We study the neutrino-photon processes such as gamma gamma --> <v(v)over ba
r>, v gamma --> v gamma, and <v(v)over bar> --> gamma gamma in a background
magnetic field smaller than the critical magnetic field Bc + m(e)(2)/e. Us
ing Schwinger's formalism, we extract leading magnetic-field contributions
to the above processes. Our result is valid throughout the kinematic regime
where both neutrino and photon energies are significantly smaller than m(w
). We briefly discuss the astrophysical implications of our result. (C) 199
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