How to determine approximate Mixmaster parameters from numerical evolution of Einstein's equations
arXiv:gr-qc/9308016 · doi:10.1103/PhysRevD.49.1120
Abstract
To assess the validity of the Belinskii, Khalatnikov, and Lifshitz (BKL) approximation to Mixmaster dynamics, it would be useful to evaluate the BKL discrete parameters as a byproduct of the numerical solution of Einstein's equations. An algorithm to do this and results for a typical trajectory are presented.
11 pages in revtex
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