Bona-Masso slicing conditions and the lapse close to black-hole punctures
arXiv:2201.08857 · doi:10.1103/PhysRevD.105.064045
Abstract
We consider several families of functions that appear in the Bona-Masso slicing condition for the lapse function . 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 in terms of the areal radius . We then transform to isotropic coordinates and determine the dependence of on the isotropic radius in the vicinity of the black-hole puncture. We propose generalizations of previously considered functions for which, to leading order, the lapse is proportional to rather than a non-integer power of . We also perform dynamical simulations in spherical symmetry and demonstrate advantages of the above choices in numerical simulations employing spectral methods.
arXiv comment8 pages, 4 figures
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