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Автор Carsten Gundlach
Автор Paul Walker
Дата выпуска 1999-03-01
dc.description We give a general scheme for finite-differencing partial differential equations in flux-conservative form to second order, with a stencil that can be arbitrarily tilted with respect to the numerical grid, parametrized by a `tilt' vector field . This can be used to centre the numerical stencil on the physical lightcone, by setting , where is the usual shift vector in the 3 + 1 split of spacetime, but other choices of the tilt may also be useful. We apply this `causal differencing' algorithm to the Bona-Massó equations, a hyperbolic and flux-conservative form of the Einstein equations, and demonstrate long-term stable causally correct evolutions of single black hole systems in spherical symmetry.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Causal differencing of flux-conservative equations applied to black hole spacetimes
Тип paper
DOI 10.1088/0264-9381/16/3/026
Electronic ISSN 1361-6382
Print ISSN 0264-9381
Журнал Classical and Quantum Gravity
Том 16
Первая страница 991
Последняя страница 1010
Аффилиация Carsten Gundlach; Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Schlaatzweg 1, 14473 Potsdam, Germany
Аффилиация Paul Walker; Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Schlaatzweg 1, 14473 Potsdam, Germany
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