On causality violation on a Kerr-de Sitter spacetime
Thomas Zannias

TL;DR
This paper investigates the causal structure of Kerr-de Sitter spacetimes, revealing that they are generally well-behaved causally except near singularities, and that a positive cosmological constant improves their causal properties.
Contribution
It provides a detailed analysis of the causal properties of Kerr-de Sitter spacetimes, comparing them to Kerr spacetimes, and shows how the cosmological constant affects causality.
Findings
Carter's blocks are mostly stably causal except near singularities.
Kerr-de Sitter spacetime's asymptotic region is causally well-behaved.
Positive cosmological constant improves causal behavior.
Abstract
The causal properties of the family of Kerr-de Sitter spacetimes are analyzed and compared to those of the Kerr family. At first we show that a Kerr-de Sitter spacetime can be viewed as an assembly of Carter's blocks i.e. four dimensional spacetime regions contained within Killing horizons or a Killing horizon and the asymptotic de Sitter region. From this perspective and leaving aside topological identifications, the causal properties of a Kerr de Sitter spacetime are determined by the causal properties of the individual Carter's blocks viewed as spacetimes in their own right. We show that any Carter's block is stably causal except for the blocks that contain the ring singularity. The latter are vicious sets: any two events within such block can be connected by a future (respectively past) directed timelike curve. This behavior is identical to the causal behavior of the Boyer-Lindquist…
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