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Spacetime constructed from a contact manifold with a degenerate metric

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abstract

We construct a four-dimensional spacetime using a three-dimensional contact manifold equipped with a degenerate metric. The degenerate metric is set to be compatible with the contact structure. The compatibility condition is defined in this paper. Our construction yields a Ricci tensor of a particularly simple form, which leads to a solution of the Einstein equation with a null dust and cosmic strings. The solution includes two arbitrary functions: the energy density of the null dust and the number density of the cosmic strings. When there exist the cosmic strings, the spacetime is of Petrov type D. Otherwise, the spacetime is conformally flat. For some simple matter densities, we examine the Einstein equation in detail.

fields

gr-qc 1

years

2026 1

verdicts

UNVERDICTED 1

representative citing papers

Geometric deformations of symmetric spacetimes with a string cloud

gr-qc · 2026-04-19 · unverdicted · novelty 5.0

A single-function deformation of 3D eta-Einstein metrics produces 4D Einstein spacetimes sourced by a string cloud, covering FLRW, Kantowski-Sachs, LRS Bianchi, Taub-NUT-(A)dS, and Reissner-Nordstrom-(A)dS solutions with spherical, planar or hyperbolic symmetry.

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  • Geometric deformations of symmetric spacetimes with a string cloud gr-qc · 2026-04-19 · unverdicted · none · ref 34 · internal anchor

    A single-function deformation of 3D eta-Einstein metrics produces 4D Einstein spacetimes sourced by a string cloud, covering FLRW, Kantowski-Sachs, LRS Bianchi, Taub-NUT-(A)dS, and Reissner-Nordstrom-(A)dS solutions with spherical, planar or hyperbolic symmetry.