On well-posedness of the Cauchy problem for the wave equation in static spherically symmetric spacetimes
Ricardo E. Gamboa Sarav\'i, Marcela Sanmartino, Philippe, Tchamitchian

TL;DR
This paper establishes simple, general conditions for the well-posedness of the Cauchy problem for scalar fields in static, spherically symmetric spacetimes, focusing on properties of the spatial wave operator.
Contribution
It introduces the concept of quasi essentially self-adjointness and characterizes conditions ensuring well-posedness beyond standard self-adjointness assumptions.
Findings
Conditions for well-posedness related to operator properties
Introduction of quasi essentially self-adjointness as a key concept
Application to various spacetime examples
Abstract
We give simple conditions implying the well-posedness of the Cauchy problem for the propagation of classical scalar fields in general (n+2)-dimensional static and spherically symmetric spacetimes. They are related to properties of the underlying spatial part of the wave operator, one of which being the standard essentially self-adjointness. However, in many examples the spatial part of the wave operator turns out to be not essentially selfadjoint, but it does satisfy a weaker property that we call here quasi essentially self-adjointness, which is enough to ensure the desired well-posedness. This is why we also characterize this second property. We state abstract results, then general results for a class of operators encompassing many examples in the literature, and we finish with the explicit analysis of some of them.
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