Gauge Invariant Perturbations of General Spherically Symmetric Spacetimes
arXiv:2201.01259 · doi:10.1007/s11433-022-1956-4
Abstract
In this paper, the gauge choices in general spherically symmetric spacetimes have been explored. We construct the gauge invariant variables and the master equations for both the Detweiler easy gauge and the Regge-Wheeler gauge, respectively. The particular cases for are also been investigated. Our results provide analytical calculations of metric perturbation in general spherically symmetric spacetimes, which can be applied to various cases, including the Effective-One-Body problem. A simple example is presented to show how the metric perturbation components are related to the source perturbation terms.
27 pages, Accepted for publication in Sci. China, Phys. Mech. Astron
References in corpus (9)
- Gravitational scattering, post-Minkowskian approximation and Effective One-Body theory
- Modified theories of Gravity: Why, How and What?
- Gravitational spin-orbit coupling in binary systems, post-Minkowskian approximation and effective one-body theory
- Master Equations for Gravitational Perturbations of Static Lovelock Black Holes in Higher Dimensions
- Stability of Lovelock Black Holes under Tensor Perturbations
- Perturbations and quasi-normal modes of black holes with time-dependent scalar hair in shift-symmetric scalar-tensor theories
- A light-cone gauge for black-hole perturbation theory
- Self-consistent Effective-one-body theory for spinless binaries based on post-Minkowskian approximation I: Hamiltonian and decoupled equation for
- Master Functions and Equations for Perturbations of Vacuum Spherically-Symmetric Spacetimes
Cited by in corpus (20)
- Light rings and shadows of static black holes in effective quantum gravity
- Static neutral black holes in Kalb-Ramond gravity
- Quasinormal modes and greybody factor of a Lorentz-violating black hole
- Hyperboloidal approach for static spherically symmetric spacetimes: a didactical introduction and applications in black-hole physics
- Kerr-MOG-(A)dS black hole and its shadow in scalar-tensor-vector gravity theory
- Shadow of slowly rotating Kalb-Ramond black holes
- Lorentz violation induces isospectrality breaking in Einstein-Bumblebee gravity theory
- Self-consistent effective-one-body theory for spinning binaries based on post-Minkowskian approximation
- The Axial Gravitational Ringing of a Spherically Symmetric Black Hole Surrounded by Dark Matter Spike
- Gravito-electromagnetic perturbations of MOG black holes with a cosmological constant: Quasinormal modes and Ringdown waveforms
- Determination of the spin parameter and the inclination angle by the relativistic images in black hole image
- Influence of dark matter equation of state on the axial gravitational ringing of supermassive black holes
- The ring-shaped shadow of rotating naked singularity with a complete photon sphere
- Lorentz violation signatures in the low-energy sector of Hořava gravity from black hole shadow observations
- Strong gravitational lensing of rotating regular black holes in non-minimally coupled Einstein-Yang-Mills theory
- Parameterized quasinormal frequencies and Hawking radiation for axial gravitational perturbations of a holonomy-corrected black hole
- The Quasinormal Modes and Isospectrality of Bardeen (Anti-) de Sitter Black Holes
- Energy flux and waveform of gravitational wave generated by coalescing slow-spinning binary system in effective one-body theory
- Even-parity stability of hairy black holes in gauge-invariant scalar-vector-tensor theories
- Linear instability of hairy black holes in Horndeski theory