Submerging islands through thermalization. (English) Zbl 1476.83117
Summary: We illustrate scenarios in which Hawking radiation collected in finite regions of a reservoir provides temporary access to the interior of black holes through transient entanglement “islands.” Whether these islands appear and the amount of time for which they dominate — sometimes giving way to a thermalization transition — is controlled by the amount of radiation we probe. In the first scenario, two reservoirs are coupled to an eternal black hole. The second scenario involves two holographic quantum gravitating systems at different temperatures interacting through a Rindler-like reservoir, which acts as a heat engine maintaining thermal equilibrium. The latter situation, which has an intricate phase structure, describes two eternal black holes radiating into each other through a shared reservoir.
MSC:
| 83C80 | Analogues of general relativity in lower dimensions |
| 83C45 | Quantization of the gravitational field |
| 83C57 | Black holes |
| 83E05 | Geometrodynamics and the holographic principle |
| 81T28 | Thermal quantum field theory |
| 81P42 | Entanglement measures, concurrencies, separability criteria |
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