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  Non-Singular Quantum Geometry of the Schwarzschild Black Hole Interior

Ashtekar, A., & Bojowald, M. (2006). Non-Singular Quantum Geometry of the Schwarzschild Black Hole Interior. Classical and Quantum Gravity, 23(2), 391-412.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4B39-6 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4B3A-4
Genre: Journal Article

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0509075.pdf (Preprint), 323KB
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 Creators:
Ashtekar, Abhay, Author
Bojowald, Martin1, Author
Affiliations:
1Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24014              

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 Abstract: In homogeneous cosmologies, quantum geometry effects lead to a resolution of the classical singularity without having to invoke special boundary conditions at the singularity or introduce ad-hoc elements such as unphysical matter. The same effects are shown to lead to a resolution of the Schwarzschild singularity. The resulting quantum extension of space-time is likely to have significant implications to the black hole evaporation process. Similarities and differences with the situation in quantum geometrodynamics are pointed out.

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Language(s): eng - English
 Dates: 2006
 Publication Status: Published in print
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 Identifiers: eDoc: 240092
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Title: Classical and Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 23 (2) Sequence Number: - Start / End Page: 391 - 412 Identifier: -