Calculating error bars for neutrino mixing parameters
H. R. Burroughs, B. K. Cogswell, J. Escamilla-Roa, D. C. Latimer, and, D. J. Ernst

TL;DR
This paper introduces a method for calculating error bars for neutrino mixing parameters using the likelihood function, especially effective when data is statistically poor or near boundaries, improving confidence interval accuracy.
Contribution
It proposes a likelihood-based approach for confidence interval estimation in neutrino oscillation data, addressing limitations of Gaussian assumptions in poor statistics scenarios.
Findings
Method yields significantly different confidence intervals from traditional methods.
Applied to T2K data, the method shows a 92% probability that chi-square is not zero.
Traditional Gaussian-based methods overestimate confidence levels, e.g., 99.5%.
Abstract
One goal of contemporary particle physics is to determine the mixing angles and mass-squared differences that constitute the phenomenological constants that describe neutrino oscillations. Of great interest are not only the best fit values of these constants but also their errors. Some of the neutrino oscillation data is statistically poor and cannot be treated by normal (Gaussian) statistics. To extract confidence intervals when the statistics are not normal, one should not utilize the value for chisquare versus confidence level taken from normal statistics. Instead, we propose that one should use the normalized likelihood function as a probability distribution; the relationship between the correct chisquare and a given confidence level can be computed by integrating over the likelihood function. This allows for a definition of confidence level independent of the functional form of the…
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