Slowly rotating Curzon-Chazy Metric

TL;DR

This paper introduces a slow rotation extension of the Curzon-Chazy metric, derived via perturbation methods, verified with computational tools, and discussed for potential applications in gravitational physics.

Contribution

A novel slow rotation version of the Curzon-Chazy metric is developed and validated using computational methods, expanding the metric's applicability.

Findings

The new metric satisfies Einstein's field equations.

The perturbation method effectively incorporates slow rotation.

Potential applications in gravitational studies are discussed.

Abstract

A new rotation version of the Curzon-Chazy metric is found. This new metric was obtained by means of a perturbation method, in order to include slow rotation. The solution is then proved to fulfill the Einstein field equations using a REDUCE program. Furthermore, the applications of this new solution are discussed.