Inside astronomically realistic black holes
| Autor: | Hamilton, Andrew J. S. |
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| Rok vydání: | 2019 |
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| Druh dokumentu: | Working Paper |
| Popis: | The singularity of a spherical (Schwarzschild) black hole is a surface, not a point. A freely-falling, non-rotating observer sees Hawking radiation with energy density diverging with radius as $\rho \propto r^{-6}$ near the Schwarzschild singular surface. Spacetime inside a rotating (Kerr) black hole terminates at the inner horizon because of the Poisson-Israel mass inflation instability. If the black hole is accreting, as all realistic black holes do, then generically inflation gives way to Belinski-Khalatnikov-Lifshitz oscillatory collapse to a strong, spacelike singular surface. Comment: 18 pages, invited plenary talk, to be published in the Proceedings of the Fifteenth Marcel Grossmann Meeting on General Relativity, July 2018, ed. Elia Battistelli, Robert T. Jantzen, and Remo Ruffini |
| Databáze: | arXiv |
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