Radiative falloff in the background of rotating black hole

Abstract

We study numerically the late-time tails of linearized fields with any spin $s$ in the background of a spinning black hole. Our code is based on the ingoing Kerr coordinates, which allow us to penetrate through the event horizon. The late time tails are dominated by the mode with the least multipole moment $\ell$ which is consistent with the equatorial symmetry of the initial data and is equal to or greater than the least radiative mode with $s$ and the azimuthal number $m$.

5 pages, 4 Encapsulated PostScript figures; Accepted to Phys. Rev. D (Rapid Communication)

References in corpus (2)

• Radiative falloff of a scalar field in a weakly curved spacetime without symmetries
• Evolution of Kerr-Schild type initial data for binary black holes using the horizon penetrating Teukolsky equation

Cited by in corpus (29)

• Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion
• Absorption of mass and angular momentum by a black hole: Time-domain formalisms for gravitational perturbations, and the small-hole/slow-motion approximation
• Gravitational radiation reaction and inspiral waveforms in the adiabatic limit
• Computing inspirals in Kerr in the adiabatic regime. I. The scalar case
• Multi-block simulations in general relativity: high order discretizations, numerical stability, and applications
• Universality of massive scalar field late-time tails in black-hole spacetimes
• Numerical solution of the 2+1 Teukolsky equation on a hyperboloidal and horizon penetrating foliation of Kerr and application to late-time decays
• Late time tails in the Kerr spacetime
• 3D simulations of linearized scalar fields in Kerr spacetime
• High accuracy simulations of Kerr tails: coordinate dependence and higher multipoles
• Intermediate behavior of Kerr tails
• Wave dynamics of a six-dimensional black hole localized on a tensional three-brane
• Mode coupling mechanism for late-time Kerr tails
• Dynamical evolution of a scalar field coupling to Einstein's tensor in the Reissner-Nordström black hole spacetime
• Late-time Kerr tails revisited
• Late-time evolution of charged massive Dirac fields in the Kerr-Newman background
• Dynamical evolution of the electromagnetic perturbation with Weyl corrections
• Late-time Kerr tails: generic and non-generic initial data sets, "up" modes, and superposition
• Radiation tails and boundary conditions for black hole evolutions
• Phenomenology and origin of late-time tails in eccentric binary black hole mergers
• Late-time tail of a coupled scalar field in the background of a black hole with a global monopole
• The late-time tails in the Reissner-Nordström spacetime revisited
• Late-time tails in nonlinear evolutions of merging black holes
• Quasinormal modes and late-time tails in the background of Schwarzschild black hole pierced by a cosmic string: scalar, electromagnetic and gravitational perturbations
• High-Precision Numerical Simulations of Rotating Black Holes Accelerated by CUDA
• Dynamical evolution of phantom scalar perturbation in the background of Schwarzschild black String spacetime
• Comment on "High-order contamination in the tail of gravitational collapse''
• Analysis of late-time tails in spin-aligned eccentric binary black hole mergers
• Numerical computation of electromagnetically sourced nonlinear tails