Rotating wormholes in Einstein-Dirac-Maxwell theory
General Relativity and Quantum Cosmology
2026-04-21 v2
Abstract
We consider rotating wormhole solutions in general relativity supported by a complex non-phantom spinor field (which provides a nontrivial spacetime topology) and electromagnetic fields. The solutions are asymmetric, regular, asymptotically flat and carry nonzero total angular momentum. The physical properties of the resulting configurations are completely determined by the values of three input quantities: the throat parameter, the spinor frequency, and the electromagnetic coupling constant. The wormholes connect two identical Minkowski spacetimes possessing in general different masses and global charges.
Keywords
Cite
@article{arxiv.2511.02431,
title = {Rotating wormholes in Einstein-Dirac-Maxwell theory},
author = {Vladimir Dzhunushaliev and Vladimir Folomeev},
journal= {arXiv preprint arXiv:2511.02431},
year = {2026}
}
Comments
15 pages, 8 figures, corrections to content, version published in GRG