Quantifying the sensitivity of oscillation experiments to the neutrino mass ordering
Mattias Blennow, Pilar Coloma, Patrick Huber, Thomas Schwetz
TL;DR
This paper clarifies the statistical interpretation of sensitivity to neutrino mass ordering by situating it in a frequentist hypothesis-testing framework and introducing the Gaussian limit for the test statistic $T$. It demonstrates that the median sensitivity under Gaussian assumptions closely matches the conventional $\sqrt{\Delta\chi^2}$-based sensitivities and provides analytic expressions to compute power and crossing sensitivities, including for composite hypotheses. Through Monte Carlo simulations of JUNO, INO, PINGU, NO$\nu$A, and LBNE, the authors validate the Gaussian approximation for most setups and quantify deviations (notably in NO$\nu$A) while showing strong agreement for others. The study offers a practical, statistically rigorous toolkit to compare current and future experiments’ capabilities to determine the neutrino mass ordering, with implications for experimental design and the interpretation of sensitivities.
Abstract
Determining the type of the neutrino mass ordering (normal versus inverted) is one of the most important open questions in neutrino physics. In this paper we clarify the statistical interpretation of sensitivity calculations for this measurement. We employ standard frequentist methods of hypothesis testing in order to precisely define terms like the median sensitivity of an experiment. We consider a test statistic $T$ which in a certain limit will be normal distributed. We show that the median sensitivity in this limit is very close to standard sensitivities based on $Δχ^2$ values from a data set without statistical fluctuations, such as widely used in the literature. Furthermore, we perform an explicit Monte Carlo simulation of the INO, JUNO, LBNE, NOvA, and PINGU experiments in order to verify the validity of the Gaussian limit, and provide a comparison of the expected sensitivities for those experiments.
