We present a flexible, non-conforming staggered-grid Chebyshev spectral multidomain method for the solution of the compressible Navier-Stokes equations. In this method, subdomain corners are not included in the approximation, thereby simplifying the subdomain connectivity. To allow for local refinem
Multidomain spectral method for the helically reduced wave equation
β Scribed by Stephen R. Lau; Richard H. Price
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 995 KB
- Volume
- 227
- Category
- Article
- ISSN
- 0021-9991
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β¦ Synopsis
We consider the 2+1 and 3+1 scalar wave equations reduced via a helical Killing field, respectively referred to as the 2-dimensional and 3-dimensional helically reduced wave equation (HRWE). The HRWE serves as the fundamental model for the mixed-type PDE arising in the periodic standing wave (PSW) approximation to binary inspiral. We present a method for solving the equation based on domain decomposition and spectral approximation. Beyond describing such a numerical method for solving strictly linear HRWE, we also present results for a nonlinear scalar model of binary inspiral. The PSW approximation has already been theoretically and numerically studied in the context of the post-Minkowskian gravitational field, with numerical simulations carried out via the ''eigenspectral method.'' Despite its name, the eigenspectral technique does feature a finite-difference component, and is lower-order accurate. We intend to apply the numerical method described here to the theoretically well-developed post-Minkowski PSW formalism with the twin goals of spectral accuracy and the coordinate flexibility afforded by global spectral interpolation.
π SIMILAR VOLUMES
An application of the spectral multidomain method to the twodimensional, time-dependent, incompressible Navier-Stokes equations is presented. The governing equations are discretized on a nonstaggered, stretched mesh with a mixed finite difference/Chebyshev method and are integrated by a time-splitti
We present a spectral method for solving elliptic equations which arise in general relativity, namely three-dimensional scalar Poisson equations, as well as generalized vectorial Poisson equations of the type N + Ξ» β( β β’ N) = S with Ξ» = -1. The source can extend in all the Euclidean space R 3 , pro