Year: 2025
Type: article
Abstract: Rapidly rotating black-hole spacetimes outside general relativity are key to many tests of Einstein's theory. We here develop an efficient spectral method to represent such spacetimes analytically, in closed-form, and to high accuracy, in a large class of effective-field-theory extensions of general relativity. We exemplify this method by constructing, for the first time, closed-form and analytic representations of spinning black holes in scalar-Gauss-Bonnet, dynamical Chern-Simons, and axidilaton gravity to an accuracy better than 10^{-8} for all dimensionless spins below 0.99.
Source: Physical Review Letters
DOI: 10.1103/6z43-xdv7
Authors: Kelvin Ka-Ho Lam, Adrian Ka-Wai Chung, Nicolás Yunes
Institution: University of Illinois Urbana-Champaign
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: green
OpenAlex ID: W4417210777
