Abstract
We discuss back-reaction in the semiclassical treatment of quantum fields near a black hole. When the state deviates significantly from Hartle-Hawking, simple energetic considerations of back-reaction give rise to a characteristic radial distance scale ∼ rs2GN1/D, below which some breakdown of effective field theory may occur.
Original language | English (US) |
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Article number | 153 |
Journal | Journal of High Energy Physics |
Volume | 2024 |
Issue number | 6 |
DOIs | |
State | Published - Jun 2024 |
Externally published | Yes |
Keywords
- Black Holes
- Models of Quantum Gravity
ASJC Scopus subject areas
- Nuclear and High Energy Physics