The wavefunction of a quantum S 1 × S 2 universe

Abstract We study quantum gravity corrections to the no-boundary wavefunction describing a universe with spatial topology S 1 × S 2. It has been suggested that quantum effects become increasingly important when the size of the circle is large relative to the sphere. In this paper, we confirm this cl...

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Bibliographic Details
Main Authors: Gustavo J. Turiaci, Chih-Hung Wu
Format: Article
Language:English
Published: SpringerOpen 2025-07-01
Series:Journal of High Energy Physics
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Online Access:https://doi.org/10.1007/JHEP07(2025)158
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Summary:Abstract We study quantum gravity corrections to the no-boundary wavefunction describing a universe with spatial topology S 1 × S 2. It has been suggested that quantum effects become increasingly important when the size of the circle is large relative to the sphere. In this paper, we confirm this claim by an explicit four-dimensional one-loop calculation of the gravitational path integral preparing such a state. In the process, we clarify some aspects of the gravitational path integral on complex spacetimes. These quantum corrections play a crucial role in ensuring that the norm of the wavefunction is naturally expressed in terms of a path integral over S 2 × S 2 at the classical level. We extend some of the analysis to more general spatial topologies, as well as to the inclusion of fermions.
ISSN:1029-8479