Electromagnetic radiative corrections to deep-inelastic neutrino interactions

The electromagnetic-radiative-correction factors to deep-inelastic neutrino-nucleon scattering are estimated using the parton-model formulas of Kiskis. Tables and approximate formulas are given for the benefit of experimenters wishing to estimate their own corrections. The corrections tend to be less than about 10%, and vary only slowly with energy, Q2, and x