Hyperboloidal data and evolution
arXiv:gr-qc/0512033 · doi:10.1063/1.2218186
Abstract
We discuss the hyperboloidal evolution problem in general relativity from a numerical perspective, and present some new results. Families of initial data which are the hyperboloidal analogue of Brill waves are constructed numerically, and a systematic search for apparent horizons is performed. Schwarzschild-Kruskal spacetime is discussed as a first application of Friedrich's general conformal field equations in spherical symmetry, and the Maxwell equations are discussed on a nontrivial background as a toy model for continuum instabilities.
11 pages, 9 figures. To appear in the Proceedings of the Spanish Relativity Meeting (ERE 2005), Oviedo, Spain, 6-10 Sept 2005
References in corpus (1)
Cited by in corpus (20)
- Calibration of Moving Puncture Simulations
- Hyperboloidal foliations and scri-fixing
- Continuum and Discrete Initial-Boundary-Value Problems and Einstein's Field Equations
- Hyperboloidal evolution with the Einstein equations
- Implementation of standard testbeds for numerical relativity
- Spacelike matching to null infinity
- Gravitational perturbations of Schwarzschild spacetime at null infinity and the hyperboloidal initial value problem
- Improved outer boundary conditions for Einstein's field equations
- Towards absorbing outer boundaries in General Relativity
- Spherical symmetry as a test case for unconstrained hyperboloidal evolution
- A hyperboloidal study of tail decay rates for scalar and Yang-Mills fields
- Spectral Cauchy-characteristic extraction of the gravitational wave news function
- Hyperboloidal evolution of test fields in three spatial dimensions
- Spherical symmetry as a test case for unconstrained hyperboloidal evolution II: gauge conditions
- Stationary hyperboloidal slicings with evolved gauge conditions
- Axisymmetric constant mean curvature slices in the Kerr space-time
- Asymptotics and singularities in cosmological models with positive cosmological constant
- Bondi-Sachs Energy-Momentum for the CMC Initial Value Problem
- Numerical calculations near spatial infinity
- Global versus Local Aspects of Critical Collapse