Chaos v pohybu kolem černých děr
The geodesic motion around Kerr black holes is regular, but this may change when an additional source is present, even if the space-time symmetry were not lowered. In this thesis we study the eect of a simple (static and axially symmetric) additional source on geodesic dynamics in the eld of a Schwa...
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| Format: | Dissertation |
| Language: | Czech |
| Published: |
2009
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| Online Access: | http://www.nusl.cz/ntk/nusl-278128 |