TL;DR
The paper introduces _AHFinderDirect_, a highly efficient and accurate apparent horizon finder for 3D numerical relativity simulations, capable of locating horizons within seconds at typical resolutions.
Contribution
It presents a novel fast apparent horizon finder that uses a star-shaped parameterization and Newton's method, significantly reducing computation time compared to existing methods.
Findings
Finds apparent horizons in a few seconds at typical resolutions.
Achieves approximately 10^{-5} m accuracy.
Implemented as a freely available Cactus thorn.
Abstract
In 3+1 numerical simulations of dynamic black hole spacetimes, it's useful to be able to find the apparent horizon(s) (AH) in each slice of a time evolution. A number of AH finders are available, but they often take many minutes to run, so they're too slow to be practically usable at each time step. Here I present a new AH finder,_AHFinderDirect_, which is very fast and accurate: at typical resolutions it takes only a few seconds to find an AH to accuracy on a GHz-class processor. I assume that an AH to be searched for is a Strahlk\"orper (star-shaped region) with respect to some local origin, and so parameterize the AH shape by for some single-valued function . The AH equation then becomes a nonlinear elliptic PDE in on , whose coefficients are algebraic functions of , , and the Cartesian-coordinate spatial…
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