Holographic Studies of The Generic Massless Cubic Gravities
arXiv:1901.03349 · doi:10.1103/PhysRevD.99.066014
Abstract
We consider the generic massless cubic gravities coupled to a negative bare cosmological constant mainly in and dimensions, which are Einstein gravity extended with cubic curvature invariants where the linearized excited spectrum around the AdS background contains no massive modes. The generic massless cubic gravities are more general than Myers quasi-topological gravity in and Einsteinian cubic gravity in . It turns out that the massless cubic gravities admit the black holes at least in a perturbative sense with the coupling constants of the cubic terms becoming infinitesimal. The first order approximate black hole solutions with arbitrary boundary topology are presented, and in addition, the second order approximate planar black holes are exhibited as well. We then establish the holographic dictionary for such theories by presenting -charge, -charge and energy flux parameters and . By perturbatively discussing the holographic Rényi entropy, we find , and can somehow determine the Rényi entropy with the limit , and up to the first order, where is the order of the Rényi entropy. For holographic hydrodynamics, we discuss the shear-viscosity-entropy-ratio and find that the patterns deviating from the KSS bound can somehow be controlled by up to the first order in , and up to the second order in , where and differ from -charge and -charge by inessential overall constants.
Latex, 69 pages, typo corrected, comments and references added, to appear in PRD
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