Quasi-topological gravities on general spherically symmetric metric

Abstract In this work we study a more restricted class of quasi-topological gravity theories where the higher curvature terms have no contribution to the equation of motion on general static spherically symmetric metric where g tt g rr ≠ constant. We construct such theories up to quintic order in Ri...

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Main Author: Feiyu Chen
Format: Article
Language:English
Published: SpringerOpen 2023-03-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP03(2023)055
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author Feiyu Chen
author_facet Feiyu Chen
author_sort Feiyu Chen
collection DOAJ
description Abstract In this work we study a more restricted class of quasi-topological gravity theories where the higher curvature terms have no contribution to the equation of motion on general static spherically symmetric metric where g tt g rr ≠ constant. We construct such theories up to quintic order in Riemann tensor and observe an important property of these theories: the higher order term in the Lagrangian vanishes identically when evaluated on the most general non-stationary spherically symmetric metric ansatz. This not only signals the higher terms could only have non-trivial effects when considering perturbations, but also makes the theories quasi-topological on a much wider range of metrics. As an example of the holographic effects of such theories, we consider a general Einstein-scalar theory and calculate it’s holographic shear viscosity.
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spelling doaj.art-ba35ce0492cd4937afecc3ba5e2035752023-06-25T11:05:56ZengSpringerOpenJournal of High Energy Physics1029-84792023-03-012023312710.1007/JHEP03(2023)055Quasi-topological gravities on general spherically symmetric metricFeiyu Chen0Institute of High Energy Physics, Chinese Academy of SciencesAbstract In this work we study a more restricted class of quasi-topological gravity theories where the higher curvature terms have no contribution to the equation of motion on general static spherically symmetric metric where g tt g rr ≠ constant. We construct such theories up to quintic order in Riemann tensor and observe an important property of these theories: the higher order term in the Lagrangian vanishes identically when evaluated on the most general non-stationary spherically symmetric metric ansatz. This not only signals the higher terms could only have non-trivial effects when considering perturbations, but also makes the theories quasi-topological on a much wider range of metrics. As an example of the holographic effects of such theories, we consider a general Einstein-scalar theory and calculate it’s holographic shear viscosity.https://doi.org/10.1007/JHEP03(2023)055AdS-CFT CorrespondenceBlack HolesClassical Theories of Gravity
spellingShingle Feiyu Chen
Quasi-topological gravities on general spherically symmetric metric
Journal of High Energy Physics
AdS-CFT Correspondence
Black Holes
Classical Theories of Gravity
title Quasi-topological gravities on general spherically symmetric metric
title_full Quasi-topological gravities on general spherically symmetric metric
title_fullStr Quasi-topological gravities on general spherically symmetric metric
title_full_unstemmed Quasi-topological gravities on general spherically symmetric metric
title_short Quasi-topological gravities on general spherically symmetric metric
title_sort quasi topological gravities on general spherically symmetric metric
topic AdS-CFT Correspondence
Black Holes
Classical Theories of Gravity
url https://doi.org/10.1007/JHEP03(2023)055
work_keys_str_mv AT feiyuchen quasitopologicalgravitiesongeneralsphericallysymmetricmetric