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, Alan Nicolás, Giribet, Gastón Enrique, Goya, Andrés Fabio, Leston, Mauricio
Formato: Articulo Preprint
Lenguaje:Inglés
Publicado: 2014
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/104127
http://hdl.handle.net/11336/17380
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id I19-R120-10915-104127
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Física
Holographic renormalization
Three-dimensional gravity
Anti-de sitter space
spellingShingle Física
Holographic renormalization
Three-dimensional gravity
Anti-de sitter space
Garbarz, Alan Nicolás
Giribet, Gastón Enrique
Goya, Andrés Fabio
Leston, Mauricio
Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions
topic_facet Física
Holographic renormalization
Three-dimensional gravity
Anti-de sitter space
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 Banados-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 finite mass and angular momentum.
format Articulo
Preprint
author Garbarz, Alan Nicolás
Giribet, Gastón Enrique
Goya, Andrés Fabio
Leston, Mauricio
author_facet Garbarz, Alan Nicolás
Giribet, Gastón Enrique
Goya, Andrés Fabio
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 http://sedici.unlp.edu.ar/handle/10915/104127
http://hdl.handle.net/11336/17380
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AT goyaandresfabio quasilocalenergyforthreedimensionalmassivegravitysolutionswithchiraldeformationsofads3boundaryconditions
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