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  Emergent Symmetry on Black Hole Horizons

Mei, J. (2014). Emergent Symmetry on Black Hole Horizons. Physical Review D, 89(6): 064066. doi:10.1103/PhysRevD.89.064066.

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1311.0225.pdf (Preprint), 120KB
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 Creators:
Mei, Jianwei1, Author           
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1Quantum Gravity & Unified Theories, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24014              

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Free keywords: High Energy Physics - Theory, hep-th,General Relativity and Quantum Cosmology, gr-qc
 Abstract: For a stationary and axisymmetric black hole, there is a natural way to split the fields into a probe sector and a background sector. The equations of motion for the probe sector enjoy a significantly enhanced symmetry on the black hole horizon. The extended symmetry is conformal in four dimensions, while in higher dimensions it is much bigger. This puts conformal symmetry at the bottom of the ladder of symmetries that can arise on black hole horizons in generic dimensions.

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 Dates: 2013-11-012014
 Publication Status: Issued
 Pages: 8 pages
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 1311.0225
DOI: 10.1103/PhysRevD.89.064066
 Degree: -

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Title: Physical Review D
  Other : Phys. Rev. D.
Source Genre: Journal
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Publ. Info: Lancaster, Pa. : American Physical Society
Pages: - Volume / Issue: 89 (6) Sequence Number: 064066 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: https://pure.mpg.de/cone/journals/resource/111088197762258