On the global structure of the Pomeransky-Senkov black holes
Piotr T. Chru\'sciel, Julien Cortier, Alfonso Garc\'ia-Parrado, G\'omez-Lobo

TL;DR
This paper constructs and analyzes extended Pomeransky-Senkov black hole solutions, revealing their global structure, horizon properties, and singularity topology, with numerical evidence supporting stable causality.
Contribution
It provides new analytic extensions of Pomeransky-Senkov metrics, clarifies the nature of singularities and horizons, and explores the global topology and causality properties.
Findings
Singularities lie beyond event horizons.
The topology of the singular set depends on parameters.
Numerical evidence suggests stable causality in the domain of outer communications.
Abstract
We construct analytic extensions of the Pomeransky-Senkov metrics with multiple Killing horizons and asymptotic regions. We show that, in our extensions, the singularities associated to an obstruction to differentiability of the metric lie beyond event horizons. We analyze the topology of the non-empty singular set, which turns out to be parameter-dependent. We present numerical evidence for stable causality of the domain of outer communications. The resulting global structure is somewhat reminiscent of that of Kerr space-time.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Advanced Differential Geometry Research
