Table of Contents
Fetching ...

Doubly Separable Spacetimes and Symmetry Constraints on their Self-Gravitating Matter Content

Prashant Kocherlakota, Ramesh Narayan

TL;DR

The work analyzes a Newman–Janis–Azreg-Aïnou–type solution-generating approach, showing that the ACKN construction yields the KSZ metric, a spacetime class that is geodesically and scalar-wave separable (doubly separable). It demonstrates that only Kerr–Newman-type electromagnetic fields can source such spacetimes (with a Killing tensor enabling geodesic and scalar separability, and a Killing–Yano tensor only in a degenerate subfamily), while massless scalars and perfect fluids cannot source these highly symmetric configurations. The analysis clarifies the precise relations among ACKN, KSZ, and Johannsen metrics, and proves that spinning JNW/MKS solutions lie outside this class, emphasizing conditions under which solution-generating techniques yield physically viable interiors and exteriors. Overall, the results reveal a tight link between spacetime symmetry, matter content, and the viability of exact, self-consistent spinning solutions in general relativity, guiding future interior–exterior matching and model-building efforts.

Abstract

A popular approach to constructing exact stationary and axisymmetric nonvacuum solutions in general relativity has been to use solution-generating techniques. Here we revisit a recent variant of the Newman-Janis-Azreg-Ainou algorithm - restricted to asymptotically-flat spacetimes - and demonstrate that this method exclusively generates Konoplya-Stuchlik-Zhidenko spacetimes. Therefore, the equations for geodesic motion and scalar-wave propagation are both separable. We call these "doubly separable" spacetimes. Of these, we identify a "degenerate" subclass that might admit a separable Dirac equation by explicitly obtaining the Killing-Yano tensor. While the degenerate subclass is Petrov Type D, the general doubly separable spacetimes are of Type I. The high degree of symmetry in these spacetimes suggests that the self-gravitating matter must also be in specialized field configurations. For this reason, we investigate whether these spacetimes can even be sourced by arbitrary types of matter. We show that doubly separable spacetimes cannot be sourced by massless real scalar fields or by perfect fluids, and that electromagnetic fields lead only to the Kerr-Newman family. Notably, this rules out the correct spinning counterpart of the Janis-Newman-Winicour naked singularity spacetimes, which contains a scalar field, as a member of this metric class. While the algorithm generates spacetimes with rich symmetry structures, valuable for studying phenomena like black hole shadows and quasinormal modes, our results highlight the need for caution when using it to construct physically consistent solutions with prespecified matter content.

Doubly Separable Spacetimes and Symmetry Constraints on their Self-Gravitating Matter Content

TL;DR

The work analyzes a Newman–Janis–Azreg-Aïnou–type solution-generating approach, showing that the ACKN construction yields the KSZ metric, a spacetime class that is geodesically and scalar-wave separable (doubly separable). It demonstrates that only Kerr–Newman-type electromagnetic fields can source such spacetimes (with a Killing tensor enabling geodesic and scalar separability, and a Killing–Yano tensor only in a degenerate subfamily), while massless scalars and perfect fluids cannot source these highly symmetric configurations. The analysis clarifies the precise relations among ACKN, KSZ, and Johannsen metrics, and proves that spinning JNW/MKS solutions lie outside this class, emphasizing conditions under which solution-generating techniques yield physically viable interiors and exteriors. Overall, the results reveal a tight link between spacetime symmetry, matter content, and the viability of exact, self-consistent spinning solutions in general relativity, guiding future interior–exterior matching and model-building efforts.

Abstract

A popular approach to constructing exact stationary and axisymmetric nonvacuum solutions in general relativity has been to use solution-generating techniques. Here we revisit a recent variant of the Newman-Janis-Azreg-Ainou algorithm - restricted to asymptotically-flat spacetimes - and demonstrate that this method exclusively generates Konoplya-Stuchlik-Zhidenko spacetimes. Therefore, the equations for geodesic motion and scalar-wave propagation are both separable. We call these "doubly separable" spacetimes. Of these, we identify a "degenerate" subclass that might admit a separable Dirac equation by explicitly obtaining the Killing-Yano tensor. While the degenerate subclass is Petrov Type D, the general doubly separable spacetimes are of Type I. The high degree of symmetry in these spacetimes suggests that the self-gravitating matter must also be in specialized field configurations. For this reason, we investigate whether these spacetimes can even be sourced by arbitrary types of matter. We show that doubly separable spacetimes cannot be sourced by massless real scalar fields or by perfect fluids, and that electromagnetic fields lead only to the Kerr-Newman family. Notably, this rules out the correct spinning counterpart of the Janis-Newman-Winicour naked singularity spacetimes, which contains a scalar field, as a member of this metric class. While the algorithm generates spacetimes with rich symmetry structures, valuable for studying phenomena like black hole shadows and quasinormal modes, our results highlight the need for caution when using it to construct physically consistent solutions with prespecified matter content.

Paper Structure

This paper contains 26 sections, 111 equations, 1 figure, 1 table.

Figures (1)

  • Figure 1: A Venn diagram for a pictoral representation of the relations between the various metrics discussed in this paper. Included here are the Konoplya-Rezzolla-Zhidenko (KRZ), the Johannsen, the Konoplya-Stuchlík-Zhidenko (KSZ), and the Azreg-Aïnou-Chen-Kocherlakota-Narayan (ACKN) metric families. The Azreg-Aïnou (AA) metric family is not shown, as its relation to the other spacetimes is not fully understood. However, the AA metric and the ACKN metric family have the Quasi-degenerate ($R=r, g=r^2/(r^2+r_0^2)$) and a strange family of nonspinning and axisymmetric spacetimes ($R=r, f=1$) in common, as discussed in Sec. \ref{['sec:SecIC-AA-Metric']} and Sec. \ref{['sec:SecIIB-Rigid-Rotation']}. The Johannsen spacetimes admit a Killing tensor due to the separability of the geodesic equation. Only the subclass of ACKN/KSZ spacetimes also admit a separable scalar-wave equation. Of these, the degenerate ACKN/KSZ spacetimes admit a Killing-Yano tensor and, therefore, likely also a separable Dirac equation (Sec. \ref{['sec:SecIG-Killing']}). The ACKN/KSZ spacetimes are in general of Petrov Type I but the subclass of degenerate spacetimes are of Type D (Sec. \ref{['sec:SecIH-Petrov']}). Shown also are the Kerr-Newman (KN) and the Kerr-Sen (KS) solution families. Finally, the Kerr metric is shown in red shading and the star represents the Minkwoski spacetime. The sizes of the shapes hold no meaning.