The infrared-safe Minkowskian Curci-Ferrari model

Abstract

We discuss the existence of Landau-pole-free renormalization group trajectories in the Minkowskian version of the Curci-Ferrari model as a function of a running parameter q2 associated to the four-vector q at which renormalization conditions are imposed, and which can take both space-like (q2<0) and time-like (q2>0) values. We discuss two possible extensions of the infrared-safe scheme defined in Ref. [Phys. Rev. D, 84, 045018, 2011] for the Euclidean version of the model, which coincide with the latter in the space-like region upon identifying Q2-q2 with the square of the renormalization scale in that reference. The first extension uses real-valued renormalization factors and leads to a flow in the time-like region with a similar structure as the flow in the space-like region (or in the Euclidean model), including a non-trivial fixed point and a family of trajectories bounded at all scales by the value of the coupling at this fixed point. Interestingly, the fixed point in the time-like region has a much smaller value of λ g2N/16π2 than the corresponding one in the space-like region, a value closer to the perturbative boundary λ=1. However, in this real-valued infrared-safe scheme, the flow cannot connect the time-like and space-like regions. Thus, it is not possible to deduce the relevant time-like flow trajectory from the sole knowledge of a space-like flow trajectory. To try to cure this problem, we investigate a second extension of the Euclidean IR-safe scheme, which allows for complex-valued renormalization factors. We discuss under which conditions these schemes can make sense and study their ability to connect space- and time-like flow trajectories. In particular, we investigate to which types of time-like trajectories the perturbative space-like trajectories are mapped onto.

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