Numerical solutions to Einstein's equations in a shearing-dust universe: a code comparison
Abstract
A number of codes for general-relativistic simulations of cosmological structure formation have been developed in recent years. Here we demonstrate that a sample of these codes produce consistent results beyond the Newtonian regime. We simulate solutions to Einstein's equations dominated by gravitomagnetism-a vector-type gravitational field that does not exist in Newtonian gravity and produces frame-dragging, the leading-order post-Newtonian effect. We calculate the coordinate-invariant effect on intersecting null geodesics by performing ray tracing in each independent code. With this observable quantity, we assess and compare each code's ability to compute relativistic effects.
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Título según WOS: | ID WOS:000553695900001 Not found in local WOS DB |
Título de la Revista: | CLASSICAL AND QUANTUM GRAVITY |
Volumen: | 37 |
Número: | 15 |
Editorial: | IOP PUBLISHING LTD |
Fecha de publicación: | 2020 |
DOI: |
10.1088/1361-6382/ab939b |
Notas: | ISI |