Binary Black Hole Waveform Extraction at Null Infinity
arXiv:1106.4841 · doi:10.1088/0264-9381/28/13/134006
Abstract
In this work, we present a work in progress towards an efficient and economical computational module which interfaces between Cauchy and characteristic evolution codes. Our goal is to provide a standardized waveform extraction tool for the numerical relativity community which will allow CCE to be readily applied to a generic Cauchy code. The tool provides a means of unambiguous comparison between the waveforms generated by evolution codes based upon different formulations of the Einstein equations and different numerical approximation.
11 pages, 7 figures
References in corpus (3)
Cited by in corpus (17)
- Extraction of Gravitational Waves in Numerical Relativity
- Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms
- Null infinity waveforms from extreme-mass-ratio inspirals in Kerr spacetime
- Binary black hole coalescence in the large-mass-ratio limit: the hyperboloidal layer method and waveforms at null infinity
- Improved Cauchy-characteristic evolution system for high-precision numerical relativity waveforms
- General relativistic null-cone evolutions with a high-order scheme
- Fully relativistic three-dimensional Cauchy-characteristic matching for physical degrees of freedom
- Gravitational waves in dynamical spacetimes with matter content in the Fully Constrained Formulation
- The affine-null metric formulation of Einstein's equations
- A note on gravitational wave extraction from binary simulations
- Spherically symmetric black hole spacetimes on hyperboloidal slices
- Gauge structure of the Einstein field equations in Bondi-like coordinates
- Merging black holes with Cauchy-characteristic matching: Computation of late-time tails
- Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations
- Where is the ringdown? Reconstructing quasinormal modes from dispersive waves
- The gravitational wave strain in the characteristic formalism of numerical relativity
- The Bondi problem revisited: a spectral domain decomposition code