New Neutrino Physics Without Fine Tuning

Simple item page
dc.creatorBurgess, C. P.
dc.creatorCline, James M.
dc.creatorLuty, Markus
dc.date1992-08-31
dc.date.accessioned2026-07-07T03:55:40Z
dc.date.available2026-07-07T03:55:40Z
dc.descriptionWe show how a 17 keV neutrino, the solar neutrino problem, and the atmospheric muon-neutrino deficit could all be the low-energy residues of the same pattern of lepton-number breaking at and above the weak scale, with no requirement for fine-tuning a symmetry-breaking scale at lower energies. Talk given at ``Beyond the Standard Model III'', Carleton University, June 1992.
dc.description6 pages, (LaTeX) McGill-92/36
dc.identifierhttps://arxiv.org/abs/hep-ph/9208262
dc.identifierhttp://arxiv.org/abs/hep-ph/9208262
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44644
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNew Neutrino Physics Without Fine Tuning
dc.typetext

Files

Collections

arXiv