Inflationary physics and transplanckian conjecture in the Stringy Running-Vacuum-Model: from the phantom vacuum to the true vacuum
Nick E. Mavromatos, Joan Sola

TL;DR
This paper extends a string-inspired cosmological model where gravitational anomalies and axions drive inflation, demonstrating a transition from a phantom vacuum to a true vacuum state consistent with trans-Planckian censorship, and addressing current cosmological tensions.
Contribution
It clarifies the roles of KR axions and gravitational Chern-Simons terms, showing their evolution from phantom to true vacuum within the RVM framework, and discusses implications for GW creation and cosmological tensions.
Findings
KR axion combined with Chern-Simons term obeys a $p=- ho$ equation of state with negative energy density.
The transition from phantom vacuum to true vacuum is facilitated by the Chern-Simons condensate.
Model is consistent with the trans-Planckian censorship hypothesis and may alleviate $ ext{Lambda}$CDM tensions.
Abstract
In previous works we have embedded the Running Vacuum Model (RVM) of Cosmology in the framework of string theory. Specifically, we considered a string-inspired Cosmology with primordial gravitational waves (GW) and gravitational anomalies, which were argued to lead, via appropriate condensation during the very-early-universe era, to dynamical inflation, of RVM type, without the need for extra inflaton fields. A crucial role for the associated slow-roll nature of the inflationary era was played by the fundamental axion field that exists in the gravitational multiplet of strings, viz. the Kalb-Ramond (KR) axion. In this paper, we study further this model and demonstrate several novel facts, completing our previous studies. We clarify the different roles played by the background KR axions, which constitute a form of stiff matter that dominates a pre-RVM-inflationary epoch of the Universe.…
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