Breakdown of field theory in near-horizon regions

Tom Banks; Patrick Draper; Manthos Karydas

doi:10.1007/JHEP06(2024)153

Breakdown of field theory in near-horizon regions

Tom Banks
, Patrick Draper
, Manthos Karydas

Research output: Contribution to journal › Article › peer-review

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 ∼ rs2GN^1/D, below which some breakdown of effective field theory may occur.

Original language	English (US)
Article number	153
Journal	Journal of High Energy Physics
Volume	2024
Issue number	6
DOIs	https://doi.org/10.1007/JHEP06(2024)153
State	Published - Jun 2024

Keywords

Black Holes
Models of Quantum Gravity

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1007/JHEP06(2024)153License: CC BY

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title = "Breakdown of field theory in near-horizon regions",

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.",

keywords = "Black Holes, Models of Quantum Gravity",

author = "Tom Banks and Patrick Draper and Manthos Karydas",

note = "The work of PD and MK is supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics under award number DE-SC0015655. The work of TB is supported by the U.S. Department of Energy, Office of Science, Office of High Energy Physics under award number DE-SC0010008. Rutgers Project 833012.",

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doi = "10.1007/JHEP06(2024)153",

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AU - Draper, Patrick

AU - Karydas, Manthos

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N2 - 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.

AB - 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.

KW - Black Holes

KW - Models of Quantum Gravity

UR - https://www.scopus.com/pages/publications/85196710457

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DO - 10.1007/JHEP06(2024)153

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JO - Journal of High Energy Physics

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IS - 6

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ER -

Breakdown of field theory in near-horizon regions

Abstract

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