An axially symmetric stationary N-center solution of Einstein's vacuum equations
Aleksandr A. Shaideman, Jesus D. Arias H, and Kirill V. Golubnichiy

TL;DR
This paper presents a new stationary vacuum solution to Einstein's equations for N rotating axially symmetric masses, generalizing static and non-distorted solutions like Zipoy and Kerr-NUT configurations.
Contribution
It introduces a novel solution method for Einstein's vacuum equations that describes multiple rotating and static axially symmetric masses simultaneously.
Findings
Derivation of a stationary N-center solution using the Euclidon method.
The solution encompasses static, rotating, and non-distorted cases.
Provides a unified framework for multiple axially symmetric mass configurations.
Abstract
Using the Euclidon method, a stationary solution of Einstein's vacuum equations was obtained, describing N rotating axially symmetric masses, which in the absence of rotation describes N arbitrary axially symmetric static masses, for example, N Zipoy masses on the axis of symmetry, and in the absence of distortion, N Kerr-NUT solutions.
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Taxonomy
TopicsRelativity and Gravitational Theory · Quantum and Classical Electrodynamics · Spacecraft Dynamics and Control
