Asymptotically flat spacetimes in three-dimensional higher spin gravity

Hernán A. González; Javier Matulich; Miguel Pino; Ricardo Troncoso

doi:10.1007/JHEP09(2013)016

Asymptotically flat spacetimes in three-dimensional higher spin gravity

Hernán A. González, Javier Matulich, Miguel Pino, Ricardo Troncoso

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94 Citas (Scopus)

Resumen

A consistent set of asymptotic conditions for higher spin gravity in three dimensions is proposed in the case of vanishing cosmological constant. The asymptotic symmetries are found to be spanned by a higher spin extension of the BMS₃ algebra with an appropriate central extension. It is also shown that our results can be recovered from the ones recently found for asymptotically AdS₃ spacetimes by virtue of a suitable gauge choice that allows to perform the vanishing cosmological constant limit.

Idioma original	Inglés
Número de artículo	16
Publicación	Journal of High Energy Physics
Volumen	2013
N.º	9
DOI	https://doi.org/10.1007/JHEP09(2013)016
Estado	Publicada - 2013
Publicado de forma externa	Sí

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abstract = "A consistent set of asymptotic conditions for higher spin gravity in three dimensions is proposed in the case of vanishing cosmological constant. The asymptotic symmetries are found to be spanned by a higher spin extension of the BMS3 algebra with an appropriate central extension. It is also shown that our results can be recovered from the ones recently found for asymptotically AdS3 spacetimes by virtue of a suitable gauge choice that allows to perform the vanishing cosmological constant limit.",

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AU - Pino, Miguel

AU - Troncoso, Ricardo

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N2 - A consistent set of asymptotic conditions for higher spin gravity in three dimensions is proposed in the case of vanishing cosmological constant. The asymptotic symmetries are found to be spanned by a higher spin extension of the BMS3 algebra with an appropriate central extension. It is also shown that our results can be recovered from the ones recently found for asymptotically AdS3 spacetimes by virtue of a suitable gauge choice that allows to perform the vanishing cosmological constant limit.

AB - A consistent set of asymptotic conditions for higher spin gravity in three dimensions is proposed in the case of vanishing cosmological constant. The asymptotic symmetries are found to be spanned by a higher spin extension of the BMS3 algebra with an appropriate central extension. It is also shown that our results can be recovered from the ones recently found for asymptotically AdS3 spacetimes by virtue of a suitable gauge choice that allows to perform the vanishing cosmological constant limit.

KW - Classical Theories of Gravity

KW - Conformal and W Symmetry

KW - Gauge-gravity correspondence

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Asymptotically flat spacetimes in three-dimensional higher spin gravity

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