Is asymptotically safe inflation eternal?

Recently, based on swampland considerations in string theory, the (no) eternal inflation principle has been put forward. The natural question arises whether similar conditions hold in other approaches to quantum gravity. In this article, the asymptotic safety hypothesis is considered in the context of eternal inflation. As exemplary inflationary models the SU(N) Yang-Mills in the Veneziano limit and various RG-improvements of the gravitational action are studied. The existence of UV fixed point generically flattens the potential and our findings suggest no tension between eternal inflation and asymptotic safety, both in the matter and gravitational sector in contradistinction to string theory. Moreover, the eternal inflation cannot take place in the range of applicability of effective field quantum gravity theory. We employ the analytical relations for eternal inflation to some of the models with single minima, such as Starobinsky inflation, alpha-attractors, or the RG-improved models and verify them with the massive numerical simulations. The validity of these constraints is also discussed for a multi-minima model.

Automated summary

This article explores the relationship between eternal inflation and the asymptotic safety hypothesis in other approaches to quantum gravity. It reveals that there is no tension between eternal inflation and asymptotic safety in both the matter and gravitational sectors, contrary to string theory. Additionally, it suggests that eternal inflation is not possible within the range of applicability of effective field quantum gravity theory.