Boundary stress tensor and asymptotically AdS3 non-Einstein spaces at the chiral point

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Chiral gravity admits asymptotically AdS3 solutions that are not locally equivalent to AdS3; meaning that solutions do exist which, while obeying the strong boundary conditions usually imposed in general relativity, happen not to be Einstein spaces. In topologically massive gravity (TMG), the existe...

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Detalles Bibliográficos
Autor principal: Giribet, G.
Otros Autores: Goya, A., Leston, M.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2011
Acceso en línea:Registro en Scopus
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Registro en la Biblioteca Digital
Aporte de:Registro referencial: Solicitar el recurso aquí
Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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100 1 |a Giribet, G. 
245 1 0 |a Boundary stress tensor and asymptotically AdS3 non-Einstein spaces at the chiral point 
260 |c 2011 
270 1 0 |m Giribet, G.; Universidad de Buenos Aires FCEN-UBA, Ciudad Universitaria, Pabellón i, 1428 Buenos Aires, Argentina; email: gaston@df.uba.ar 
506 |2 openaire  |e Política editorial 
504 |a Deser, S., Jackiw, R., Templeton, S., (1982) Phys. Rev. Lett., 48, p. 975. , PRLTAO 0031-9007 10.1103/PhysRevLett.48.975 
504 |a Li, W., Song, W., Strominger, A., J. High Energy Phys., 2008 (4), p. 082. , JHEPFG 1029-8479 10.1088/1126-6708/2008/04/082 
504 |a Anninos, D., Li, W., Padi, M., Song, W., Strominger, A., J. High Energy Phys., 2009 (3), p. 130. , JHEPFG 1029-8479 10.1088/1126-6708/2009/03/130 
504 |a Brown, J., Henneaux, M., (1986) Commun. Math. Phys., 104, p. 207. , CMPHAY 0010-3616 10.1007/BF01211590 
504 |a Maloney, A., Song, W., Strominger, A., (2010) Phys. Rev. D, 81, p. 064007. , PRVDAQ 1550-7998 10.1103/PhysRevD.81.064007 
504 |a Maloney, A., Witten, E., J. High Energy Phys., 2010 (2), p. 029. , JHEPFG 1029-8479 10.1007/JHEP02(2010)029 
504 |a De Buyl, S., Compére, G., Detournay, S., J. High Energy Phys., 2010 (10), p. 042. , JHEPFG 1029-8479 
504 |a Giribet, G., Leston, M., J. High Energy Phys., 2010 (9), p. 070. , JHEPFG 1029-8479 10.1007/JHEP09(2010)070 
504 |a Bergshoeff, E., Hohm, O., Townsend, P., (2009) Phys. Rev. Lett., 102, p. 201301. , PRLTAO 0031-9007 10.1103/PhysRevLett.102.201301 
504 |a Bergshoeff, E., Hohm, O., Townsend, P., (2009) Phys. Rev. D, 79, p. 124042. , PRVDAQ 1550-7998 10.1103/PhysRevD.79.124042 
504 |a Henneaux, M., Martinez, C., Troncoso, R., Zanelli, J., (2007) Ann. Phys. (N.Y.), 322, p. 824. , APNYA6 0003-4916 10.1016/j.aop.2006.05.002 
504 |a Grumiller, D., Johansson, N., J. High Energy Phys., 2008 (7), p. 134. , JHEPFG 1029-8479 10.1088/1126-6708/2008/07/134 
504 |a Grumiller, D., Johansson, N., (2008) Int. J. Mod. Phys. D, 17, p. 2367. , IMPDEO 0218-2718 10.1142/S0218271808014096 
504 |a Henneaux, M., Martínez, C., Troncoso, R., (2009) Phys. Rev. D, 79, pp. 081502R. , PRVDAQ 1550-7998 10.1103/PhysRevD.79.081502 
504 |a Henneaux, M., Martínez, C., Troncoso, R., (2010) Phys. Rev. D, 82, p. 064038. , PRVDAQ 1550-7998 10.1103/PhysRevD.82.064038 
504 |a Liu, Y., Sun, Y.-W., (2009) Phys. Rev. D, 79, p. 126001. , PRVDAQ 1550-7998 10.1103/PhysRevD.79.126001 
504 |a Liu, Y., Sun, Y.-W., J. High Energy Phys., 2009 (4), p. 106. , JHEPFG 1029-8479 10.1088/1126-6708/2009/04/106 
504 |a Liu, Y., Sun, Y.-W., J. High Energy Phys., 2009 (5), p. 039. , JHEPFG 1029-8479 10.1088/1126-6708/2009/05/039 
