Constructing hyperbolic systems in the Ashtekar formulation of general relativity
arXiv:gr-qc/9901053 · doi:10.1142/S0218271800000037
Abstract
Hyperbolic formulations of the equations of motion are essential technique for proving the well-posedness of the Cauchy problem of a system, and are also helpful for implementing stable long time evolution in numerical applications. We, here, present three kinds of hyperbolic systems in the Ashtekar formulation of general relativity for Lorentzian vacuum spacetime. We exhibit several (I) weakly hyperbolic, (II) diagonalizable hyperbolic, and (III) symmetric hyperbolic systems, with each their eigenvalues. We demonstrate that Ashtekar's original equations form a weakly hyperbolic system. We discuss how gauge conditions and reality conditions are constrained during each step toward constructing a symmetric hyperbolic system.
15 pages, RevTeX, minor changes in Introduction. published as Int. J. Mod. Phys. D 9 (2000) 13
References in corpus (5)
- Comparison of 32-site exact diagonalization results and ARPES spectral functions for the AFM insulator
- Numerical Evolution of Black Holes with a Hyperbolic Formulation of General Relativity
- Symmetric hyperbolic system in the Ashtekar formulation
- Einstein's equations in Ashtekar's variables constitute a symmetric hyperbolic system
- A trick for passing degenerate points in Ashtekar formulation
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