Probing the puncture for black hole simulations
J. David Brown

TL;DR
This paper investigates the behavior of perturbations near the puncture boundary in black hole simulations, demonstrating that no pathological reflections occur due to mode propagation differences, supported by numerical experiments.
Contribution
It clarifies how different perturbative modes propagate in puncture black hole simulations, explaining the absence of boundary reflections and improving understanding of numerical stability.
Findings
Perturbations in physical and conformal geometries propagate differently.
Modes in the physical geometry are directed away from the boundary.
Numerical experiments confirm the absence of pathological reflections.
Abstract
With the puncture method for black hole simulations, the second infinity of a wormhole geometry is compactified to a single "puncture point" on the computational grid. The region surrounding the puncture quickly evolves to a trumpet geometry. The computational grid covers only a portion of the trumpet throat. It ends at a boundary whose location depends on resolution. This raises the possibility that perturbations in the trumpet geometry could propagate down the trumpet throat, reflect from the puncture boundary, and return to the black hole exterior with a resolution--dependent time delay. Such pathological behavior is not observed. This is explained by the observation that some perturbative modes propagate in the conformal geometry, others propagate in the physical geometry. The puncture boundary exists only in the physical geometry. The modes that propagate in the physical geometry…
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