Solutions of massive gravity theories in constant scalar invariant geometries

Abstract

We solve massive gravity field equations in the framework of locally homogenous and vanishing scalar invariant (VSI) Lorentzian spacetimes, which in three dimensions are the building blocks of constant scalar invariant (CSI) spacetimes. At first, we provide an exhaustive list of all Lorentzian three-dimensional homogeneous spaces and then we determine the Petrov type of the relevant curvature tensors. Among these geometries we determine for which values of their structure constants they are solutions of the field equations of massive gravity theories with cosmological constant. The homogeneous solutions founded are of all various Petrov types : I_C, I_R, II, III, D_t, D_s, N, O; the VSI geometries which we found are of Petrov type III. The Petrov types II and III are new explicit CSI spacetimes solutions of these types. We also examine the conditions under which the obtained anti-de Sitter solutions are free of tachyonic massive graviton modes.

v3: Latex, 42 pages, 4 figures; fixed typos and added sentences

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• Massive Gravity in Three Dimensions
• Warped AdS_3 Black Holes
• More on Massive 3D Gravity
• Ghost-free, finite, fourth order D=3 (alas) gravity
• Lorentzian spacetimes with constant curvature invariants in four dimensions
• On the Generalized Massive Gravity in $Ad{S}_3$
• Renormalizability of Massive Gravity in Three Dimensions
• Homogeneous anisotropic solutions of topologically massive gravity with cosmological constant and their homogeneous deformations

Cited by in corpus (4)

• Critical solutions in topologically gauged N=8 CFTs in three dimensions
• Conserved charges in timelike Warped-AdS${}_3$ spaces
• Kundt solutions of Minimal Massive 3D Gravity
• Homogeneous Solutions of Minimal Massive 3D Gravity