The Ernst equation and ergosurfaces
arXiv:gr-qc/0603041 · doi:10.1088/0264-9381/23/13/007
Abstract
We show that analytic solutions $\mcE$ of the Ernst equation with non-empty zero-level-set of $\Re \mcE$ lead to smooth ergosurfaces in space-time. In fact, the space-time metric is smooth near a "Ernst ergosurface" if and only if $\mcE$ is smooth near and does not have zeros of infinite order there.
23 pages, 4 figures; misprints corrected
Cited by in corpus (5)
- Constructive proof of the Kerr-Newman black hole uniqueness including the extreme case
- Rotating spacetimes with a cosmological constant
- Self-gravitating perfect-fluid tori around black holes: Bifurcations, ergoregions, and geometrical properties
- Toroidal magnetic fields in self-gravitating disks around black holes
- Ernst equation and spheroidal coordinates with a cosmological constant term