We review some aspects of three-dimensional quantum gravity with emphasis in
the `CFT -> Geometry' map that follows from the Brown-Henneaux conformal
algebra. The general solution to the classical equations of motion with anti-de
Sitter boundary conditions is displayed. This solution is parametrized by two
functions which become Virasoro operators after quantisation. A map from the
space of states to the space of classical solutions is exhibited. Some recent
proposals to understand the Bekenstein-Hawking entropy are reviewed in this
context. The origin of the boundary degrees of freedom arising in 2+1 gravity
is analysed in detail using a Hamiltonian Chern-Simons formalism.
%0 Journal Article
%1 Banados1999Threedimensional
%A Banados, Maximo
%D 1999
%K 3dgravity, ads3-cft2, btz
%P 147--169
%R 10.1063/1.59661
%T Three-dimensional quantum geometry and black holes
%U http://dx.doi.org/10.1063/1.59661
%X We review some aspects of three-dimensional quantum gravity with emphasis in
the `CFT -> Geometry' map that follows from the Brown-Henneaux conformal
algebra. The general solution to the classical equations of motion with anti-de
Sitter boundary conditions is displayed. This solution is parametrized by two
functions which become Virasoro operators after quantisation. A map from the
space of states to the space of classical solutions is exhibited. Some recent
proposals to understand the Bekenstein-Hawking entropy are reviewed in this
context. The origin of the boundary degrees of freedom arising in 2+1 gravity
is analysed in detail using a Hamiltonian Chern-Simons formalism.
@article{Banados1999Threedimensional,
abstract = {{We review some aspects of three-dimensional quantum gravity with emphasis in
the `CFT -\> Geometry' map that follows from the Brown-Henneaux conformal
algebra. The general solution to the classical equations of motion with anti-de
Sitter boundary conditions is displayed. This solution is parametrized by two
functions which become Virasoro operators after quantisation. A map from the
space of states to the space of classical solutions is exhibited. Some recent
proposals to understand the Bekenstein-Hawking entropy are reviewed in this
context. The origin of the boundary degrees of freedom arising in 2+1 gravity
is analysed in detail using a Hamiltonian Chern-Simons formalism.}},
added-at = {2019-02-26T10:37:35.000+0100},
archiveprefix = {arXiv},
author = {Banados, Maximo},
biburl = {https://www.bibsonomy.org/bibtex/2c3c1f27bca5a9bc0d90f86caf0779748/acastro},
citeulike-article-id = {12527993},
citeulike-linkout-0 = {http://arxiv.org/abs/hep-th/9901148},
citeulike-linkout-1 = {http://arxiv.org/pdf/hep-th/9901148},
citeulike-linkout-2 = {http://dx.doi.org/10.1063/1.59661},
day = 22,
doi = {10.1063/1.59661},
eprint = {hep-th/9901148},
interhash = {ad2846fd474a29511b0858b51102ffa9},
intrahash = {c3c1f27bca5a9bc0d90f86caf0779748},
keywords = {3dgravity, ads3-cft2, btz},
location = {Buenos Aires,(Argentina)},
month = feb,
pages = {147--169},
posted-at = {2013-07-25 20:59:33},
priority = {2},
timestamp = {2019-02-26T10:37:35.000+0100},
title = {{Three-dimensional quantum geometry and black holes}},
url = {http://dx.doi.org/10.1063/1.59661},
year = 1999
}