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

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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, Alan Nicolás, Leston, Mauricio
Publicado: 2014
Materias:
Anti-de Sitter space
Holographic renormalization
Three-dimensional gravity
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v46_n5_p1_Garbarz
http://hdl.handle.net/20.500.12110/paper_00017701_v46_n5_p1_Garbarz
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_00017701_v46_n5_p1_Garbarz
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spelling paper:paper_00017701_v46_n5_p1_Garbarz2023-06-08T14:21:38Z Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions Garbarz, Alan Nicolás Leston, Mauricio 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. 2014 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v46_n5_p1_Garbarz 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, Alan Nicolás
Leston, Mauricio
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.
author Garbarz, Alan Nicolás
Leston, Mauricio
author_facet Garbarz, Alan Nicolás
Leston, Mauricio
author_sort Garbarz, Alan Nicolás
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
publishDate 2014
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v46_n5_p1_Garbarz
http://hdl.handle.net/20.500.12110/paper_00017701_v46_n5_p1_Garbarz
work_keys_str_mv AT garbarzalannicolas quasilocalenergyforthreedimensionalmassivegravitysolutionswithchiraldeformationsofads3boundaryconditions
AT lestonmauricio quasilocalenergyforthreedimensionalmassivegravitysolutionswithchiraldeformationsofads3boundaryconditions
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