On quantum creation of a toroidal universe
Abstract
We consider the quantum creation of a universe with flat spatial sections and the topology of a 3-torus, taking into account the effect of Casimir energy. We show that the corresponding instantons are singular. Since these instantons describe universes originating in a state of infinite energy, we argue that they cannot be interpreted as quantum creation from `nothing'. If quantum corrections to the energy-momentum tensor are neglected, the spacetime of the toroidal universe reduces to de Sitter space with appropriate periodic identifications. Contrary to previous claims in the literature, this spacetime is geodesically incomplete. We argue that this spacetime describes a classical universe originating at a singularity, and not a quantum origin. We conclude that the quantum creation of a toroidal universe from nothing cannot be described in the context of semiclassical quantum gravity -- it is either impossible, or it depends essentially on Planck-scale physics. We therefore see no reasonable way to compare the probability of creation of a toroidal universe, if it is possible at all, with that of a spherical universe.
Keywords
Cite
@article{arxiv.2508.08747,
title = {On quantum creation of a toroidal universe},
author = {Alan H. Guth and Alexander Vilenkin},
journal= {arXiv preprint arXiv:2508.08747},
year = {2025}
}
Comments
23 pages, no figures. To be published in "Open Issues in Gravitation and Cosmology - Original Contributions, Essays and Recollections in Honor of Alexei Starobinsky," edited by Andrei Barvinsky and Alexander Kamenshchik (Springer Nature, 2025). V2 includes additional references, and a minor wording change in Footnote 6