Extreme and very-near-extreme spin J Kerr black holes have been conjectured
to be holographically dual to two-dimensional (2D) conformal field theories
(CFTs) with left and right central charges c\_L=c\_R=12J. In this paper it is
observed that the 2D conformal symmetry of the scalar wave equation at low
frequencies persists for generic non-extreme values of the mass M.
Interestingly, this conformal symmetry is not derived from a conformal symmetry
of the spacetime geometry except in the extreme limit. The periodic
identification of the azimuthal angle is shown to correspond to a spontaneous
breaking of the conformal symmetry by left and right…(more)
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%0 Journal Article
%1 Castro2010Hidden
%A Castro, Alejandra
%A Maloney, Alexander
%A Strominger, Andrew
%D 2010
%J Physical Review D
%K hcs, kerr-cft, kerrbh
%N 2
%R 10.1103/physrevd.82.024008
%T Hidden Conformal Symmetry of the Kerr Black Hole
%U http://dx.doi.org/10.1103/physrevd.82.024008
%V 82
%X Extreme and very-near-extreme spin J Kerr black holes have been conjectured
to be holographically dual to two-dimensional (2D) conformal field theories
(CFTs) with left and right central charges c\_L=c\_R=12J. In this paper it is
observed that the 2D conformal symmetry of the scalar wave equation at low
frequencies persists for generic non-extreme values of the mass M.
Interestingly, this conformal symmetry is not derived from a conformal symmetry
of the spacetime geometry except in the extreme limit. The periodic
identification of the azimuthal angle is shown to correspond to a spontaneous
breaking of the conformal symmetry by left and right temperatures (T\_L,T\_R).
The well-known low-frequency scalar-Kerr scattering amplitudes coincide with
correlators of a 2D CFT at these temperatures. Moreover the CFT microstate
degeneracy inferred from the Cardy formula agrees exactly with the
Bekenstein-Hawking area law for all M and J. These observations provide
evidence for the conjecture that the Kerr black hole is dual to a c\_L=c\_R=12J
2D CFT at temperatures (T\_L,T\_R) for every value of M and J.
@article{Castro2010Hidden,
abstract = {{Extreme and very-near-extreme spin J Kerr black holes have been conjectured
to be holographically dual to two-dimensional (2D) conformal field theories
(CFTs) with left and right central charges c\_L=c\_R=12J. In this paper it is
observed that the 2D conformal symmetry of the scalar wave equation at low
frequencies persists for generic non-extreme values of the mass M.
Interestingly, this conformal symmetry is not derived from a conformal symmetry
of the spacetime geometry except in the extreme limit. The periodic
identification of the azimuthal angle is shown to correspond to a spontaneous
breaking of the conformal symmetry by left and right temperatures (T\_L,T\_R).
The well-known low-frequency scalar-Kerr scattering amplitudes coincide with
correlators of a 2D CFT at these temperatures. Moreover the CFT microstate
degeneracy inferred from the Cardy formula agrees exactly with the
Bekenstein-Hawking area law for all M and J. These observations provide
evidence for the conjecture that the Kerr black hole is dual to a c\_L=c\_R=12J
2D CFT at temperatures (T\_L,T\_R) for every value of M and J.}},
added-at = {2019-02-26T10:37:35.000+0100},
archiveprefix = {arXiv},
author = {Castro, Alejandra and Maloney, Alexander and Strominger, Andrew},
biburl = {https://www.bibsonomy.org/bibtex/2b82aaf56b6436b0977a848d7c23f6ef6/acastro},
citeulike-article-id = {6994970},
citeulike-linkout-0 = {http://arxiv.org/abs/1004.0996},
citeulike-linkout-1 = {http://arxiv.org/pdf/1004.0996},
citeulike-linkout-2 = {http://dx.doi.org/10.1103/physrevd.82.024008},
day = 7,
doi = {10.1103/physrevd.82.024008},
eprint = {1004.0996},
interhash = {24ed24c41404efe8fc0f278d780181cb},
intrahash = {b82aaf56b6436b0977a848d7c23f6ef6},
journal = {Physical Review D},
keywords = {hcs, kerr-cft, kerrbh},
month = apr,
number = 2,
posted-at = {2010-06-21 00:17:20},
priority = {2},
timestamp = {2019-02-26T10:37:35.000+0100},
title = {{Hidden Conformal Symmetry of the Kerr Black Hole}},
url = {http://dx.doi.org/10.1103/physrevd.82.024008},
volume = 82,
year = 2010
}