Global structure of bigravity solutions
Diego Blas, Cedric Deffayet, Jaume Garriga

TL;DR
This paper analyzes the causal structure and maximal extensions of static, spherically symmetric bigravity solutions, revealing complex global properties and conditions for causality preservation.
Contribution
It classifies bigravity solutions into types, provides maximal extensions, and discusses their causal and global properties, including non-globally hyperbolic features.
Findings
Causality is preserved despite different light-cone structures.
Maximal extensions can contain multiple copies of individual geometries.
Most solutions are not globally hyperbolic, even when individual metrics are.
Abstract
We discuss the causal diagrams of static and spherically symmetric bigravity vacuum solutions, with interacting metrics and . Such solutions can be classified into type I (or "non-diagonal") and type II (or "diagonal"). The general solution of type I is known, and leads to metrics and in the Schwarzschild-(Anti)de Sitter family. The two metrics are not always diagonalizable in the same coordinate system, and the light-cone structure of both metrics can be quite different. In spite of this, we find that causality is preserved, in the sense that closed time-like curves cannot be pieced together from geodesics of both metrics. We propose maximal extensions of Type I bigravity solutions, where geodesics of both metrics do not stop unless a curvature singularity is encountered. Such maximal extensions can contain several copies (or even an infinite number of them) of the…
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