Curved traversable wormholes in (3+1)-dimensional spacetime
Vee-Liem Saw, Lock Yue Chew

TL;DR
This paper introduces a general method for constructing curved traversable wormholes in (3+1)-dimensional spacetime, analyzing their physics, and providing explicit examples like the static zero tidal force catenary wormhole, highlighting differences from lower-dimensional models.
Contribution
It presents a novel geometric construction approach for (3+1)-d wormholes, including explicit solutions and comparisons with lower-dimensional cases, advancing understanding of their physical properties.
Findings
Existence of geodesics supported by non-exotic matter
Positive mass-energy supports the wormhole with some null energy condition violations
Method can be used to construct time-evolving inflationary wormholes
Abstract
We present the general method of constructing curved traversable wormholes in (3+1)-d spacetime and proceed to thoroughly discuss the physics of a zero tidal force metric without cross-terms. The (3+1)-d solution is compared with the recently studied lower-dimensional counterpart, where we identify that the much richer physics - involving pressures and shear forces of the mass-energy fluid supporting the former - is attributed to the mixing of all three spatial coordinates. Our (3+1)-d universe is the lowest dimension where such nontrivial terms appear. An explicit example, the static zero tidal force (3+1)-d catenary wormhole is analysed and we show the existence of a geodesic through it supported locally by non-exotic matter, similar to the (2+1)-d version. A key difference is that positive mass-energy is used to support the entire (3+1)-d catenary wormhole, though violation of the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
