Stable bound orbits around static Einstein-Gauss-Bonnet black holes
arXiv:2204.10087 · doi:10.1103/PhysRevD.105.124033
Abstract
As is well-known, asymptotically flat, static and spherically symmetric black holes do not admit stable bound orbits of massive/massless particles outside the horizon in higher-dimensional Einstein gravity. However, for massive particles, this dramatically changes in higher curvature theories. We clarify the parameter range such that there exist stable bound orbits in -dimensional Einstein-Gauss-Bonnet theories for . In particular, we show the existence of the lower bound of the Gauss-Bonnet coupling constant below which stable bound orbits cease to exist. Moreover, we also find that for AdS-black holes in the theories, there can exist two stable circular orbits outside the horizon.
14 pages, 23 figures; v2: typos fixed; v3: published version
References in corpus (13)
- Light rings as observational evidence for event horizons: long-lived modes, ergoregions and nonlinear instabilities of ultracompact objects
- Complete Integrability of Geodesic Motion in General Kerr-NUT-AdS Spacetimes
- Final fate of spherically symmetric gravitational collapse of a dust cloud in Einstein-Gauss-Bonnet gravity
- Instability of supersymmetric microstate geometries
- Stable photon orbits in stationary axisymmetric electrovacuum spacetimes
- Stable Bound Orbits around Black Rings
- Chaos in Geodesic Motion around a Black Ring
- Innermost stable circular orbits in Majumdar--Papapetrou dihole spacetime
- Stable circular orbits in higher-dimensional multi-black hole spacetimes
- Circular Orbits in Einstein-Gauss-Bonnet Gravity
- Stable bound orbits in black lens backgrounds
- Stable circular orbits in caged black hole spacetimes
- Stable bound orbits in microstate geometries