Emission of neutrinos by alternating fields |
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Authors: | V. V. Skobelev |
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Affiliation: | 1. Moscow Institute of Geodesy, Aerial Photography, and Cartography Engineers, USSR
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Abstract: | It is supposed that the effective Lagrangian of interaction of a magnetic field with a neutrino can be written in the form $$L_{eff} = frac{{G_{mathbf{gamma }} }}{{m_W^2 }} frac{{partial ^2 A^mu }}{{partial x^v partial x_v }}[bar Psi _v {mathbf{gamma }}_mu (1 + {mathbf{gamma }}^5 )Psi _v ].$$ Formulas are obtained for the emission of neutrinos by alternating fields. In particular, neutrino synchrotron emission and neutrino emission in the case of collision of two classical charges are considered. Arguments are presented that this mechanism can make a contribution to the neutrino luminosity of stars. |
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