arXiv · hep-ph/9208262
New Neutrino Physics Without Fine Tuning
Abstract
We 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.
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C. P. Burgess, James M. Cline, Markus Luty. 1992-08-31. New Neutrino Physics Without Fine Tuning. https://arxiv.org/abs/hep-ph/9208262
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