Killing Vector Fields in Three Dimensions: A Method to Solve Massive Gravity Field Equations
arXiv:1001.1039 · doi:10.1088/0264-9381/27/20/205018
Abstract
Killing vector fields in three dimensions play important role in the construction of the related spacetime geometry. In this work we show that when a three dimensional geometry admits a Killing vector field then the Ricci tensor of the geometry is determined in terms of the Killing vector field and its scalars. In this way we can generate all products and covariant derivatives at any order of the ricci tensor. Using this property we give ways of solving the field equations of Topologically Massive Gravity (TMG) and New Massive Gravity (NMG) introduced recently. In particular when the scalars of the Killing vector field (timelike, spacelike and null cases) are constants then all three dimensional symmetric tensors of the geometry, the ricci and einstein tensors, their covariant derivatives at all orders, their products of all orders are completely determined by the Killing vector field and the metric. Hence the corresponding three dimensional metrics are strong candidates of solving all higher derivative gravitational field equations in three dimensions.
25 pages, some changes made and some references added, to be published in Classical and Quantum Gravity
References in corpus (13)
- Massive Gravity in Three Dimensions
- Warped AdS_3 Black Holes
- More on Massive 3D Gravity
- Ghost-free, finite, fourth order D=3 (alas) gravity
- Warped AdS_3 black holes in new massive gravity
- Bending AdS Waves with New Massive Gravity
- Classification of solutions in topologically massive gravity
- Three-dimensional Chern-Simons black holes
- Kundt spacetimes as solutions of topologically massive gravity
- Massive Higher Derivative Gravity in D-dimensional Anti-de Sitter Spacetimes
- Black holes with a null Killing vector in three-dimensional massive gravity
- Cosmology in three dimensions: steps towards the general solution
- Circular Symmetry in Topologically Massive Gravity
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- New Exact Solutions of Quadratic Curvature Gravity
- Chiral Massive News: Null Boundary Symmetries in Topologically Massive Gravity
- Some exact solutions of all f(Ricci) theories in three dimensions
- Weyl-Invariant Higher Curvature Gravity Theories in n Dimensions
- Type D Solutions of 3D New Massive Gravity
- All stationary axi-symmetric local solutions of topologically massive gravity
- On Exact Solutions and the Consistency of 3D Minimal Massive Gravity
- Asymptotically flat black holes in 2+1 dimensions
- Gravity Waves in Three Dimensions
- Extension of Kodama vector and quasilocal quantities in three-dimensional axisymmetric spacetimes
- Type N Spacetimes as Solutions of Extended New Massive Gravity
- Homogeneous anisotropic solutions of topologically massive gravity with cosmological constant and their homogeneous deformations
- Exotic Massive Gravity: Causality and a Birkhoff-like Theorem