Stochastic Quantization of the Hořava Gravity
arXiv:0906.1645
Abstract
The stochastic quantization method is applied to the recent proposal by Hořava for gravity. We show that in contrast to General Relativity, the Hořava's action, satisfying the detailed balance condition, has a stable, non-perturbative quantum vacuum when the DeWitt parameter is not greater than 1/3, providing a possible candidate for consistent quantum gravity.
5 pages
Cited by in corpus (6)
- Phase-space analysis of Horava-Lifshitz cosmology
- Holographic dark energy with varying gravitational constant in Horava-Lifshitz cosmology
- A Test of Horava Gravity: The Dark Energy
- Quantization of the Horava theory at the kinetic-conformal point
- Cosmological Perturbations in the Projectable Version of Horava-Lifshitz Gravity
- Wave zone in the Hořava-Lifshitz theory at the kinetic-conformal point in the low energy regime