arXiv · hep-ph/9808294
Direct computation of inelastic photon-neutrino processes in the Standard Model
Abstract
In this paper, we compute the Standard Model polarized amplitudes and cross sections of the processes $γν\toγγν$, $γγ\to γν\barν$ and $ν\barν\to γγγ$, for centre-of-mass energies $ω$ within the range of validity of the Fermi theory. By using a large electron-mass expansion of the exact result, we also derive the first correction term to the effective, low-energy ($ω< m_e$) formula for $γν\toγγν$. Finally, we discuss possible astrophysical implications of our results and provide simple fits to the exact expressions.
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A. Abada, J. Matias, R. Pittau. 1998-08-11. Direct computation of inelastic photon-neutrino processes in the Standard Model. https://doi.org/10.1016/s0550-3213(98)00790-1
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