On the cutoff identification and the quantum improvement in asymptotically safe gravity
arXiv:1812.09135 · doi:10.1016/j.physletb.2019.04.062
Abstract
Applying the exact renormalization group method to search the nonGaussian fixed points of gravitational coupling, is frequently followed by two steps: cutoff identification and improvement. Although there are various models for identifying the cutoff momentum by some physical length, saving the general covariance should be considered as an important property in the procedure. In this paper, use of an arbitrary function of curvature invariants for cutoff identification is suggested. It is shown that the field equations for this approach differs from the ones obtained from the conventional cutoff identification and improvement, even for nonvacuum solutions of the improved Einstein equations. Indeed, it is concluded that these two steps are correlated to each other.
References in corpus (24)
- Nonperturbative Evolution Equation for Quantum Gravity
- Renormalization group improved black hole spacetimes
- Ultraviolet Fixed Point and Generalized Flow Equation of Quantum Gravity
- Non-Trivial Ultraviolet Fixed Point in Quantum Gravity
- Cosmology of the Planck Era from a Renormalization Group for Quantum Gravity
- Ultraviolet properties of f(R)-Gravity
- The Running Gravitational Couplings
- Spacetime Structure of an Evaporating Black Hole in Quantum Gravity
- Taming perturbative divergences in asymptotically safe gravity
- Renormalization group improved gravitational actions: a Brans-Dicke approach
- Asymptotically Safe Inflation
- Asymptotic safety of quantum gravity beyond Ricci scalars
- Black holes and asymptotically safe gravity
- Lectures on renormalization and asymptotic safety
- Aspects of asymptotic safety for quantum gravity
- Asymptotically safe inflation from quadratic gravity
- Quantum Improved Schwarzschild-(A)dS and Kerr-(A)dS Space-times
- An effective action for asymptotically safe gravity
- Towards conditions for black-hole singularity-resolution in asymptotically safe quantum gravity
- Cosmological bounds on the field content of asymptotically safe gravity-matter models
- Cosmic Censorship in Quantum Einstein Gravity
- Renormalization group scale-setting from the action - a road to modified gravity theories
- Vacuum energy and cosmological evolution
- On the effect of renormalization group improvement on the cosmological power spectrum
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- Geodesic Motions near an improved Schwarzschild black hole
- Generalized Ellis-Bronnikov wormholes in asymptotically safe gravity
- The effects of running gravitational coupling on three dimensional black holes
- On the quantum gravastar
- On the Lorentz symmetry in conformally reduced Quantum Gravity
- On the Quantum Improved Affine Gravity