The $\bar{\Lambda}CDM$ cosmology: from inflation to dark energy through running $\Lambda$
Joan Sola, Adria Gomez-Valent

TL;DR
This paper proposes a unified dynamical vacuum model that explains inflation, radiation, matter, and dark energy phases of the universe, aligning with observations and offering testable predictions.
Contribution
It introduces a single vacuum structure, $ar{ extLambda}(H)$, that naturally incorporates inflation and dark energy without separate mechanisms.
Findings
Model reproduces inflation, radiation, matter, and dark energy epochs.
Compatible with current cosmological data.
Predicts distinctive observational signatures.
Abstract
Perhaps the deepest mystery of our accelerating Universe in expansion is the existence of a tiny and rigid cosmological constant, . Its size is many orders of magnitude below the expected one in the standard model of particle physics. However, an expanding Universe is not expected to have a static vacuum energy density. We should rather observe a mildly dynamical behavior with the expansion rate . At the same time, it is natural to think that the huge value of the primeval vacuum energy (presumably connected to some grand unified theory) was responsible for the initial inflationary phase. In the traditional inflaton models such phase is inserted by hand in the early epoch of the cosmic evolution, and it is assumed to match the concordance CDM regime during the radiation epoch. Here, instead, we consider a class of dynamical vacuum…
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