Study of neutrino spin oscillations in a gravitational field with a differential equations method
arXiv:2510.26621 · doi:10.1134/S1063779626701595
Abstract
In this work, we employ Ordinary Differential Equation solution method to study neutrino spin oscillations in the case when they are gravitationally scattered off a rotating Kerr black hole. Previously, this problem involved the integral solution of the Hamilton-Jacobi equation. We analyze the consistency of these two methods.
Contribution to The XXVIth International Baldin Seminar on High Energy Physics Problems "Relativistic Nuclear Physics and Quantum Chromodynamics" (ISHEPP 2025). 12 pages, 4 figures