skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Solar neutrinos: Radiative corrections in neutrino-electron scattering experiments

Abstract

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.

Authors:
 [1];  [1];  [2]
  1. Institute for Advanced Study, Olden Lane, Princeton, New Jersey 08540 (United States)
  2. Department of Physics, New York University, New York, New York 10003 (United States)
Publication Date:
Research Org.:
Institute for Advanced Study, Princeton, NJ (United States)
OSTI Identifier:
45674
DOE Contract Number:  
FG02-90ER40542; FG02-92ER40699
Resource Type:
Journal Article
Journal Name:
Physical Review, D
Additional Journal Information:
Journal Volume: 51; Journal Issue: 11; Other Information: PBD: 1 Jun 1995
Country of Publication:
United States
Language:
English
Subject:
66 PHYSICS; SOLAR NEUTRINOS; NEUTRINO-ELECTRON INTERACTIONS; RADIATIVE CORRECTIONS; ELECTRONS; RECOILS; ENERGY SPECTRA; TOTAL CROSS SECTIONS; BORON 8; NITROGEN 13; OXYGEN 15; PROBABILITY

Citation Formats

Bahcall, J N, Kamionkowski, M, Physics Department, Columbia University, New York, New York 10027, and Sirlin, A. Solar neutrinos: Radiative corrections in neutrino-electron scattering experiments. United States: N. p., 1995. Web. doi:10.1103/PhysRevD.51.6146.
Bahcall, J N, Kamionkowski, M, Physics Department, Columbia University, New York, New York 10027, & Sirlin, A. Solar neutrinos: Radiative corrections in neutrino-electron scattering experiments. United States. https://doi.org/10.1103/PhysRevD.51.6146
Bahcall, J N, Kamionkowski, M, Physics Department, Columbia University, New York, New York 10027, and Sirlin, A. 1995. "Solar neutrinos: Radiative corrections in neutrino-electron scattering experiments". United States. https://doi.org/10.1103/PhysRevD.51.6146.
@article{osti_45674,
title = {Solar neutrinos: Radiative corrections in neutrino-electron scattering experiments},
author = {Bahcall, J N and Kamionkowski, M and Physics Department, Columbia University, New York, New York 10027 and Sirlin, A},
abstractNote = {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.},
doi = {10.1103/PhysRevD.51.6146},
url = {https://www.osti.gov/biblio/45674}, journal = {Physical Review, D},
number = 11,
volume = 51,
place = {United States},
year = {Thu Jun 01 00:00:00 EDT 1995},
month = {Thu Jun 01 00:00:00 EDT 1995}
}