https://doi.org/10.1140/epjp/s13360-024-05052-y
Regular Article
Analytical representation of a charged black hole puncture solution
Departamento de Física Teórica - Instituto de Física A. D. Tavares, Universidade do Estado do Rio de Janeiro, R. São Francisco Xavier, 524, 20550-013, Rio de Janeiro, RJ, Brazil
Received:
9
January
2024
Accepted:
1
March
2024
Published online:
25
March
2024
The evolution of a single uncharged black hole with the moving puncture method, considering suitable gauge conditions, leads to a time-independent maximal slicing of Schwarzschild spacetime. This configuration was constructed numerically and later analytically. We proceed here taking an inverse path: We first derived the analytical solution representing time-independent maximal slicing of Reissner–Nordstrom spacetime and show that it is a final state dictated by the moving puncture evolution using appropriate gauge conditions.
Copyright comment Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2024. Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
