Journal
PHYSICAL REVIEW D
Volume 103, Issue 10, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.103.106014
Keywords
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Funding
- FQXi Grant [FQXi-RFP-1818]
- John Templeton Foundation, Quantum Information Structure of Spacetime (QISS) Project [61466]
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At the end of Hawking radiation, the horizon of a black hole enters a physical region where quantum gravity cannot be ignored. The physics of this region has not been thoroughly explored, but a technique to study it has been introduced.
At the end of the Hawking evaporation the horizon of a black hole enters a physical region where quantum gravity cannot be neglected. The physics of this region has not been much explored. We characterize its physics and introduce a technique to study it.
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