A Spacetime in Toroidal Coordinates
J.P. Krisch, E.N. Glass (Department of Physics, University of, Michigan, Ann Arbor, Michgan)

TL;DR
This paper derives an exact Einstein's field equations solution in toroidal coordinates, describing a spacetime with distinct interior, boundary, and exterior regions, including implications for cosmological constants and anti-de Sitter spacetime.
Contribution
It introduces a novel exact solution in Einstein's equations with a toroidal geometry, incorporating a string equation of state and boundary layers.
Findings
The exterior spacetime is locally isometric to anti-de Sitter space.
The size and mass of the toroidal structure depend on the cosmological constant.
The solution includes an interior string-like region and a boundary layer.
Abstract
We present an exact solution of Einstein's field equations in toroidal coordinates. The solution has three regions: an interior with a string equation of state; an Israel boundary layer; an exterior with constant isotropic pressure and constant density, locally isometric to anti-de Sitter spacetime. The exterior can be a cosmological vacuum with negative cosmological constant. The size and mass of the toroidal loop depend on the size of the cosmological constant.
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