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VOLUME 59 (1994) | ISSUE 5 | PAGE 297
On the detection of neutrino flavour oscillations during observation of neutrino burst from stellar collapse in the galaxy
The ability of large volume scintillation counters based on white-spirit ((CH2)n) to select charged current (CC) v*tve interactions with 12С while observing a neutrino burst from a stellar collapse in the Galaxy is discussed. If there exist neutrino flavour oscillations *7*(r) *~* v* and the temperature of ι^,τ^μ,τ fluxes is higher than that of veue> the number of the С С interactions will increase. The scintillation counters have very good sensitivity to detect these effects.