Electron Spectra in the Ionization of Atoms by Neutrinos
arXiv:hep-ph/0409053 · doi:10.1103/PhysRevD.70.113008
Abstract
For neutrinos of O(10keV) energies, their oscillation lengths are less than a few hundred meters, thereby suggesting the fascinating idea of oscillation experiments of small geometrical size. To help evaluating this idea we calculate the ionization cross sections of H, He, Ne and Xe, using any neutrino flavor, in the few keV energy range. We find that the atomic ionization cross sections per electron are always smaller than the neutrino cross sections off free electrons, approaching it from below as the energy increases to the 100 keV region. At the 10-20 keV range though, atomic binding effects are very important, particularly for the heavier atoms, inducing a factor of two reduction of the Xe ionization cross section, compared to the free electron one.
arXiv commentTypos corrected. Version appeared in Phys. Rev. D70:113008 (2004)
References in corpus (8)
- Limits on Neutrino Oscillations from the CHOOZ Experiment
- Measurement of the flux and zenith-angle distribution of upward through-going muons by Super-Kamiokande
- Solar Neutrinos Before and After Neutrino 2004
- Neutrino Properties Studied with a Triton Source Using Large TPC Detectors
- Prospects for Detecting a Neutrino Magnetic Moment with a Tritium Source and Beta-beams
- Neutrinos in Extra Dimensions and the Anomalous Magnetic Moments of Leptons
- The ionization of H, He and Ne atoms using neutrinos or antineutrinos at keV energies
- Neutrino Electron Scattering and Electroweak Gauge Structure: Future Tests
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