Isofrequency pairing of geodesic orbits in Kerr geometry
Abstract ? Bound geodesic orbits around a Kerr black hole can be parametrized by three constants of the motion: the (specific) orbital energy, angular momentum, and Carter constant. Generically, each orbit also has associated with it three frequencies, related to the radial, longitudinal, and (m...
| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
2013-04-03.
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| Subjects: | |
| Online Access: | Get fulltext |