Abstract:Realizing a quantum theory for gravity based on Asymptotic Safety hinges on the existence of a non-Gaussian fixed point of the theory's renormalization group flow. In this work, we use the functional renormalization group equation for the effective average action to study the fixed point underlying Quantum Einstein Gravity at the functional level including an infinite number of scale-dependent coupling constants. We formulate a list of guiding principles underlying the construction of a partial differential eq… Show more
“…On the other hand, no ghosts are present in [22]. In spite of these differences, the equation of [22] was shown in [23] to have a global scaling solution whose general shape is quite similar to ours. The equation for unimodular gravity has only been analyzed at polynomial level so far.…”
Section: Discussionsupporting
confidence: 65%
“…In the Hessian on the four-sphere (2.11), the operator = −∇ 2 appears everywhere and is a natural choice. However, in order to gain some additional freedom, we follow [22,23] and add to terms proportional to the scalar curvature, with coefficients −α, −γ , and −β for spin two, one, and zero, respectively. These parameters should not be confused with the gauge fixing parameters which do not appear in the following.…”
Section: Cutoff and Functional Renormalization Group Equationmentioning
confidence: 99%
“…The heat kernel coefficients b 2n for acting on spin two, one, and zero are given in [12,23] for type I cutoff. We extend the calculation to our case and give the results in Appendix C. Substituting these heat kernel coefficients and Eqs.…”
Section: Four Dimensionsmentioning
confidence: 99%
“…This is a general issue that goes beyond the f (R) truncations and progress in this direction has been made in [19,20]. In the meantime solutions were found in simplified (lower-dimensional and/or conformally reduced) settings [21,22] and recently also in the full four-dimensional case [23].…”
We employ the exponential parametrization of the metric and a "physical" gauge fixing procedure to write a functional flow equation for the gravitational effective average action in an f (R) truncation. The background metric is a four-sphere and the coarse-graining procedure contains three free parameters. We look for scaling solutions, i.e. nonGaussian fixed points for the function f . For a discrete set of values of the parameters, we find simple global solutions of quadratic polynomial form. For other values, global solutions can be found numerically. Such solutions can be extended in certain regions of parameter space and have two relevant directions. We discuss the merits and the shortcomings of this procedure.
“…On the other hand, no ghosts are present in [22]. In spite of these differences, the equation of [22] was shown in [23] to have a global scaling solution whose general shape is quite similar to ours. The equation for unimodular gravity has only been analyzed at polynomial level so far.…”
Section: Discussionsupporting
confidence: 65%
“…In the Hessian on the four-sphere (2.11), the operator = −∇ 2 appears everywhere and is a natural choice. However, in order to gain some additional freedom, we follow [22,23] and add to terms proportional to the scalar curvature, with coefficients −α, −γ , and −β for spin two, one, and zero, respectively. These parameters should not be confused with the gauge fixing parameters which do not appear in the following.…”
Section: Cutoff and Functional Renormalization Group Equationmentioning
confidence: 99%
“…The heat kernel coefficients b 2n for acting on spin two, one, and zero are given in [12,23] for type I cutoff. We extend the calculation to our case and give the results in Appendix C. Substituting these heat kernel coefficients and Eqs.…”
Section: Four Dimensionsmentioning
confidence: 99%
“…This is a general issue that goes beyond the f (R) truncations and progress in this direction has been made in [19,20]. In the meantime solutions were found in simplified (lower-dimensional and/or conformally reduced) settings [21,22] and recently also in the full four-dimensional case [23].…”
We employ the exponential parametrization of the metric and a "physical" gauge fixing procedure to write a functional flow equation for the gravitational effective average action in an f (R) truncation. The background metric is a four-sphere and the coarse-graining procedure contains three free parameters. We look for scaling solutions, i.e. nonGaussian fixed points for the function f . For a discrete set of values of the parameters, we find simple global solutions of quadratic polynomial form. For other values, global solutions can be found numerically. Such solutions can be extended in certain regions of parameter space and have two relevant directions. We discuss the merits and the shortcomings of this procedure.
“…However this is also an area where there is little guidance from current experimental observation or other techniques, and therefore one must place particular reliance on a rigorous understanding of the mathematical structure that the exact RG exposes, in so far as this is possible. This is especially so with recent work on "functional truncations" [17][18][19][20][21][22][23][24][25][26][27][28][29][30][31][32][33][34][35][36].…”
We present an exact RG (renormalization group) analysis of O(N )-invariant scalar field theory about the Gaussian fixed point. We prove a series of statements that taken together show that the non-polynomial eigen-perturbations found in the LPA (local potential approximation) at the linearised level, do not lead to new interactions, i.e. enlarge the universality class, neither in the LPA or treated exactly. Non-perturbatively, their RG flow does not emanate from the fixed point. For the equivalent Wilsonian effective action they can be re-expressed in terms of the usual couplings to polynomial interactions, which can furthermore be tuned to be as small as desired for all finite RG time. For the infrared cutoff Legendre effective action, this can also be done for the infrared evolution. We explain why this is nevertheless consistent with the fact that the large field behaviour is fixed by these perturbations.arXiv:1605.06075v3 [hep-th]
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