f5f | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/30683 | |
dc.description.abstract | We 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.extent | 635745 bytes | |
dc.format.extent | 3118 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Elsevier | en_US |
dc.title | Implications for minimal supersymmetry from grand unification and the neutralino relic abundance | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbsecondlevel | Mathematics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Randall Physics Laboratory, University of Michigan, Ann Arbor, MI 48190, USA | en_US |
dc.contributor.affiliationother | Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 OQX, UK | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/30683/1/0000327.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0370-2693(93)90941-A | en_US |
dc.identifier.source | Physics Letters B | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
Files in this item
Remediation of Harmful Language
The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.
Accessibility
If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.