New Improved Massive Gravity and Three Dimensional Spacetimes of Constant Curvature and Constant Torsion
arXiv:1604.00463 · doi:10.1103/PhysRevD.94.064067
Abstract
We derive the field equations for topologically massive gravity coupled with the most general quadratic curvature terms using the language of exterior differential forms and a first order constrained variational principle. We find variational field equations both in the presence and absence of torsion. We then show that spaces of constant negative curvature (i.e. the anti de-Sitter space ) and constant torsion provide exact solutions.
16 pages
References in corpus (11)
- Massive Gravity in Three Dimensions
- More on Massive 3D Gravity
- Ghost-free, finite, fourth order D=3 (alas) gravity
- Minimal Massive 3D Gravity
- Minimal Massive Gravity: Conserved Charges, Excitations and the Chiral Gravity Limit
- Extended massive gravity in three dimensions
- On 3D Minimal Massive Gravity
- On Solutions of Minimal Massive 3D Gravity
- On Exact Solutions and the Consistency of 3D Minimal Massive Gravity
- An alternative derivation of the Minimal massive 3D gravity
- Holographically Viable Extensions of Topologically Massive and Minimal Massive Gravity?
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- A note on the pp-wave solution of Minimal Massive 3D Gravity coupled with Maxwell-Chern-Simons theory