Understand
Recent work has shown that non-local modifications of gravity involving terms such as $m^2R\Box^{-2}R$ (and no cosmological constant) provide a phenomenologically viable alternative to $\Lambda$CDM.
- We first discuss the possibility that such non-local terms emerge in the far infrared from the running of a coupling constant associated to the $R^2$ term in higher-derivative gravity, which, depending on the UV completion of the theory, can be asymptotically free in the ultraviolet and strongly coupled in the infrared.
- In this scenario the mass scale $m$ of the non-local model emerges from dimensional transmutation, similarly to $\Lambda_{\rm QCD}$ for strong interactions, leading to a technically natural value and to a novel understanding of the scale associated to dark energy.
- Motivated by these findings, we then explore the possibility of generating strong infrared effects in Einstein gravity, with no $R^2$ terms, as a consequence of the higher-derivative term generated by the conformal anomaly.