Extended Hořava Gravity with Physical Ground-State Wavefunction
arXiv:1009.3677
Abstract
We propose a new extended theory of Hořava gravity based on the following three conditions: (i) UV completion, (ii) healthy IR behavior and (iii) a stable vacuum state in quantized version of the theory. Compared with other extended theories, we stress that any realistic theory of gravity must have physical ground states when quantization is performed. To fulfill the three conditions, we softly break the detailed balance but keep its basic structure unchanged. It turns out that the new model constructed in this way can avoid the strong coupling problem and remains power-counting renormalizable, moreover, it has a stable vacuum state by an appropriate choice of parameters.
15 pages,no figure
References in corpus (9)
- Quantum Gravity at a Lifshitz Point
- Spectral Dimension of the Universe in Quantum Gravity at a Lifshitz Point
- Horava-Lifshitz Cosmology
- Atom Interferometry tests of the isotropy of post-Newtonian gravity
- Black holes in asymptotically Lifshitz spacetime
- On IR solutions in Horava gravity theories
- Primordial perturbation with a modified dispersion relation
- Singularities in Horava-Lifshitz theory
- theory and geometric origin of the dark sector in Horava-Lifshitz gravity