Implications of a nonzero neutrino mass for the process γγ-->νν¯

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

Recent considerations relating to neutrino oscillations and to the decay μ-->eγ suggest that neutrinos may acquire a small but nonzero mass. The process γγ-->π0-->νν¯ could then proceed via either an induced S,P coupling arising from a primitive V,A neutrino current or via a fundamental S,P neutrino coupling. Although the resulting γγ-->π0-->νν¯ cross section would, in the former case, be suppressed by a factor of order (mνmπ)2, this process could, nonetheless, be of interest in astrophysical processes in a temperature region where the pion pole is significant.

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