Solar neutrinos: Radiative corrections in neutrino-electron scattering experiments

Radiative corrections to the electron recoil-energy spectra and to total cross sections are computed for neutrino-electron scattering by solid neutrinos. Radiative corrections change monotonically the electron recoil spectrum for incident {sup 8}B neutrinos, with the relative probability of observin...

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Veröffentlicht in:Physical Review, D D, 1995-06, Vol.51 (11), p.6146-6158
Hauptverfasser: Bahcall, JN, Kamionkowski, M, Sirlin, A
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Kamionkowski, M
Sirlin, A
description Radiative corrections to the electron recoil-energy spectra and to total cross sections are computed for neutrino-electron scattering by solid neutrinos. Radiative corrections change monotonically the electron recoil spectrum for incident {sup 8}B neutrinos, with the relative probability of observing recoil electrons being reduced by about 4% at the highest electron energies. For {ital p}-{ital p} and {sup 7}Be 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 {sup 13}N and {sup 15}O neutrinos including radiative corrections.
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source American Physical Society Journals
subjects BORON 8
ELECTRONS
ENERGY SPECTRA
NEUTRINO-ELECTRON INTERACTIONS
NITROGEN 13
OXYGEN 15
PHYSICS
PROBABILITY
RADIATIVE CORRECTIONS
RECOILS
SOLAR NEUTRINOS
TOTAL CROSS SECTIONS
title Solar neutrinos: Radiative corrections in neutrino-electron scattering experiments
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