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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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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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 |
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I-28 |
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R-134 |
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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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1768544661561933824 |