Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions

We consider critical gravity in three dimensions; that is, the New Massive Gravity theory formulated about Anti-de Sitter (AdS) space with the specific value of the graviton mass for which it results dual to a two-dimensional conformal field theory with vanishing central charge. As it happens with K...

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Autores principales:	Garbarz, A., Giribet, G., Goya, A., Leston, M.
Formato:	JOUR
Materias:	Anti-de Sitter space Holographic renormalization Three-dimensional gravity
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00017701_v46_n5_p1_Garbarz
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

id	todo:paper_00017701_v46_n5_p1_Garbarz
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spelling	todo:paper_00017701_v46_n5_p1_Garbarz2023-10-03T13:52:09Z Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions Garbarz, A. Giribet, G. Goya, A. Leston, M. Anti-de Sitter space Holographic renormalization Three-dimensional gravity We consider critical gravity in three dimensions; that is, the New Massive Gravity theory formulated about Anti-de Sitter (AdS) space with the specific value of the graviton mass for which it results dual to a two-dimensional conformal field theory with vanishing central charge. As it happens with Kerr black holes in four-dimensional critical gravity, in three-dimensional critical gravity the Bañados-Teitelboim-Zanelli black holes have vanishing mass and vanishing angular momentum. However, provided suitable asymptotic conditions are chosen, the theory may also admit solutions carrying non-vanishing charges. Here, we give simple examples of exact solutions that exhibit falling-off conditions that are even weaker than those of the so-called Log-gravity. For such solutions, we define the quasilocal stress-tensor and use it to compute conserved charges. Despite the drastic deformation of AdS3 asymptotic, these solutions have non-zero mass and angular momentum, which we compute. © 2014 Springer Science+Business Media New York. Fil:Garbarz, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Leston, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00017701_v46_n5_p1_Garbarz
institution	Universidad de Buenos Aires
institution_str	I-28
repository_str	R-134
collection	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic	Anti-de Sitter space Holographic renormalization Three-dimensional gravity
spellingShingle	Anti-de Sitter space Holographic renormalization Three-dimensional gravity Garbarz, A. Giribet, G. Goya, A. Leston, M. Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions
topic_facet	Anti-de Sitter space Holographic renormalization Three-dimensional gravity
description	We consider critical gravity in three dimensions; that is, the New Massive Gravity theory formulated about Anti-de Sitter (AdS) space with the specific value of the graviton mass for which it results dual to a two-dimensional conformal field theory with vanishing central charge. As it happens with Kerr black holes in four-dimensional critical gravity, in three-dimensional critical gravity the Bañados-Teitelboim-Zanelli black holes have vanishing mass and vanishing angular momentum. However, provided suitable asymptotic conditions are chosen, the theory may also admit solutions carrying non-vanishing charges. Here, we give simple examples of exact solutions that exhibit falling-off conditions that are even weaker than those of the so-called Log-gravity. For such solutions, we define the quasilocal stress-tensor and use it to compute conserved charges. Despite the drastic deformation of AdS3 asymptotic, these solutions have non-zero mass and angular momentum, which we compute. © 2014 Springer Science+Business Media New York.
format	JOUR
author	Garbarz, A. Giribet, G. Goya, A. Leston, M.
author_facet	Garbarz, A. Giribet, G. Goya, A. Leston, M.
author_sort	Garbarz, A.
title	Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions
title_short	Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions
title_full	Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions
title_fullStr	Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions
title_full_unstemmed	Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions
title_sort	quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of ads3 boundary conditions
url	http://hdl.handle.net/20.500.12110/paper_00017701_v46_n5_p1_Garbarz
work_keys_str_mv	AT garbarza quasilocalenergyforthreedimensionalmassivegravitysolutionswithchiraldeformationsofads3boundaryconditions AT giribetg quasilocalenergyforthreedimensionalmassivegravitysolutionswithchiraldeformationsofads3boundaryconditions AT goyaa quasilocalenergyforthreedimensionalmassivegravitysolutionswithchiraldeformationsofads3boundaryconditions AT lestonm quasilocalenergyforthreedimensionalmassivegravitysolutionswithchiraldeformationsofads3boundaryconditions
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Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions

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