Non-Perturbative Effects of Strong Magnetic Fields on Neutrino Self-energy: A New Approach
Abstract
The Ritus' Ep eigenfunction method is extended to the case of spin-1 charged particles in a constant electromagnetic field and used to calculate the one-loop neutrino self-energy in the strong-field approximation me2 eB MW2. The implications of the obtained results for neutrino oscillations in the early Universe, assuming the existence of a sufficiently large (me2 eB mμ2) primordial magnetic field, are discussed.
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