Tunneling Potentials to Nothing
J.J. Blanco-Pillado, J.R. Espinosa, J. Huertas, K. Sousa

TL;DR
This paper uses the tunneling potential approach to analyze bubbles of nothing in compactified spacetimes, classifying different types and exploring their decay dynamics and interactions with vacuum decay.
Contribution
It introduces a simplified 4D tunneling potential framework to understand bubbles of nothing and categorizes four distinct types based on higher-dimensional theories.
Findings
Identified four classes of bubbles of nothing in various theories
Analyzed how bubbles of nothing decay and interact with vacuum decay
Provided a unified, simplified picture of these decay processes
Abstract
The catastrophic decay of a spacetime with compact dimensions, via bubbles of nothing (BoNs), is probably a generic phenomenon. BoNs admit a 4-dimensional description as singular Coleman-de Luccia bounces of the size modulus field, stabilized by some potential . We apply the tunneling potential approach to this 4d description to provide a very simple picture of BoNs. Using it we identify four different types of BoN, corresponding to different classes of higher dimensional theories. We study the quenching of BoN decays and their interplay with standard vacuum decays.
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Taxonomy
TopicsCosmology and Gravitation Theories · Quantum Mechanics and Applications · Dark Matter and Cosmic Phenomena
