Corrections to the Aretakis type behaviour of the metric due to an infalling particle
arXiv:1811.01371 · doi:10.1103/PhysRevD.99.044018
Abstract
We consider an extremal Reissner-Nordström black hole perturbed by a neutral massive point particle, which falls in radially. We study the linear metric perturbation in the vicinity of the black hole and find that the and spherical modes of the metric oscillate rather than decay.
arXiv comment7 pages, title is changed, clarifications are added
References in corpus (18)
- Soft Hair on Black Holes
- The Extreme Kerr Throat Geometry: A Vacuum Analog of AdS_2 x S^2
- Near-horizon symmetries of extremal black holes
- Supertranslations and Superrotations at the Black Hole Horizon
- Classification of near-horizon geometries of extremal black holes
- Stability and Instability of Extreme Reissner-Nordström Black Hole Spacetimes for Linear Scalar Perturbations I
- Stability and Instability of Extreme Reissner-Nordström Black Hole Spacetimes for Linear Scalar Perturbations II
- Extended Symmetries at the Black Hole Horizon
- On the horizon instability of an extreme Reissner-Nordström black hole
- Perturbations of near-horizon geometries and instabilities of Myers-Perry black holes
- Gravity Waves from Extreme-Mass-Ratio Plunges into Kerr Black Holes
- Horizon Instability of Extremal Kerr Black Holes: Nonaxisymmetric Modes and Enhanced Growth Rate
- Fast plunges into Kerr black holes
- Horizon instability of extremal Reissner-Nordström black holes to charged perturbations
- Symmetries at the black hole horizon
- Whirling orbits around twirling black holes from conformal symmetry
- Exact Gravitational Wave Signatures from Colliding Extreme Black Holes
- Lectures on General Theory of Relativity