
TL;DR
This paper investigates the construction, stability, and dominance of Euclidean wormholes in AdS spaces across various models, revealing stable solutions that resemble phase transitions but also face instabilities in UV-complete theories, impacting AdS/CFT factorization.
Contribution
It demonstrates the existence of stable, dominant Euclidean wormholes in simple models and explores their stability issues in string compactifications, advancing understanding of their role in holography.
Findings
Stable wormholes exist in simple AdS models and resemble Hawking-Page transitions.
In string compactifications, wormholes are stable but suffer from brane-nucleation instabilities.
Additional solutions with lower action suggest factorization challenges in AdS/CFT.
Abstract
We explore the construction and stability of asymptotically anti-de Sitter Euclidean wormholes in a variety of models. In simple ad hoc low-energy models, it is not hard to construct two-boundary Euclidean wormholes that dominate over disconnected solutions and which are stable (lacking negative modes) in the usual sense of Euclidean quantum gravity. Indeed, the structure of such solutions turns out to strongly resemble that of the Hawking-Page phase transition for AdS-Schwarzschild black holes, in that for boundary sources above some threshold we find both a `large' and a `small' branch of wormhole solutions with the latter being stable and dominating over the disconnected solution for large enough sources. We are also able to construct two-boundary Euclidean wormholes in a variety of string compactifications that dominate over the disconnected solutions we find and that are stable…
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