September 25, 2000

Apparent horizon finder for general three-dimensional spaces

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Resumen

We present a numerical method for finding the apparent horizon in general three-dimensional (3D) spaces without any symmetries for 3D numerical relativity. We apply this method for black hole spacetimes to demonstrate its quick convergence to solutions and reasonable accuracy.

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Shibata et al. (Mon,) studied this question.

synapsesocial.com/papers/6a202dabf40cfd3fe2294779 https://doi.org/https://doi.org/10.1103/physrevd.62.087501

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