Perhaps scalar neutrinos are the lightest supersymmetric partners
dc.contributor.author | Hagelin, John S. | en_US |
dc.contributor.author | Kane, Gordon L. | en_US |
dc.contributor.author | Raby, Stuart | en_US |
dc.date.accessioned | 2006-04-07T18:25:45Z | |
dc.date.available | 2006-04-07T18:25:45Z | |
dc.date.issued | 1984-07-23 | en_US |
dc.identifier.citation | Hagelin, John S., Kane, G. L., Raby, S. (1984/07/23)."Perhaps scalar neutrinos are the lightest supersymmetric partners." Nuclear Physics B 241(2): 638-652. <http://hdl.handle.net/2027.42/24754> | en_US |
dc.identifier.uri | http://www.sciencedirect.com/science/article/B6TVC-471XJYJ-5K/2/33cef30fac70899d3133f7771ab6b630 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/24754 | |
dc.description.abstract | We consider the possibility that the scalar partners of the neutrinos are the least massive supersymmetric partners, and show that this alternative is compatible with cosmological constraints, which put a significant lower bound on photino masses but not on masses. Various consequences are examined: the photon counting rate for 0--> increases [Gamma](Z0) by about 0.25 GeV; may be enhanced; the decay <inl may be detectable; there can be additional contributions to the rare decay <inl; restrictions on gluino masses, which depend on photinos interacting before they decay, have to be re-examined; scalar neutrinos have suitable characteristics as candidates for dark matter in the universe. We discuss one currently fashionable class of models that can predicr a light . | en_US |
dc.format.extent | 661682 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 | Perhaps scalar neutrinos are the lightest supersymmetric partners | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbsecondlevel | Nuclear Engineering and Radiological Sciences | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.subject.hlbtoplevel | Engineering | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Randall Laboratory of Physics, University of Michigan, Ann Arbor, MI 48109, USA | en_US |
dc.contributor.affiliationum | Randall Laboratory of Physics, University of Michigan, Ann Arbor, MI 48109, USA | en_US |
dc.contributor.affiliationother | Department of Physics, Maharishi International University, Fairfield, IA 52556, USA | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/24754/1/0000176.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0550-3213(84)90064-6 | en_US |
dc.identifier.source | Nuclear Physics B | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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