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Published on: November 15, 2013
Asymptotic freedom in Hořava-Lifshitz gravity.
Giulio D'Odorico1, Frank Saueressig1, Marrit Schutten1
1Radboud University Nijmegen, Institute for Mathematics, Astrophysics and Particle Physics, Heyendaalseweg 135, 6525 AJ Nijmegen, The Netherlands.
Projectable Hořava-Lifshitz gravity coupled to Lifshitz scalars exhibits an asymptotically free renormalization group flow. This indicates perturbative renormalizability, though the fixed point action does not obey detailed balance.
Area of Science:
- Theoretical physics
- Quantum gravity
- Cosmology
Background:
- Hořava-Lifshitz gravity offers a potential framework for quantum gravity.
- Understanding its renormalization group flow is crucial for its consistency.
- Coupling to matter fields, like Lifshitz scalars, introduces complexities.
Purpose of the Study:
- To investigate the renormalization group flow of projectable Hořava-Lifshitz gravity.
- To analyze the impact of coupling to n Lifshitz scalars.
- To determine the theory's perturbative renormalizability and fixed-point behavior.
Main Methods:
- Application of the Wetterich equation for foliated spacetimes.
- Utilizing novel results for anisotropic heat kernels.
- Explicit computation of matter-induced beta functions for gravitational couplings.
Main Results:
- Identification of an UV attractive anisotropic Gaussian fixed point.
- Observation that Newton's constant vanishes at this fixed point.
- The extra scalar mode decouples, ensuring asymptotic freedom in the large-n expansion.
Conclusions:
- Projectable Hořava-Lifshitz gravity coupled to n Lifshitz scalars is perturbatively renormalizable.
- The identified fixed point suggests a viable high-energy behavior for the theory.
- The fundamental fixed point action deviates from the detailed balance condition.
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