Efficient numerical integration of neutrino oscillations in matter
Fernando Casas, Jose Angel Oteo, Juan Carlos D'Olivo

TL;DR
This paper introduces a Magnus expansion-based solver that significantly accelerates the numerical integration of three-neutrino oscillation equations in matter, facilitating faster data analysis in neutrino physics.
Contribution
The paper presents a specialized, efficient solver for neutrino oscillation equations that outperforms general integrators in speed by up to two orders of magnitude.
Findings
Speed improvement up to 100 times over general integrators
Detailed analysis of numerical procedure and computational costs
Potential to enhance large-scale neutrino data analysis
Abstract
A special purpose solver, based on the Magnus expansion, well suited for the integration of the linear three neutrino oscillations equations in matter is proposed. The computations are speeded up to two orders of magnitude with respect to a general numerical integrator, a fact that could smooth the way for massive numerical integration concomitant with experimental data analyses. Detailed illustrations about numerical procedure and computer time costs are provided.
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