Neutrino properties and SUSY without $R$-parity

Details Neutrino properties and SUSY without $R$-parity Neutrino properties and SUSY without $R$-parity

1996-09-30

arxiv.org/abs/hep-ph/9609528v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, 3 PS-fig, LATEX, uses world-sci.sty

Scientific paper

In supersymmetric models without $R$-parity neutrinos naturally become massive and mix with each other. We explore the predictions of a very restricted model with only three free parameters and find that this model naturally yields masses and mixing angles compatible with experimental results from solar and atmospheric neutrino experiments. Furthermore, there is a tiny region in parameter space where the solution to the solar neutrino puzzle is compatible with either the LSND result or the existence of significant hot dark matter neutrinos.

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