Abstract
Hints of physics beyond the Standard Model come from solar1 and atmospheric2neutrino experiments, where apparent deficits are interpreted as signs of oscillations, and also from the claim of the LSND experiment,3where a signal of \({\bar v_e}\) is observed in a beam which does not contain this flavour at production. Figure 1 shows the preferred regions corresponding to these three ‘evidences’. They do not necessarily apply to the same physical oscillation channel.
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Vannucci, F. (1997). Neutrino Oscillations at Accelerators. In: Kursunoglu, B.N., Mintz, S.L., Perlmutter, A. (eds) High-Energy Physics and Cosmology. Springer, Boston, MA. https://doi.org/10.1007/978-1-4615-5397-7_2
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DOI: https://doi.org/10.1007/978-1-4615-5397-7_2
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