Numerical study of the Kerr solution in rotating coordinates
arXiv:1602.06400 · doi:10.1103/PhysRevD.93.124001
Abstract
The Kerr solution in coordinates corotating with the horizon is studied as a testbed for a spacetime with a helical Killing vector in the Ernst picture. The solution is numerically constructed by solving the Ernst equation with a spectral method and a Newton iteration. We discuss convergence of the iteration for several initial iterates and different values of the Kerr parameters.
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