On Axially Symmetric Perturbations of Kerr Black Hole Spacetimes

TL;DR

This paper establishes a positive-definite, conserved energy functional for axially symmetric linear perturbations of Kerr black holes, providing a significant step towards proving their linear stability.

Contribution

It constructs a gauge-invariant, positive-definite energy functional for Kerr perturbations and proves its strict conservation over time, advancing stability analysis.

Findings

Existence of a positive-definite, conserved energy for Kerr perturbations

Boundary terms vanish dynamically, ensuring energy conservation

Supports the linear stability of Kerr black hole exteriors

Abstract

The lack of a positive-definite and conserved energy is a serious obstacle in the black hole stability problem. In this work, we will show that there exists a positive-definite and conserved Hamiltonian energy for axially symmetric linear perturbations of the exterior of Kerr black hole spacetimes. In the first part, based on the Hamiltonian dimensional reduction of 3+1 axially symmetric, Ricci-flat Lorentzian spacetimes to a 2+1 Einstein-wave map system with the negatively curved hyperbolic 2-plane target, we construct a positive-definite, spacetime gauge-invariant energy functional for linear axially symmetric perturbations in the exterior of Kerr black holes, in a manner that is also gauge-independent on the target manifold. In the construction of the positive-definite energy, various dynamical terms at the boundary of the orbit space occur critically. In the second part, after setting up the initial value problem in harmonic coordinates, we prove that the positive energy for the axially symmetric linear perturbative theory of Kerr black holes is strictly conserved in time, by establishing that all the boundary terms dynamically vanish for all times. This result implies a form of dynamical linear stability of the exterior of Kerr black hole spacetimes.