Stellar energy loss and anomalous contributions to γγ-->νν¯

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Elementary Particle Processes, Other Topics In Specific Reactions And Phenomenology Of Elementary Particles

Scientific paper

We compute the stellar energy-loss rate for several anomalous
contributions to γγ-->νν¯ and for massive
neutrinos. Except for the cases where the mass scale of these new
contributions is small, or the neutrino masses are large, these
reactions are not important as a mechanism for stellar energy loss.

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