Abstract

We use the functional renormalization group equation for the effective average action to study the fixed point structure of gravity-fermion systems on a curved background spacetime. We approximate the effective average action by the Einstein-Hilbert action supplemented by a fermion kinetic term and a coupling of the fermion bilinears to the spacetime curvature. The latter interaction is singled out based on a “smart truncation building principle”. The resulting renormalization group flow possesses two families of interacting renormalization group fixed points extending to any number of fermions. The first family exhibits an upper bound on the number of fermions for which the fixed points could provide a phenomenologically interesting high-energy completion via the asymptotic safety mechanism. The second family comes without such a bound. The inclusion of the non-minimal gravity-matter interaction is crucial for discriminating the two families. Our work also clarifies the origin of the strong regulator-dependence of the fixed point structure reported in earlier literature and we comment on the relation of our findings to studies of the same system based on a vertex expansion of the effective average action around a flat background spacetime.

Highlights

  • Any realistic quantum theory for the gravitational interactions has to incorporate matter degrees of freedom in one way or another

  • A high-energy completion based on a non-Gaussian renormalization group fixed point (NGFP) from the family A may predict the low-energy value of α while for the fixed points in the family B this value corresponds to a free parameter which must be taken from experiment

  • The bold black line connecting the NGFPs acts as a boundary: renormalization group (RG) trajectories below this line are attracted to the Gaussian fixed point (GFP) as k → 0 while trajectories above this line typically terminate at a finite value of k

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Summary

Introduction

Any realistic quantum theory for the gravitational interactions has to incorporate matter degrees of freedom in one way or another. A crucial ingredient in developing phenomenologically interesting gravity-matter theories within the asymptotic safety program is the inclusion of fermionic degrees of freedom. An intriguing property of the background computations is the potential presence of a (regularization-procedure dependent) upper critical value on the number of fermions which, once exceeded, could impede the phenomenological viability of the corresponding NGFP This situation is rather unsatisfactory, since the number of fermions contained in the standard model of particle physics, N. The goal of this work is to provide a detailed analysis of this situation In this course, we identify and characterize a new one-parameter family of gravity-fermion fixed points which are invisible in approximations where the fermions are minimally coupled. Our computation employs the spinbase formalism developed in [68,69] and reviewed in [70]

General setup
Fermions minimally coupled to gravity
Smartly extending the effective average action
RG flows including the fermion-curvature coupling
Beta functions
Fixed-point structure of the extended system
Flow diagram and predictivity
Conclusions
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