Coleman-de Luccia reconsidered: a subtlety of gravity and the thin wall approximation
Keith Copsey

TL;DR
This paper revisits the Coleman-de Luccia tunnelling analysis, revealing that accounting for gravitational backreaction significantly increases decay rates of metastable vacua, challenging previous assumptions about the longevity of de Sitter spaces in string theory.
Contribution
It identifies a crucial subtlety in the thin-wall approximation that alters decay rate calculations by including gravitational backreaction effects.
Findings
Decay rates are much larger than previously thought.
High and not overly wide barriers lead to rapid decays.
Implications question the stability of de Sitter vacua in string theory.
Abstract
I point out that the usual Coleman-de Luccia analysis of tunnelling via instantons between perturbatively stable minima using the thin-wall approximation misses one of the effects of gravitational backreaction on the on-shell action and hence the decay rate. Once this oversight is corrected, one finds these decay rates are much larger than has been generally appreciated; including the effects of gravity potentials involving barriers which are relatively high and not overly wide result in decays which are quite rapid instead of slow. In the light of these results, it is no longer clear that one should believe string theory predicts a wide class of cosmologically long-lived metastable de Sitter vacua.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Particle physics theoretical and experimental studies
