Semiclassical black holes and horizon singularities
In spherical symmetry, solutions of the semiclassical Einstein equations belong to one of two possible classes. Both classes contain solutions that - depending on the dynamic behavior of the horizon - describe evaporating physical black holes or expanding white holes (trapped/anti-trapped regions th...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
American Institute of Physics Inc.
2022
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| Online Access: | View Fulltext in Publisher |
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