Asymptotic freedom in Horava-Lifshitz gravity
arXiv:1406.4366 · doi:10.1103/PhysRevLett.113.171101
Abstract
We use the Wetterich equation for foliated spacetimes to study the RG flow of projectable Horava-Lifshitz gravity coupled to n Lifshitz scalars. Using novel results for anisotropic heat kernels, the matter-induced beta functions for the gravitational couplings are computed explicitly. The RG flow exhibits an UV attractive anisotropic Gaussian fixed point where Newton's constant vanishes and the extra scalar mode decouples. This fixed point ensures that the theory is asymptotically free in the large-n expansion, indicating that projectable Horava-Lifshitz gravity is perturbatively renormalizable. Notably, the fundamental fixed point action does not obey detailed balance.
4 pages, 2 figures
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- On power-counting renormalizability of Hořava gravity with detailed balance
- Quark stars with isotropic matter in Hořava gravity and Einstein-æther theory
- BFV quantization of the nonprojectable 2+1 Horava theory
- Quantum Lagrangian of the Horava theory and its nonlocalities