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  Modelling black holes with angular momentum in loop quantum gravity

Frodden, E., Perez, A., Pranzetti, D., & Roeken, C. (2014). Modelling black holes with angular momentum in loop quantum gravity. General Relativity and Gravitation, 46: 1828. doi:10.1007/s10714-014-1828-6.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000E-EE79-E Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0024-8F0B-A
Genre: Journal Article

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1212.5166 (Preprint), 235KB
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 Creators:
Frodden, Ernesto, Author
Perez, Alejandro, Author
Pranzetti, Daniele1, Author              
Roeken, Christian, Author
Affiliations:
1Microscopic Quantum Structure & Dynamics of Spacetime, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, 67201              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,High Energy Physics - Theory, hep-th
 Abstract: We construct a SU(2) connection formulation of Kerr isolated horizons. As in the non-rotating case, the model is based on a SU(2) Chern-Simons theory describing the degrees of freedom on the horizon. The presence of a non-vanishing angular momentum modifies the admissibility conditions for spin network states. Physical states of the system are in correspondence with open intertwiners with total spin matching the angular momentum of the spacetime.

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 Dates: 2012-12-202014
 Publication Status: Published in print
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 Rev. Method: -
 Identifiers: arXiv: 1212.5166
DOI: 10.1007/s10714-014-1828-6
 Degree: -

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Title: General Relativity and Gravitation
Source Genre: Journal
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Publ. Info: Dordrecht, etc. : Kluwer Academic Publishers [etc.]
Pages: - Volume / Issue: 46 Sequence Number: 1828 Start / End Page: - Identifier: ISSN: 0001-7701
CoNE: /journals/resource/954925263179