Generating Solutions to the Einstein - Maxwell Equations
I. G. Contopoulos, F. P. Esposito, K. Kleidis, D. B. Papadopoulos, and, L. Witten

TL;DR
This paper derives solutions to the Einstein-Maxwell equations in curved spacetime with symmetries, using a potential transformation approach to generate new exact solutions from known seed solutions.
Contribution
It introduces a method to generate new Einstein-Maxwell solutions via continuous transformations of potentials based on a Lagrangian framework.
Findings
Recovered new exact solutions from the γ_A-metric
Demonstrated the transformation of seed solutions into novel solutions
Provided a systematic approach for solution generation in Einstein-Maxwell theory
Abstract
The Einstein-Maxwell (E-M) equations in a curved spacetime that admits at least one Killing vector are derived, from a Lagrangian density adapted to symmetries. In this context, an auxiliary space of potentials is introduced, in which, the set of potentials associated to an original (seed) solution of the E-M equations are transformed to a new set, either by continuous transformations or by discrete transformations. In this article, continuous transformations are considered. Accordingly, originating from the so-called -metric, other exact solutions to the E-M equations are recovered and discussed.
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