Vacuum decay by p-branes production
Lorenzo Sindoni, Stefano Ansoldi

TL;DR
This paper generalizes the calculation of vacuum decay via p-brane nucleation in N-dimensional (anti-)de Sitter spacetimes using a semiclassical Euclidean approach.
Contribution
It extends previous models to higher dimensions and provides a method to compute the nucleation coefficient for spherical p-branes in these settings.
Findings
Derived a formula for p-brane nucleation coefficient in N dimensions
Applied semiclassical Euclidean methods to analyze vacuum decay
Generalized previous 4D results to higher-dimensional spacetimes
Abstract
We present a generalization to the N-dimensional case for the nucleation coefficient of a spherical p-brane, separating two (anti-)de Sitter spacetimes. We use a semiclassical approximation based on the analytical continuation to the Euclidean sector of a suitable effective action describing a p-brane in General Relativity.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
