Solutions to Horava Gravity
arXiv:0904.1595 · doi:10.1103/PhysRevLett.103.091301
Abstract
Recently Horava proposed a non-relativistic renormalisable theory of gravitation, which reduces to Einstein's general relativity at large distances, and that may provide a candidate for a UV completion of Einstein's theory. In this paper, we derive the full set of equations of motion, and then we obtain spherically symmetric solutions and discuss their properties. We also obtain solutions for the Friedman-Lemaitre-Robertson-Walker cosmological metric.
Latex, 8 pages, version to appear in Phys. Rev. Lett
References in corpus (7)
- Quantum Gravity at a Lifshitz Point
- Spectral Dimension of the Universe in Quantum Gravity at a Lifshitz Point
- Membranes at Quantum Criticality
- Horava-Lifshitz Cosmology
- Chiral Primordial Gravitational Waves from a Lifshitz Point
- Phenomenologically viable Lorentz-violating quantum gravity
- Correlation Functions in Non-Relativistic Holography
Cited by in corpus (13)
- Strong coupling in Horava gravity
- Thermodynamics of Black Holes in Horava-Lifshitz Gravity
- The Black Hole and Cosmological Solutions in IR modified Horava Gravity
- On the z=4 Horava-Lifshitz Gravity
- Towards constraining of the Horava-Lifshitz gravities
- Caustic avoidance in Horava-Lifshitz gravity
- On IR solutions in Horava gravity theories
- Anisotropic Cosmology and (Super)Stiff Matter in Hořava's Gravity Theory
- Generalized uncertainty principle and Hořava-Lifshitz gravity
- Strong Coupling Quantum Einstein Gravity at a z=2 Lifshitz Point
- Quintessence and phantom dark energy from ghost D-branes
- A Note on Quasi-Riemannian Gravity with Higher Derivatives
- Power spectra of scalar and tensor modes in modified Horava-Lifshitz gravity