Understand
We present the first numerical code based on the Galerkin and Collocation methods to integrate the field equations of the Bondi problem.
- The Galerkin method like all spectral methods provide high accuracy with moderate computational effort.
- Several numerical tests were performed to verify the issues of convergence, stability and accuracy with promising results.
- This code opens up several possibilities of applications in more general scenarios for studying the evolution of spacetimes with gravitational waves.
Built on
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Similar
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1989
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1993
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R. Gómez, P. Papadopoulos, and J. Winicour, J. Math. Phys., 35
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D. Gottlieb and S. A. Orszag, Numerical Analysis of Spectral Methods: Theory and Applications
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P. Holmes, John L. Lumley and Gal Berkooz, Turbulence, Coherent Structures, Dynamical Systems and Symmetry
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S. Bonazzola, E. Gourgoulhon and J. A. Mark, Spectral Methods in General Relativistic Astrophysics
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C. Canuto, M. Y. Hussaini, A. Quarteroni and T. A. Zang, Spectral Methods in Fluid Dynamics
2001
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J. Boyd, Chebyshev and Fourier spectral methods
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F. Siebel, Simulation of axisymmetric flows in the characteristic formulation of general relativity
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Jeffrey Winicour, Characteristic Evolution and Matching
2005
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R. Gómez, W. Barreto and S. Frittelli, A framework for large-scale relativistic simulations in the characteristic approach
2007
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