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  Quantum geometry and the Schwarzschild singularity

Ashtekar, A., & Bojowald, M. (2006). Quantum geometry and the Schwarzschild singularity. Classical and Quantum Gravity, 23(2), 391-411.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4AB0-D Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-4AB1-B
Genre: Journal Article

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cqg6_2_008.pdf (Publisher version), 260KB
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 Creators:
Ashtekar, Abhay1, Author
Bojowald, Martin2, Author
Affiliations:
1External Organizations, escidoc:persistent13              
2Quantum 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 spacetime is likely to have significant implications for 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: 2006-01-21
 Publication Status: Published in print
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 Identifiers: eDoc: 297781
ISI: 000235052300010
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Title: Classical and Quantum Gravity
  Alternative Title : Class. Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 23 (2) Sequence Number: - Start / End Page: 391 - 411 Identifier: ISSN: 0264-9381