Causality in 3D massive gravity theories

We study the constraints coming from the local causality requirement in various 2+1 dimensional dynamical theories of gravity. In topologically massive gravity, with a single parity noninvariant massive degree of freedom, and in new massive gravity, with two massive spin-2 degrees of freedom, causal...

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Publicado: 2017
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_24700010_v95_n10_p_Edelstein
http://hdl.handle.net/20.500.12110/paper_24700010_v95_n10_p_Edelstein
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spelling paper:paper_24700010_v95_n10_p_Edelstein2023-06-08T16:36:28Z Causality in 3D massive gravity theories We study the constraints coming from the local causality requirement in various 2+1 dimensional dynamical theories of gravity. In topologically massive gravity, with a single parity noninvariant massive degree of freedom, and in new massive gravity, with two massive spin-2 degrees of freedom, causality and unitarity are compatible with each other and both require the Newton's constant to be negative. In their extensions, such as the Born-Infeld gravity and the minimal massive gravity the situation is similar and quite different from their higher dimensional counterparts, such as quadratic (e.g., Einstein-Gauss-Bonnet) or cubic theories, where causality and unitarity are in conflict. We study the problem both in asymptotically flat and asymptotically anti-de Sitter spaces. © 2017 American Physical Society. 2017 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_24700010_v95_n10_p_Edelstein http://hdl.handle.net/20.500.12110/paper_24700010_v95_n10_p_Edelstein
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description We study the constraints coming from the local causality requirement in various 2+1 dimensional dynamical theories of gravity. In topologically massive gravity, with a single parity noninvariant massive degree of freedom, and in new massive gravity, with two massive spin-2 degrees of freedom, causality and unitarity are compatible with each other and both require the Newton's constant to be negative. In their extensions, such as the Born-Infeld gravity and the minimal massive gravity the situation is similar and quite different from their higher dimensional counterparts, such as quadratic (e.g., Einstein-Gauss-Bonnet) or cubic theories, where causality and unitarity are in conflict. We study the problem both in asymptotically flat and asymptotically anti-de Sitter spaces. © 2017 American Physical Society.
title Causality in 3D massive gravity theories
spellingShingle Causality in 3D massive gravity theories
title_short Causality in 3D massive gravity theories
title_full Causality in 3D massive gravity theories
title_fullStr Causality in 3D massive gravity theories
title_full_unstemmed Causality in 3D massive gravity theories
title_sort causality in 3d massive gravity theories
publishDate 2017
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_24700010_v95_n10_p_Edelstein
http://hdl.handle.net/20.500.12110/paper_24700010_v95_n10_p_Edelstein
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