Abstract
AbstractWe discuss and implement a spectral method approach to computing stationary and axisymmetric black hole solutions and their properties in modified theories of gravity. The resulting code is written in theJulialanguage and is transparent and easily adapted to new settings. We test the code on both general relativity and on Einstein-scalar-Gauss–Bonnet gravity. It is accurate and fast, converging on a spinning solution in these theories with tiny errors (in most cases) in a matter of seconds.
Subject
Physics and Astronomy (miscellaneous)
Cited by
5 articles.
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