Baby Universes in AdS$_3$
Alexandre Belin, Jan de Boer
TL;DR
The paper investigates Euclidean geometries in AdS$_3$ whose Lorentzian slices yield baby universes of genus $g\ge 2$ within a holographic CFT on a higher-genus boundary. It shows that in the standard CFT-path-integral construction these baby-universe geometries exist but are subdominant saddles, so they do not provide a semiclassical description of the state. By applying a microscopic prescription that contracts the density matrix with OPE data, the authors render a state whose leading bulk dual includes a baby universe, at the cost of the CFT state becoming mixed; crucially, the fluctuations remain small and the baby universe is semiclassical. The Virasoro TQFT interpretation clarifies how the baby universe is encoded in an auxiliary conformal-block Hilbert space and discusses canonical purification, observers, and purification structure. The work offers a coherent framework to analyze baby universes in AdS$_3$/CFT$_2$, outlining extensions to include matter and higher-genus geometries and addressing longstanding puzzles about semiclassical descriptions and purifications in quantum gravity.
Abstract
We discuss Euclidean geometries in AdS$_3$ whose Lorentzian slicing gives rise to closed baby universes with a spatial geometry given by genus $g\geq 2$ surfaces. Our setup only involves a two-dimensional holographic CFT defined on a higher genus Riemann surface and thus provides a well-posed alternative to shell states whose microscopic duals are less well understood. We find that geometries giving rise to baby universes are always subdominant. It follows that the baby universe does not provide a semi-classical description of the state since it is encoded in an exponentially suppressed part of the wave function. We then apply a prescription developed in \cite{Belin:2025wju} to make the baby universe geometry the leading saddle. In the process, the CFT state becomes mixed, in agreement with the qualitative gravitational picture. We show that the fluctuations in the baby universe are small, even at fixed central charge, making the geometry reliable in the semi-classical limit. Finally, we discuss the interpretation of this mixed state in pure gravity from the perspective of the Virasoro TQFT.
