Abstract
The geodesic flow of a perturbation of the Schwarzschild metric is shown to possess a chaotic invariant set. The perturbed meric is a relativistic analogue of Hill's problem in classical celestial mechanics in that is models the effects of a distant third body.
Original language | English (US) |
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Pages (from-to) | 415-430 |
Number of pages | 16 |
Journal | Communications in Mathematical Physics |
Volume | 150 |
Issue number | 2 |
DOIs | |
State | Published - Nov 1 1992 |