Black hole evaporation: A paradigm

Ashtekar, Abhay; Bojowald, Martin

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Black hole evaporation: A paradigm

Ashtekar, A., & Bojowald, M. (2005). Black hole evaporation: A paradigm. Classical and Quantum Gravity, 22(16), 3349-3362.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-4DEC-4 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0013-4DED-2

Genre: Journal Article

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Creators:
Ashtekar, Abhay¹, Author
Bojowald, Martin¹, Author

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1Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24014

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Abstract: A paradigm describing black hole evaporation in non-perturbative quantum gravity is developed by combining two sets of detailed results: i) resolution of the Schwarzschild singularity in loop quantum gravity; and ii) time-evolution of black holes in the dynamical horizon framework. Quantum geometry effects introduce a major modification in the traditional space-time diagram of black hole evaporation, providing a possible mechanism for recovery of information that is classically lost in the process of black hole formation. The paradigm is developed directly in the Lorentzian regime and necessary conditions for its viability are discussed. If these conditions are met, much of the tension between expectations based on space-time geometry and structure of quantum theory would be resolved.

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Language(s): eng - English

Dates: Date issued: 2005-08-21

Publication Status: Issued

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Identifiers: eDoc: 204946

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Title: Classical and Quantum Gravity

Source Genre: Journal

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Pages: - Volume / Issue: 22 (16) Sequence Number: - Start / End Page: 3349 - 3362 Identifier: -