Analytical Approximation of the Neutrino Oscillation Matter Effects at large $\theta_{13}$
Sanjib Kumar Agarwalla, Yee Kao, and Tatsu Takeuchi

TL;DR
This paper introduces a simple analytical method to approximate neutrino oscillation probabilities in matter at large , improving accuracy over previous approximations by accounting for the running of mixing parameters.
Contribution
The authors propose a novel analytical approximation framework that models the running of neutrino mixing parameters in matter, simplifying calculations especially at large and improving accuracy over existing methods.
Findings
The approximation accurately matches exact numerical results.
Neglecting the running of and parameters simplifies analysis.
The method aids in determining optimal baseline lengths and energies.
Abstract
We argue that the neutrino oscillation probabilities in matter are best understood by allowing the mixing angles and mass-squared differences in the standard parametrization to `run' with the matter effect parameter , where is the electron density in matter and is the neutrino energy. We present simple analytical approximations to these `running' parameters. We show that for the moderately large value of , as discovered by the reactor experiments, the running of the mixing angle and the CP violating phase can be neglected. It simplifies the analysis of the resulting expressions for the oscillation probabilities considerably. Approaches which attempt to directly provide approximate analytical expressions for the oscillation probabilities in matter suffer in accuracy due to their reliance on expansion in , or…
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