Conserved currents for a Kerr black hole and orthogonality of quasinormal modes
We introduce a bilinear form for Weyl scalar perturbations of Kerr. The form is symmetric and
conserved, and we show that, when combined with a suitable renormalization prescription …
conserved, and we show that, when combined with a suitable renormalization prescription …
Linear stability of slowly rotating Kerr black holes
We prove the linear stability of slowly rotating Kerr black holes as solutions of the Einstein
vacuum equations: linearized perturbations of a Kerr metric decay at an inverse polynomial …
vacuum equations: linearized perturbations of a Kerr metric decay at an inverse polynomial …
Teukolsky formalism for nonlinear Kerr perturbations
SR Green, S Hollands… - Classical and Quantum …, 2020 - iopscience.iop.org
We develop a formalism to treat higher order (nonlinear) metric perturbations of the Kerr
spacetime in a Teukolsky framework. We first show that solutions to the linearized Einstein …
spacetime in a Teukolsky framework. We first show that solutions to the linearized Einstein …
Gauge invariant perturbations of general spherically symmetric spacetimes
In this paper, the gauge choices in general spherically symmetric spacetimes are explored.
In particular, we construct the gauge invariant variables and the master equations for both …
In particular, we construct the gauge invariant variables and the master equations for both …
Conservative evolution of black hole perturbations with time-symmetric numerical methods
MF O'Boyle, C Markakis, LJG Da Silva… - arXiv preprint arXiv …, 2022 - arxiv.org
The scheduled launch of the LISA Mission in the next decade has called attention to the
gravitational self-force problem. Despite an extensive body of theoretical work, long-time …
gravitational self-force problem. Despite an extensive body of theoretical work, long-time …
Metric reconstruction in Kerr spacetime
S Hollands, V Toomani - Classical and Quantum Gravity, 2024 - iopscience.iop.org
Metric reconstruction is the general problem of parameterizing GR in terms of its two “true
degrees of freedom”, eg, by a complex scalar “potential”—in practice mostly with the aim of …
degrees of freedom”, eg, by a complex scalar “potential”—in practice mostly with the aim of …
Canonical quantization of Teukolsky fields on Kerr backgrounds
C Iuliano, J Zahn - Physical Review D, 2023 - APS
Electromagnetic and gravitational perturbations on Kerr spacetime can be reconstructed
from solutions to the Teukolsky equations. We study the canonical quantization of solutions …
from solutions to the Teukolsky equations. We study the canonical quantization of solutions …
Symmetries of linearized gravity from adjoint operators
S Aksteiner, T Bäckdahl - Journal of Mathematical Physics, 2019 - pubs.aip.org
Based on operator identities and their formal adjoints, we derive two symmetry operators for
the linearized Einstein operator on vacuum backgrounds of Petrov type D and, in particular …
the linearized Einstein operator on vacuum backgrounds of Petrov type D and, in particular …
Coercivity properties of the canonical energy in double null gauge on the 4-dimensional Schwarzschild exterior
SC Collingbourne - Classical and Quantum Gravity, 2023 - iopscience.iop.org
In this paper, we study the canonical energy associated with solutions to the linearised
vacuum Einstein equation on a stationary spacetime. The main result of this paper …
vacuum Einstein equation on a stationary spacetime. The main result of this paper …
Spin-2 Green's Functions on Kerr in Radiation Gauge
We construct retarded and advanced Green's functions for gravitational perturbations in Kerr
in an ingoing radiation gauge. Our Green's functions have a frequency domain piece that …
in an ingoing radiation gauge. Our Green's functions have a frequency domain piece that …