On the application of Lorentz-Finsler geometry to model wave propagation
Enrique Pendás-Recondo
TL;DR
This work presents a cohesive, step-by-step framework that uses Lorentz-Finsler geometry to model wave propagation in anisotropic, time-varying media. By embedding time as a spacetime dimension and defining a Lorentz-Finsler metric $G$ with lightlike pregeodesics, the authors unify Fermat's and Huygens' principles within a single geometric scheme, enabling efficient computation of wave trajectories and fronts. The paper provides explicit methodological steps—from initial-front orthogonality to pregeodesic integration and cut-point handling—forming a practical pipeline for real-time wavefront evolution. The approach offers a flexible, accurate alternative to PDE-based wave equations, adaptable to diverse physical settings (e.g., sound, seismic, wildfires) and capable of incorporating complex, direction-dependent speed profiles through the $F$-induced indicatrix on $N$ and its spacetime extension.
Abstract
The recent increasing interest in the study of Lorentz-Finsler geometry has led to several applications to model real-world physical phenomena. Our purpose is to provide a simple, step-by-step review on how to build and implement such a geometric model to describe the propagation of a classical wave satisfying Fermat's and Huygens' principles in an anisotropic and rheonomic (time-dependent) medium. The model is based on identifying the individual wave trajectories as lightlike pregeodesics of a specific Lorentz-Finsler metric, which obey a simple ODE system and can therefore be easily computed in real time.
