Abstract
The result from the LSND experiment are examined in the framework of three-flavour neutrino oscillations together with all other available experimental information. A comparison with solar, reactor and accelerator experiments indicates that the results are compatible in the 2.5 × 10 −1 < ΔM 2 < 3.0 eV 2 range. By assuming ΔM 2 = 3.0 eV 2, the corresponding mixing angles values are determined. For ΔM 2 = 3.0 eV 2, data on solar and atmospheric neutrinos combined with the limit on reactor experiments give a value for P eμ that is consistent with the LSND observation.
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