arXiv · 2201.08857
Bona-Masso slicing conditions and the lapse close to black-hole punctures
Abstract
We consider several families of functions $f(\alpha)$ that appear in the Bona-Masso slicing condition for the lapse function $\alpha$. Focusing on spherically symmetric and time-independent slices we apply these conditions to the Schwarzschild spacetime in order to construct analytical expressions for the lapse $\alpha$ in terms of the areal radius $R$. We then transform to isotropic coordinates and determine the dependence of $\alpha$ on the isotropic radius $r$ in the vicinity of the black-hole puncture. We propose generalizations of previously considered functions $f(\alpha)$ for which, to leading order, the lapse is proportional to $r$ rather than a non-integer power of $r$. We also perform dynamical simulations in spherical symmetry and demonstrate advantages of the above choices in numerical simulations employing spectral methods.
Explore related subjects
Keep this discovery
Thomas W. Baumgarte, Henrique P. de Oliveira. 2022-01-21. Bona-Masso slicing conditions and the lapse close to black-hole punctures. https://doi.org/10.1103/physrevd.105.064045
Cite the original work for its findings. Save a collection to share your selection of sources.