Axisymmetric constant mean curvature slices in the Kerr space-time
arXiv:1310.4699 · doi:10.1088/0264-9381/31/7/075017
Abstract
Recently, there have been efforts to solve Einstein's equation in the context of a conformal compactification of space-time. Of particular importance in this regard are the so called CMC-foliations, characterized by spatial hyperboloidal hypersurfaces with a constant extrinsic mean curvature K. However, although of interest for general space-times, CMC-slices are known explicitly only for the spherically symmetric Schwarzschild metric. This work is devoted to numerically determining axisymmetric CMC-slices within the Kerr solution. We construct such slices outside the black hole horizon through an appropriate coordinate transformation in which an unknown auxiliary function A is involved. The condition K=const. throughout the slice leads to a nonlinear partial differential equation for the function A, which is solved with a pseudo-spectral method. The results exhibit exponential convergence, as is to be expected in a pseudo-spectral scheme for analytic solutions. As a by-product, we identify CMC-slices of the Schwarzschild solution which are not spherically symmetric.
14 pages, 4 figures, Version published in CQG
References in corpus (6)
- Binary-black-hole initial data with nearly-extremal spins
- Regularity of the Einstein Equations at Future Null Infinity
- Gravitational perturbations of Schwarzschild spacetime at null infinity and the hyperboloidal initial value problem
- Tetrad formalism for numerical relativity on conformally compactified constant mean curvature hypersurfaces
- Black hole initial data on hyperboloidal slices
- The general spherically symmetric constant mean curvature foliations of the Schwarzschild solution
Cited by in corpus (9)
- Perturbing the perturbed: Stability of quasinormal modes in presence of a positive cosmological constant
- Hyperboloidal slicing approach to quasi-normal mode expansions: the Reissner-Nordström case
- Hyperboloidal framework for the Kerr spacetime
- Hyperboloidal approach for static spherically symmetric spacetimes: a didactical introduction and applications in black-hole physics
- Spherically symmetric black hole spacetimes on hyperboloidal slices
- Evolution of scalar fields surrounding black holes on compactified constant mean curvature hypersurfaces
- Slicing black hole spacetimes
- Hyperboloidal method for frequency-domain self-force calculations
- Hyperboloidal neutron star and black hole initial data in spherical symmetry