The Periodic Standing-Wave Approximation: Overview and Three Dimensional Scalar Models
arXiv:gr-qc/0310001 · doi:10.1103/PhysRevD.70.064001
Abstract
The periodic standing-wave method for binary inspiral computes the exact numerical solution for periodic binary motion with standing gravitational waves, and uses it as an approximation to slow binary inspiral with outgoing waves. Important features of this method presented here are: (i) the mathematical nature of the ``mixed'' partial differential equations to be solved, (ii) the meaning of standing waves in the method, (iii) computational difficulties, and (iv) the ``effective linearity'' that ultimately justifies the approximation. The method is applied to three dimensional nonlinear scalar model problems, and the numerical results are used to demonstrate extraction of the outgoing solution from the standing-wave solution, and the role of effective linearity.
arXiv comment13 pages RevTeX, 5 figures. New version. A revised form of the nonlinearity produces better results
References in corpus (10)
- Generic Isolated Horizons and their Applications
- A Catalog of Candidate Intermediate-luminosity X-ray Objects
- Modeling gravitational radiation from coalescing binary black holes
- Thermodynamics of binary black holes and neutron stars
- Improved numerical stability of stationary black hole evolution calculations
- Periodic Solutions of the Einstein Equations for Binary Systems
- Toward stable 3D numerical evolutions of black-hole spacetimes
- Quasi-stationary binary inspiral II: Radiation-balanced boundary conditions
- Radiation-balanced simulations for binary inspiral
- The Helically-Reduced Wave Equation as a Symmetric-Positive System
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