504 |a Garbarz, A., Giribet, G., Vásquez, Y., (2009) Phys. Rev. D, 79, p. 044036. , PRVDAQ 1550-7998 10.1103/PhysRevD.79.044036 
504 |a Clément, G., (2009) Classical Quantum Gravity, 26, p. 165002. , CQGRDG 0264-9381 10.1088/0264-9381/26/16/165002 
504 |a Ayón-Beato, E., Giribet, G., Hassaïne, M., J. High Energy Phys., 2009 (5), p. 029. , JHEPFG 1029-8479 10.1088/1126-6708/2009/05/029 
504 |a Bañados, M., Teitelboim, C., Zanelli, J., (1992) Phys. Rev. Lett., 69, p. 1849. , PRLTAO 0031-9007 10.1103/PhysRevLett.69.1849 
504 |a Bañados, M., Henneaux, M., Teitelboim, C., Zanelli, J., (1993) Phys. Rev. D, 48, p. 1506. , PRVDAQ 0556-2821 10.1103/PhysRevD.48.1506 
504 |a Henningson, M., Skenderis, K., J. High Energy Phys., 1998 (7), p. 023. , JHEPFG 1029-8479 10.1088/1126-6708/1998/07/023 
504 |a Balasubramanian, V., Kraus, P., (1999) Commun. Math. Phys., 208, p. 413. , CMPHAY 0010-3616 10.1007/s002200050764 
504 |a Brown, J., York, J., (1993) Phys. Rev. D, 47, p. 1407. , PRVDAQ 0556-2821 10.1103/PhysRevD.47.1407 
504 |a Hohm, O., Tonni, E., J. High Energy Phys., 2010 (4), p. 093. , JHEPFG 1029-8479 10.1007/JHEP04(2010)093 
504 |a Y. Kwon, S. Nam, J-D. Park, and S-H. Yi, arXiv:1106.4609; Pérez, A., Tempo, D., Troncoso, R., J. High Energy Phys., 2011 (7), p. 093. , JHEPFG 1029-8479 10.1007/JHEP07(2011)093 
504 |a Kraus, P., Larsen, F., J. High Energy Phys., 2006 (1), p. 022. , JHEPFG 1029-8479 10.1088/1126-6708/2006/01/022 
504 |a Kraus, P., (2008) Lect. Notes Phys., 755, p. 1. , LNPHA4 0075-8450 10.1007/978-3-540-79523-0-4 
504 |a Saida, H., Soda, J., (2000) Phys. Lett. B, 471, p. 358. , PYLBAJ 0370-2693 10.1016/S0370-2693(99)01405-7 
520 3 |a Chiral gravity admits asymptotically AdS3 solutions that are not locally equivalent to AdS3; meaning that solutions do exist which, while obeying the strong boundary conditions usually imposed in general relativity, happen not to be Einstein spaces. In topologically massive gravity (TMG), the existence of non-Einstein solutions is particularly connected to the question about the role played by complex saddle points in the Euclidean path integral. Consequently, studying (the existence of) nonlocally AdS3 solutions to chiral gravity is relevant to understanding the quantum theory. Here, we discuss a special family of nonlocally AdS3 solutions to chiral gravity. In particular, we show that such solutions persist when one deforms the theory by adding the higher-curvature terms of the so-called new massive gravity. Moreover, the addition of higher-curvature terms to the gravity action introduces new nonlocally AdS3 solutions that have no analogues in TMG. Both stationary and time-dependent, axially symmetric solutions that asymptote AdS3 space without being locally equivalent to it appear. Defining the boundary stress tensor for the full theory, we show that these non-Einstein geometries have associated vanishing conserved charges. © 2011 American Physical Society.  |l eng 
593 |a Universidad de Buenos Aires FCEN-UBA, Ciudad Universitaria, Pabellón i, 1428 Buenos Aires, Argentina 
593 |a Instituto de Astronomía y Física Del Espacio IAFE-CONICET, Ciudad Universitaria, Pabellón IAFE, 1428 C. C. 67 Suc. 28, Buenos Aires, Argentina 
700 1 |a Goya, A. 
700 1 |a Leston, M. 
773 0 |d 2011  |g v. 84  |k n. 6  |p Phys Rev D Part Fields Gravit Cosmol  |x 15507998  |t Physical Review D - Particles, Fields, Gravitation and Cosmology 
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