Avenues for Analytic exploration in Axisymmetric Spacetimes. Foundations and the Triad Formalism

TL;DR

This paper reviews the reduction of axisymmetric vacuum Einstein equations to a concise form using a triad formalism, explores solution spaces, and simplifies equations for static and twist-free cases with applications to null infinity.

Contribution

It introduces two novel triad choices that simplify the Einstein equations in axisymmetric spacetimes and analyzes their hierarchical structure and solution space.

Findings

Explicit solutions for static axisymmetric spacetimes.

Identification of conditions for physical solutions.

Simplification of equations using harmonic and null coordinate adapted triads.

Abstract

Axially symmetric spacetimes are the only models for isolated systems with continuous symmetries that also include dynamics. For such systems, we review the reduction of the vacuum Einstein field equations to their most concise form by dimensionally reducing to the three-dimensional space of orbits of the Killing vector, followed by a conformal rescaling. The resulting field equations can be written as a problem in three-dimensional gravity with a complex scalar field as source. This scalar field, the Ernst potential is constructed from the norm and twist of the spacelike Killing field. In the case where the axial Killing vector is twist-free, we discuss the properties of the axis and simplify the field equations using a triad formalism. We study two physically motivated triad choices that further reduce the complexity of the equations and exhibit their hierarchical structure. The first choice is adapted to a harmonic coordinate that asymptotes to a cylindrical radius and leads to a simplification of the three-dimensional Ricci tensor and the boundary conditions on the axis. We illustrate its properties by explicitly solving the field equations in the case of static axisymmetric spacetimes. The other choice of triad is based on geodesic null coordinates adapted to null infinity as in the Bondi formalism. We then explore the solution space of the twist-free axisymmetric vacuum field equations, identifying the known (unphysical) solutions together with the assumptions made in each case. This singles out the necessary conditions for obtaining physical solutions to the equations.