Semiclassical Wormholes toward Typical Entangled States
Year: 2025
Type: article
Abstract: What do the typical entangled states of two black holes look like? Do they contain semiclassical interiors? We approach these questions constructively, providing ensembles of states that densely explore the black hole Hilbert space. The states contain very long Einstein-Rosen caterpillars: semiclassical wormholes with large numbers of matter inhomogeneities. Distinguishing these ensembles from the typical entangled states of the black holes is hard. We quantify this by deriving the correspondence between a microscopic notion of quantum randomness and the geometric length of the wormhole. This formalizes a "complexity = geometry" relation.
Source: Physical Review Letters
DOI: 10.1103/btw6-44ry
Authors: Javier M. Magán, Martin Sasieta, Brian Swingle
Institutions: Balseiro Institute, Brandeis University
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Estimated APC paid: $3,750
OpenAlex ID: W4415226773
