Abstract
We compute the β functions of marginal couplings in projectable Hořava gravity in 2+1 spacetime dimensions. We show that the renormalization group flow has an asymptotically free fixed point in the ultraviolet (UV), establishing the theory as a UV-complete model with dynamical gravitational degrees of freedom. Therefore, this theory may serve as a toy model to study fundamental aspects of quantum gravity. Our results represent a step forward towards understanding the UV properties of realistic versions of Hořava gravity.
Original language | English |
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Pages (from-to) | 211301 |
Number of pages | 1 |
Journal | Physical Review Letters |
Volume | 119 |
Early online date | 20 Nov 2017 |
DOIs | |
Publication status | Published - 24 Nov 2017 |
Keywords
- High Energy Physics - Theory, General Relativity and Quantum Cosmology