Abstract

We investigate the asymptotic safety conjecture for quantum gravity including curvature invariants beyond Ricci scalars. Our strategy is put to work for families of gravitational actions which depend on functions of the Ricci scalar, the Ricci tensor, and products thereof. Combining functional renormalisation with high order polynomial approximations and full numerical integration we derive the renormalisation group flow for all couplings and analyse their fixed points, scaling exponents, and the fixed point effective action as a function of the background Ricci curvature. The theory is characterised by three relevant couplings. Higher-dimensional couplings show near-Gaussian scaling with increasing canonical mass dimension. We find that Ricci tensor invariants stabilise the UV fixed point and lead to a rapid convergence of polynomial approximations. We apply our results to models for cosmology and establish that the gravitational fixed point admits inflationary solutions. We also compare findings with those from $f(R)$-type theories in the same approximation and pin-point the key new effects due to Ricci tensor interactions. Implications for the asymptotic safety conjecture of gravity are indicated.

Highlights

  • It is widely acknowledged that for quantum field theories to be fundamental and predictive up to highest energies, their short-distance behavior should be controlled by an ultraviolet (UV) fixed point under the renormalization group [1,2]

  • We investigate the asymptotic safety conjecture for quantum gravity including curvature invariants beyond Ricci scalars

  • Our strategy is put to work for families of gravitational actions which depend on functions of the Ricci scalar, the Ricci tensor, and products thereof

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Summary

INTRODUCTION

It is widely acknowledged that for quantum field theories to be fundamental and predictive up to highest energies, their short-distance behavior should be controlled by an ultraviolet (UV) fixed point under the renormalization group [1,2]. Much unlike in non-Abelian gauge theories, proofs or theorems for asymptotic safety are presently not at hand This is largely due to the dimensional nature of Newton’s coupling whose canonical mass dimension must be compensated by large anomalous dimensions. In other words, evaluating the renormalization group equations on spaces with constant curvature is sufficient to find the running for all polynomial couplings of the theory, as well as the nonperturbative renormalization group flow of the functions F and Z. By and large, these ideas are similar to what had been done previously for fðRÞ type actions.

Main idea and approximations
Field decompositions
Gauge fixing and ghosts
Auxiliary fields
Gravitational path integral
Wilsonian momentum cutoff
TRACE COMPUTATION ALGORITHM
Heat kernels
Diagonal pieces
Nondiagonal pieces
DetðGφiφj Þ
Excluded modes
RICCI TENSOR EXPANSION
Hessian
Gravitational flow equation
INTERACTING FIXED POINTS
Classical fixed points
Quantum fixed points
Fixed point data
Universal coupling ratios
Beyond polynomial expansions
Scaling exponents
UNIVERSALITY AND SCALING EXPONENTS
Degeneracy
Bootstrap hypothesis
Testing asymptotic safety
Large order behavior
Origin of near-Gaussianity
VIII. FROM ASYMPTOTIC SAFETY TO COSMOLOGY
Stationarity of the quantum effective action
De Sitter and anti–de Sitter solutions
COMPARISON
SUMMARY
Constrained fields
Heat-kernel coefficients
Full Text
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