Trumpet-puncture initial data for black holes
arXiv:0908.0337 · doi:10.1103/PhysRevD.80.061501
Abstract
We propose a new approach, based on the puncture method, to construct black hole initial data in the so-called trumpet geometry, i.e. on slices that asymptote to a limiting surface of non-zero areal radius. Our approach is easy to implement numerically and, at least for non-spinning black holes, does not require any internal boundary conditions. We present numerical results, obtained with a uniform-grid finite-difference code, for boosted black holes and binary black holes. We also comment on generalizations of this method for spinning black holes.
6 pages, 5 figures, published version
References in corpus (6)
- Binary-black-hole initial data with nearly-extremal spins
- Wormholes and trumpets: the Schwarzschild spacetime for the moving-puncture generation
- Analytical Representation of a Black Hole Puncture Solution
- Puncture Evolution of Schwarzschild Black Holes
- Extreme Bowen-York initial data
- Equilibrium initial data for moving puncture simulations: The stationary 1+log slicing