Note About Equivalence of F(R) and Scalar Tensor Horava-Lifshitz Gravities
arXiv:1107.5660 · doi:10.1103/PhysRevD.84.104014
Abstract
In this note we study the relation between F(R) and scalar tensor Horava-Lifshitz gravity. We find that due to the broken diffeomorphism invariance corresponding scalar tensor theory has more complicated form than in case of the full diffeomorphism invariant F(R) theory of gravity. We also show that in the low energy limit this theory flows to the relativistic scalar tensor theory of gravity.
12 pages,v2: references added
References in corpus (16)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- Quantum Gravity at a Lifshitz Point
- Membranes at Quantum Criticality
- Horava-Lifshitz Cosmology
- Horava-Lifshitz Cosmology: A Review
- Cosmology of the Lifshitz universe
- Dark Energy: the equation of state description versus scalar-tensor or modified gravity
- Horava-Lifshitz gravity: a status report
- 3+1 Formalism and Bases of Numerical Relativity
- General Covariance in Gravity at a Lifshitz Point
- Projectable Horava-Lifshitz gravity in a nutshell
- The good, the bad and the ugly .... of Horava gravity
- Status of Horava gravity: A personal perspective
- Detailed balance condition and ultraviolet stability of scalar field in Horava-Lifshitz gravity
- theory and geometric origin of the dark sector in Horava-Lifshitz gravity
- 3+1 Orthogonal and Conformal Decomposition of the Einstein Equation and the ADM Formalism for General Relativity