Perturbative exponential expansion and matter neutrino oscillations
A. D. Supanitsky, J. C. D'Olivo, G. Medina-Tanco

TL;DR
This paper presents a simple, analytical method using Magnus exponential representation to accurately describe matter neutrino oscillations across various energies, improving upon existing perturbative approaches and applicable to diverse neutrino sources.
Contribution
It introduces a novel Magnus exponential-based analytical framework for neutrino oscillations in matter, enhancing accuracy and simplicity over previous perturbative methods.
Findings
Reproduces numerical day-night asymmetry with better than 1% accuracy at first order.
Improves accuracy to better than 5% at second order for neutrino energies up to 100 MeV.
Accurately models maxima positions in flavor transition probabilities in the GeV energy range.
Abstract
We derive an analytical description of neutrino oscillations in matter based on the Magnus exponential representation of the time evolution operator. Our approach is valid in a wide range of the neutrino energies and properly accounts for the modifications that the respective probability transitions suffer when neutrinos originated in different sources traverse the Earth. The present approximation considerably improves over other perturbative treatments existing in the current literature. Furthermore, the analytical expressions derived inside the Magnus framework are remarkably simple, which facilitates their practical use. When applied to the calculation of the day-night asymmetry in the solar neutrino flux our result reproduces the numerical calculation with an accuracy better than 1% for the first order approximation. When the approximation is extended to the second order, the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
