Indirect Neutrino Oscillations

Details Indirect Neutrino Oscillations Indirect Neutrino Oscillations

1995-05-18

arxiv.org/abs/hep-ph/9505334v1

Phys.Lett.B359:351-354,1995; ERRATUM-ibid.B364:251,1995

Physics

High Energy Physics

High Energy Physics - Phenomenology

8 pages; compressed postscript

Scientific paper

10.1016/0370-2693(95)01080-A

We show how two different scales for oscillations between $e$ and $\mu$ neutrinos, characterized by different mixing angles and effective mass scales, can arise in a simple and theoretically attractive framework. One scale characterizes direct oscillations, which can accommodate the MSW approach to the solar neutrino problem, whereas the other can be considered as arising indirectly, through virtual transitions involving the $\tau$ neutrino with a mass $\sim$ 1 eV. This indirect transition allows the possibility of observable $\bar \nu_\mu \leftrightarrow \bar \nu_e$ oscillations at accelerator and reactor energies. We discuss specifically the parameters suggested by a recent experiment at Los Alamos within this framework.

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