Euclidean action for vacuum decay in a de Sitter universe
V. Balek, M. Demetrian

TL;DR
This paper derives approximate formulas for the Euclidean action of near-to-limit instantons in de Sitter space, analyzing how their properties influence vacuum decay outcomes and comparing different instanton solutions.
Contribution
It provides new analytical approximations for the Euclidean action of near-to-limit instantons in de Sitter space, clarifying their role in vacuum decay.
Findings
First-order instantons can dominate vacuum decay if their action is less than Hawking-Moss.
The correction to Hawking-Moss action depends on the instanton's order and scalar field amplitude.
Numerical results confirm the dominance of first-order Coleman-de Luccia instantons in certain potentials.
Abstract
The behavior of the action of the instantons describing vacuum decay in a de Sitter is investigated. For a near-to-limit instanton (a Coleman-de Luccia instanton close to some Hawking-Moss instanton) we find approximate formulas for the Euclidean action by expanding the scalar field and the metric of the instanton in the powers of the scalar field amplitude. The order of the magnitude of the correction to the Hawking-Moss action depends on the order of the instanton (the number of crossings of the barrier by the scalar field): for instantons of odd and even orders the correction is of the fourth and third order in the scalar field amplitude, respectively. If a near-to-limit instanton of the first order exists in a potential with the curvature at the top of the barrier greater than 4 (Hubble constant), which is the case if the fourth derivative of the potential at the top of…
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