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Breakdown of Field Theory in Near-Horizon Regions

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arxiv 2401.03572 v3 pith:VWK7XR6L submitted 2024-01-07 hep-th gr-qc

Tom Banks , Patrick Draper , Manthos Karydas This is my paper · ORCID
classification hep-thgr-qc
keywords back-reactionbreakdownfieldtheorybelowblackcharacteristicconsiderations
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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 $\sim (r_s^{2}G_N)^{1/D}$, below which some breakdown of effective field theory may occur.

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  1. Quantum uncertainty in the area of a black hole

    hep-th 2024-12 conditional novelty 7.0 of 10

    The variance of the Schwarzschild horizon area in linearized quantum gravity is computed to be ~ r_H^2 l_P^2, giving a standard deviation ∆A ~ r_H l_P.

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