Mass and Mixing Angles of the τ Neutrino

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

We examine the possibility that the τ neutrino is sufficiently massive to require it to be unstable (mντ>~50 eV). A combination of experimental and astrophysical bounds requires a mass greater than 10 MeV. For larger masses, we bracket the lifetime and decay modes of ντ, and we give concomitant limits on the leptonic mixing angles.

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