MG15 - Talk detail |
|
Participant |
Hamilton, Andrew J. S. | |||||||
|
Institution |
JILA - Box 440, U. Colorado - Boulder - CO - USA | |||||||
|
Session |
EU2 |
Accepted |
|
Order |
Time |
|||
|
Talk |
Plenary talk shifted to EU2 session |
Title |
Inflation is Followed by BKL Collapse in Accreting, Rotating Black Holes | |||||
| Coauthors | ||||||||
|
Abstract |
In 1970 Belinskii, Khalatnikov and Lifshitz argued that the generic outcome of collapse to a spacelike singularity would be chaotic and oscillatory. The conclusion was called into question with Poisson & Israel's 1990 discovery of the mass inflation instability at the inner horizon of a rotating black hole. It has been widely claimed that the generic outcome of mass inflation is a weak null singularity. However, this claim is premised on a black hole that remains forever isolated. Real astronomical black holes accrete. Nonlinear general relativistic numerical calculations show that for a black hole that accretes, inflation is followed by BKL collapse. This talk will be illustrated by real-time interactive visualizations with the Black Hole Flight Simulator. |
|||||||
Pdf file |
||||||||