Euclidean wormholes in holographic RG flows
Jeevan Chandra

TL;DR
This paper constructs Euclidean wormhole solutions in Einstein-dilaton gravity that connect two boundaries with different marginal couplings, analyzing how correlations between dual CFTs decay as the difference in couplings increases.
Contribution
It introduces a family of Euclidean wormholes in AdS that model the decorrelation of boundary CFTs with varying marginal couplings and computes related correlation function variances.
Findings
Wormhole volumes increase with boundary coupling differences.
Correlation functions decay monotonically as boundary couplings differ.
Variance of OPE data decreases with increasing marginal coupling difference.
Abstract
We describe a one-parameter family of Euclidean wormhole solutions with the topology of a compact hyperbolic space times an interval in Einstein gravity minimally coupled to a massless scalar field in AdS commonly referred to as Einstein-dilaton gravity. These solutions are locally described by the same metric and dilaton profile as the single-boundary Janus domain wall solutions in the same theory which are usually studied in the context of holographic RG flows. The wormholes compute the averaged product of partition functions of CFTs on either boundary deformed by different marginal couplings to the scalar operator dual to the dilaton. We observe that the renormalised volumes of these wormholes increase monotonically with the difference in the marginal couplings on the boundary thereby showing that the pair of CFTs on the boundaries get increasingly decorrelated as the…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Solar and Space Plasma Dynamics · Astro and Planetary Science
