Rotating traversable wormholes in Einstein-Maxwell theory
arXiv:2210.08913 · doi:10.1016/j.physletb.2023.137677
Abstract
It is well-known that traversable wormhole solutions to the Einstein equations require the existence of an exotic matter source violating the null energy condition. An apparent exception is the overcharged Kerr-Newman-NUT solution of the Einstein-Maxwell equations, which has all the properties of a geodesically complete, traversable wormhole spacetime. We show that the exotic matter sourcing this consists in two counter-rotating tensionless straight cosmic strings -- the Misner-Dirac strings -- which, as expected, violate the null energy condition. The wormhole possesses an ergoregion, but no superradiance. The geodesic motion in this spacetime is briefly discussed, and the absence of closed circular null geodesics is demonstrated.
16 pages, no figures, published version
References in corpus (2)
Cited by in corpus (16)
- Ehlers transformations as a tool for constructing accelerating NUT black holes
- Exact rotating wormholes via Ehlers transformations
- Traversable Morris-Thorne-Buchdahl wormholes in quadratic gravity
- Influence of GUP corrected Casimir energy on zero tidal force wormholes in modified teleparallel gravity with matter coupling
- Morris-Thorne-type wormhole with global monopole charge and the energy conditions
- Killing horizons and surface gravities for a well-behaved three-function generalisation of the Kerr spacetime
- Rotational influence on fermions within negative curvature wormholes
- Wormhole metric
- Rotating traversable wormhole geometries in the presence of three-form fields
- Catenoid Inspired Hyperbolic Wormhole Geometry
- Outgoing electromagnetic flux from rotating wormholes
- Charged traversable wormholes: charge without charge
- On the role of closed timelike curves and confinement structure around Kerr-Newman singularity
- An exact Kerr-like rotating Morris--Thorne wormhole: throat, ergoregion and equatorial shadow slice
- Exact Spinning Morris-Thorne Wormhole: Causal Structure, Shadows, and Multipole Moments
- Exact solutions for slowly rotating wormholes in the presence of an anisotropic fluid