Solar Neutrinos: Radiative Corrections in Neutrino-Electron Scattering Experiments

Details Solar Neutrinos: Radiative Corrections in Neutrino-Electron Scattering Experiments Solar Neutrinos: Radiative Corrections in Neutrino-Electron Scattering Experiments

1995-02-01

arxiv.org/abs/astro-ph/9502003v1

Phys.Rev. D51 (1995) 6146-6158

Astronomy and Astrophysics

Astrophysics

40 pages, uuencoded, Z-compress file.

Scientific paper

10.1103/PhysRevD.51.6146

Radiative corrections to the electron recoil-energy spectra and to total cross sections are computed for neutrino-electron scattering by solar neutrinos. Radiative corrections change monotonically the electron recoil spectrum for incident \b8 neutrinos, with the relative probability of observing recoil electrons being reduced by about 4 \% at the highest electron energies. For $p-p$ and $\be7$ neutrinos, the recoil spectra are not affected significantly. Total cross sections for solar neutrino-electron scattering are reduced by about 2 \% compared to previously computed values. We also calculate the recoil spectra from $^{13}$N and $^{15}$O neutrinos including radiative corrections.

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