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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Autor principal: Garbarz, A.
Otros Autores: Giribet, G., Goya, A., Leston, M.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Springer New York LLC 2014
Acceso en línea:Registro en Scopus
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100 1 |a Garbarz, A. 
245 1 0 |a Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS3 boundary conditions 
260 |b Springer New York LLC  |c 2014 
270 1 0 |m Giribet, G.; Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla, 4950 Valparaiso, Chile; email: gaston@df.uba.ar 
506 |2 openaire  |e Política editorial 
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504 |a Giribet, G., Leston, M., (2010) Jhep, 1009, p. 070 
504 |a Giribet, G., Goya, A., Leston, M., (2011) Phys. Rev., D84, p. 066003 
504 |a Correa, F., Martínez, C., Troncoso, R., (2012) Jhep, 1202, p. 136 
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520 3 |a 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.  |l eng 
536 |a Detalles de la financiación: Umweltbundesamt 
536 |a Detalles de la financiación: Agencia Nacional de Promoción Científica y Tecnológica 
536 |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas 
536 |a Detalles de la financiación: Acknowledgments This work has been supported by UBA, CONICET, and ANPCyT. The authors are grateful to Stéphane Detournay and Guillem Pérez–Nadal for discussions. G.G. thanks Pontificia Univer-sidad Católica de Valparaíso for the hospitality during his stays, where part of this work was done. 
593 |a Departamento de Física, Universidad de Buenos Aires FCEN-UBA, IFIBA-CONICET, Ciudad Universitaria, Pabellón I, 1428 Buenos Aires, Argentina 
593 |a Instituto de Física de La Plata, Universidad Nacional de La Plata IFLP-UNLP, C.C. 67, 1900 La Plata, Argentina 
593 |a Instituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla, 4950 Valparaiso, Chile 
593 |a Instituto de Astronomía y Física del Espacio IAFE-CONICET, Ciudad Universitaria, C.C. 67 Suc. 28, 1428 Buenos Aires, Argentina 
690 1 0 |a ANTI-DE SITTER SPACE 
690 1 0 |a HOLOGRAPHIC RENORMALIZATION 
690 1 0 |a THREE-DIMENSIONAL GRAVITY 
700 1 |a Giribet, G. 
700 1 |a Goya, A. 
700 1 |a Leston, M. 
773 0 |d Springer New York LLC, 2014  |g v. 46  |h pp. 1-14  |k n. 5  |p Gen. Relativ. Gravit.  |x 00017701  |w (AR-BaUEN)CENRE-369  |t General Relativity and Gravitation 
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