Nonuniqueness of Representations of Wave Equations in Lorentzian Space-Times
Horst Reinhard Beyer

TL;DR
This paper highlights the nonuniqueness of initial-boundary value problem formulations for wave equations in Lorentzian space-times, showing that different formulations can lead to different stability outcomes, with implications for various physically relevant spacetimes.
Contribution
It demonstrates that the formulation of initial-boundary value problems in Lorentzian space-times is not unique and can affect stability analysis, using the Rindler wedge as a case study.
Findings
Multiple inequivalent formulations exist for wave equations in Lorentzian space-times.
Different formulations can lead to different stability outcomes.
Methods can be extended to higher-dimensional space-times like Schwarzschild and Kerr.
Abstract
This brief note wants to bring to attention that the formulation of physically reasonable initial-boundary value problems for wave equations in Lorentzian space-times is not unique, i.e., that there are inequivalent such formulations that lead to a different outcome of the stability discussion of the solutions. For demonstration, the paper uses the case of the wave equation on the right Rindler wedge in 2-dimensional Minkowski space. The used methods can be generalized to wave equations on stationary globally hyperbolic space-times with horizons in higher dimensions, such as Schwarzschild and Kerr space-times.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
