arXiv · 0811.3815
Homoclinic Orbits around Spinning Black Holes II: The Phase Space Portrait
Abstract
In paper I in this series, we found exact expressions for the equatorial homoclinic orbits: the separatrix between bound and plunging, whirling and not whirling. As a companion to that physical space study, in this paper we paint a phase space portrait of the homoclinic orbits that includes exact expressions for the actions and fundamental frequencies. Additionally, we develop a reduced Hamiltonian description of Kerr motion that allows us to track groups of trajectories with a single global clock. This facilitates a variational analysis, whose stability exponents and eigenvectors could potentially be useful for future studies of families of black hole orbits and their associated gravitational waveforms.
Explore related subjects
Keep this discovery
Gabe Perez-Giz, Janna Levin. 2008-11-24. Homoclinic Orbits around Spinning Black Holes II: The Phase Space Portrait. https://doi.org/10.1103/physrevd.79.124014
Cite the original work for its findings. Save a collection to share your selection of sources.