New type of hill-top inflation
A.O. Barvinsky, A.Yu. Kamenshchik, D.V. Nesterov

TL;DR
This paper introduces a novel hill-top inflation model based on initial conditions from a microcanonical density matrix, involving cosmological instantons and oscillations, with potential shapes generated by quantum corrections in specific gravity models.
Contribution
It proposes a new hill-top inflation scenario derived from initial conditions set by cosmological instantons and explores its realization in non-minimal Higgs inflation and $R^2$-gravity models.
Findings
Initial conditions from microcanonical density matrix lead to hill-top inflation.
Oscillatory instanton solutions describe underbarrier inflaton dynamics.
Logarithmic loop corrections shape the inflaton potential.
Abstract
We suggest a new type of hill-top inflation originating from the initial conditions in the form of the microcanonical density matrix for the cosmological model with a large number of quantum fields conformally coupled to gravity. Initial conditions for inflation are set up by cosmological instantons describing underbarrier oscillations in the vicinity of the inflaton potential maximum. These periodic oscillations of the inflaton field and cosmological scale factor are obtained within the approximation of two coupled oscillators subject to the slow roll regime in the Euclidean time. This regime is characterized by rapid oscillations of the scale factor on the background of a slowly varying inflaton, which guarantees smallness of slow roll parameters and of the following inflation stage. A hill-like shape of the inflaton potential is shown to be generated by logarithmic…
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