Asymptotically flat spacetimes in three-dimensional higher spin gravity

A bstract 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 BMS 3 algebra with an appropriate central extension. It is a...

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Published in:The journal of high energy physics 2013-09, Vol.2013 (9), p.1-16, Article 16
Main Authors: González, Hernán A., Matulich, Javier, Pino, Miguel, Troncoso, Ricardo
Format: Article
Language:English
Subjects:
Algebra
Asymptotic properties
Classical and Quantum Gravitation
Cosmological constant
Elementary Particles
Flats
Gages
Gravitation
High energy physics
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Quantum Physics
Relativity Theory
String Theory
Symmetry
Three dimensional
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cited_by cdi_FETCH-LOGICAL-c455t-c20a7d143f5ec70394eceac01990c8d2b897b2d503105d4b39ceb5e4350a18363
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description A bstract 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 BMS 3 algebra with an appropriate central extension. It is also shown that our results can be recovered from the ones recently found for asymptotically AdS 3 spacetimes by virtue of a suitable gauge choice that allows to perform the vanishing cosmological constant limit.
doi_str_mv 10.1007/JHEP09(2013)016
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subjects Algebra
Asymptotic properties
Classical and Quantum Gravitation
Cosmological constant
Elementary Particles
Flats
Gages
Gravitation
High energy physics
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Quantum Physics
Relativity Theory
String Theory
Symmetry
Three dimensional
title Asymptotically flat spacetimes in three-dimensional higher spin gravity
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