Neutrino flux prediction at MiniBooNE
By MiniBooNE Collaboration. 2008
247 citations recorded by the source corpus.
The booster neutrino experiment (MiniBooNE) searches for {nu}{sub {mu}}{yields}{nu}{sub e} oscillations using the O(1 GeV) neutrino beam produced by the booster synchrotron at the Fermi National Accelerator Laboratory). The booster delivers protons with 8 GeV kinetic energy (8.89 GeV/c momentum) to a beryllium target, producing neutrinos from the decay of secondary particles in the beam line. We describe the Monte Carlo simulation methods used to estimate the flux of neutrinos from the beam line incident on the MiniBooNE detector for both polarities of the focusing horn. The simulation uses the Geant4 framework for propagating particles, accounting for electromagnetic processes and hadronic interactions in the beam line materials, as well as the decay of particles. The absolute double differential cross sections of pion and kaon production in the simulation have been tuned to match external measurements, as have the hadronic cross sections for nucleons and pions. The statistical precision of the flux predictions is enhanced through reweighting and resampling techniques. Systematic errors in the flux estimation have been determined by varying parameters within their uncertainties, accounting for correlations where appropriate.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/e616e01ffaf2d45861db590013331921696412c6
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In Nuclear and High Energy Physics
Citations in the corpus
- Where are we with light sterile neutrinos? (2019, background): “5% [47].”
- Status of light sterile neutrino searches (2019, background): “All detectors are located in the Booster Neutrino Beamline (BNB) [204].”
- Neutrino non-standard interactions: A status report (2019, unknown): “[203].”
- Sterile Neutrino Fits to Short-Baseline Neutrino Oscillation Measurements (2012, background): “Pion sign selection, via a large magnet placed directly in the beamlines before the decay pipe, allows for nearly pure neutrino or antineutrino running, with only a few percent “wrong sign” neutrino flux content in the case of neutrino running, and ∼15% [46] in the case of antineutrino running.”