Abstract:Abstract:We study the non-perturbative renormalisation of quantum gravity in four dimensions. Taking care to disentangle physical degrees of freedom, we observe the topological nature of conformal fluctuations arising from the functional measure. The resulting beta functions possess an asymptotically safe fixed point with a global phase structure leading to classical general relativity for positive, negative or vanishing cosmological constant. If only the conformal fluctuations are quantised we find an asympto… Show more
“…Note, that the evaluation of the two-point function at M 2 = 0 ensures that only the momentum dependent part of the latter enters for the class of regulators defined by (31). Since the effective graviton mass M 2 is the only mass parameter in the present truncation the above definition implies that Γ (22). This generic class covers the regulator choices in the literature, and implements the correct renormalisation group scaling of the effective action as discussed in [8,41,60].…”
Section: Anomalous Dimensions and Bounds For The Generic Class Of mentioning
confidence: 92%
“…Here d is the dimension of spinor space, which we set to d = 4 throughout. Since (22), (26) and (28) are of the same form, we apply the same bilocal momentum projection for the extraction of the respective momentum dependent anomalous dimensions. This crucial procedure is discussed in more detail in the next section.…”
Section: B Gravity Contributions To Matter Flowsmentioning
confidence: 99%
“…The development of modern functional renormalisation group (FRG) techniques and their application to quantum gravity [3,4] has led to strong evidence for the nontrivial UV fixed point for pure gravity. It was first found in basic Einstein-Hilbert approximations [3,5,6] and later confirmed in more elaborate truncations [1,[7][8][9][10][11][12][13][14][15][16][17][18][19][20][21][22][23][24], for reviews see [25][26][27][28].…”
We study the ultraviolet stability of gravity-matter systems for general
numbers of minimally coupled scalars and fermions. This is done within the
functional renormalisation group setup put forward in
\cite{Christiansen:2015rva} for pure gravity. It includes full dynamical
propagators and a genuine dynamical Newton's coupling, which is extracted from
the graviton three-point function.
We find ultraviolet stability of general gravity-fermion systems.
Gravity-scalar systems are also found to be ultraviolet stable within validity
bounds for the chosen generic class of regulators, based on the size of the
anomalous dimension. Remarkably, the ultraviolet fixed points for the dynamical
couplings are found to be significantly different from those of their
associated background counterparts, once matter fields are included. In
summary, the asymptotic safety scenario does not put constraints on the matter
content of the theory within the validity bounds for the chosen generic class
of regulators.Comment: 19 pages, 10 figure
“…Note, that the evaluation of the two-point function at M 2 = 0 ensures that only the momentum dependent part of the latter enters for the class of regulators defined by (31). Since the effective graviton mass M 2 is the only mass parameter in the present truncation the above definition implies that Γ (22). This generic class covers the regulator choices in the literature, and implements the correct renormalisation group scaling of the effective action as discussed in [8,41,60].…”
Section: Anomalous Dimensions and Bounds For The Generic Class Of mentioning
confidence: 92%
“…Here d is the dimension of spinor space, which we set to d = 4 throughout. Since (22), (26) and (28) are of the same form, we apply the same bilocal momentum projection for the extraction of the respective momentum dependent anomalous dimensions. This crucial procedure is discussed in more detail in the next section.…”
Section: B Gravity Contributions To Matter Flowsmentioning
confidence: 99%
“…The development of modern functional renormalisation group (FRG) techniques and their application to quantum gravity [3,4] has led to strong evidence for the nontrivial UV fixed point for pure gravity. It was first found in basic Einstein-Hilbert approximations [3,5,6] and later confirmed in more elaborate truncations [1,[7][8][9][10][11][12][13][14][15][16][17][18][19][20][21][22][23][24], for reviews see [25][26][27][28].…”
We study the ultraviolet stability of gravity-matter systems for general
numbers of minimally coupled scalars and fermions. This is done within the
functional renormalisation group setup put forward in
\cite{Christiansen:2015rva} for pure gravity. It includes full dynamical
propagators and a genuine dynamical Newton's coupling, which is extracted from
the graviton three-point function.
We find ultraviolet stability of general gravity-fermion systems.
Gravity-scalar systems are also found to be ultraviolet stable within validity
bounds for the chosen generic class of regulators, based on the size of the
anomalous dimension. Remarkably, the ultraviolet fixed points for the dynamical
couplings are found to be significantly different from those of their
associated background counterparts, once matter fields are included. In
summary, the asymptotic safety scenario does not put constraints on the matter
content of the theory within the validity bounds for the chosen generic class
of regulators.Comment: 19 pages, 10 figure
“…The absence of a mass-like term in the "on-shell" propagator of the graviton is well known in general relativity and cosmology and has been discussed for the renormalization flow in refs. [53,54]. It is at the origin of scepticism about the relevance of the "avoidance of instabilities" for observable cosmology.…”
Section: Flow On Cosmological Backgroundsmentioning
Graviton fluctuations induce strong non-perturbative infrared renormalization
effects for the cosmological constant. The functional renormalization flow
drives a positive cosmological constant towards zero, solving the cosmological
constant problem without the need to tune parameters. We propose a simple
computation of the graviton contribution to the flow of the effective potential
for scalar fields. Within variable gravity we find that the potential increases
asymptotically at most quadratically with the scalar field. With effective
Planck mass proportional to the scalar field, the solutions of the derived
cosmological equations lead to an asymptotically vanishing cosmological
"constant" in the infinite future, providing for dynamical dark energy in the
present cosmological epoch. Beyond a solution of the cosmological constant
problem, our simplified computation also entails a sizeable positive
graviton-induced anomalous dimension for the quartic Higgs coupling in the
ultraviolet regime, substantiating the successful prediction of the Higgs boson
mass within the asymptotic safety scenario for quantum gravity.Comment: extended discussion, new references, 14 pages, 2 figure
“…for gravity with matters and gauge fields ; for higher derivative gravity with f (R)type truncation [71][72][73][74][75][76][77][78][79][80][81][82][83][84]; R µν R µν [85][86][87][88][89][90][91][92]; and the Goroff-Sagnotti term [93]; see also [94][95][96][97][98][99][100] for review papers. 5 Also studies based on the vertex expansion have been performed in [125][126][127][128][129][130][131][132].…”
Abstract:We study asymptotic safety of models of the higher derivative quantum gravity with and without matter. The beta functions are derived by utilizing the functional renormalization group, and non-trivial fixed points are found. It turns out that all couplings in gravity sector, namely the cosmological constant, the Newton constant, and the R 2 and R 2 µν coupling constants, are relevant in case of higher derivative pure gravity. For the Higgs-Yukawa model non-minimal coupled with higher derivative gravity, we find a stable fixed point at which the scalar-quartic and the Yukawa coupling constants become relevant. The relevant Yukawa coupling is crucial to realize the finite value of the Yukawa coupling constants in the standard model.
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