Constraining quantum gravity from observations is a challenge. We expand on the idea that the interplay of quantum gravity with matter could be key to meeting this challenge.Thus, we set out to confront different potential candidates for quantum gravity -unimodular asymptotic safety, Weyl-squared gravity and asymptotically safe gravity -with constraints arising from demanding an ultraviolet complete Standard Model. Specifically, we show that within approximations, demanding that quantum gravity solves the Landau-pole problems in Abelian gauge couplings and Yukawa couplings strongly constrains the viable gravitational parameter space. In the case of Weyl-squared gravity with a dimensionless gravitational coupling, we also investigate whether the gravitational contribution to beta functions in the matter sector calculated from functional Renormalization Group techniques is universal, by studying the dependence on the regulator, metric field parameterization and choice of gauge.
I. INTRODUCTIONObservational constraints on quantum gravity are hard to come by. Based on a simple dimensional argument, one typically expects a power-law suppression of quantum-gravity effects 1 with (E/M Pl ) # , with E being the energy scale relevant for experiments, M Pl being the Planck mass and # > 0. Nevertheless, mathematical and internal consistency are not the only conditions that could * Electronic address: gpbrito@cbpf.br † Electronic address: eichhorn@sdu.dk ‡ Electronic address: adpjunior@id.uff.br 1 In the presence of a second "meso"-scale, as hinted at by some quantum-gravity approaches, e.g., [1], this situation can change.