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VOLUME 59 (1994) | ISSUE 5 | PAGE 297
Detection of neutrino flavor oscillations during observation of a neutrino burst from a stellar collapse in the galaxy
The ability of large-volume scintillation counters based on white spirit [(CH2)„] to select charged current (CC) ve,ve interactions with 12C, while observing a neutrino burst from a stellar collapse in the Galaxy is discussed. If there exist neutrino flavor oscillations, v^^+Vg, and the temperature of νμ>τν fluxes is higher than that of veve, then the number of the CC interactions will increase. The scintillation counters have very high sensitivity for detection of these effects.