
doi: 10.2172/555478
The cross sections for the processes {gamma}{nu} {yields} {gamma}{gamma} {yields} {nu}{anti {nu}} are calculated with the aid of an effective Lagrangian derived from the Standard model. These cross sections are shown to be much larger than the elastic cross section {sigma}({gamma}{nu} {yields} {gamma}{nu}) for photon energies {omega} {ge} 1 keV. Possible astrophysical implications are discussed.
Inelastic Scattering, Photon-Neutrino Interactions, Cross Sections, 66 Physics, Lagrangian Function, Elastic Scattering, 530
Inelastic Scattering, Photon-Neutrino Interactions, Cross Sections, 66 Physics, Lagrangian Function, Elastic Scattering, 530
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