Using L/E Oscillation Probability Distributions
A. A. Aguilar-Arevalo, B. C. Brown, L. Bugel, G. Cheng, E. D. Church,, J. M. Conrad, R. Dharmapalan, Z. Djurcic, D. A. Finley, R. Ford, F. G., Garcia, G. T. Garvey, J. Grange, W. Huelsnitz, C. Ignarra, R. Imlay, R. A., Johnson, G. Karagiorgi, T. Katori, T. Kobilarcik

TL;DR
This paper discusses how $L/E$ oscillation probability distributions can be used to compare experimental neutrino data with oscillation models, providing qualitative insights and methodological guidance, including corrections to previous analyses.
Contribution
It introduces a method for using $L/E$ distributions for model comparison and clarifies the calculation and interpretation of these distributions, including corrections to prior work.
Findings
Provides $L/E$ data points for MiniBooNE
Shows $L/E$ distributions offer qualitative model agreement insights
Corrects previous analysis by ICARUS
Abstract
This paper explores the use of oscillation probability distributions to compare experimental measurements and to evaluate oscillation models. In this case, is the distance of neutrino travel and is a measure of the interacting neutrino's energy. While comparisons using allowed and excluded regions for oscillation model parameters are likely the only rigorous method for these comparisons, the distributions are shown to give qualitative information on the agreement of an experiment's data with a simple two-neutrino oscillation model. In more detail, this paper also outlines how the distributions can be best calculated and used for model comparisons. Specifically, the paper presents the data points for the final MiniBooNE data samples and, in the Appendix, explains and corrects the mistaken analysis published by the ICARUS collaboration.
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Taxonomy
TopicsNeutrino Physics Research · Astrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena
