Interacting Kerr-Newman Electromagnetic Fields
Sajad Aghapour, Lars Andersson, Kjell Rosquist, Tomasz Smołka
TL;DR
The paper analyzes the G→0 limit of the Kerr-Newman solution, known as the electromagnetic magic field, and develops a field-only description in flat space with a nontrivial two-sheeted topology and a ring singularity. It formulates a Lagrangian framework using the complex potential and computes the self-energy and interaction energy for one and two magic fields, respectively, revealing a finite single-field Lagrangian and spin-induced corrections to the Coulomb potential. By examining two canonical configurations (up-down and side-by-side) of interacting magic fields, it derives closed-form interaction energies and their asymptotic expansions, uncovering potential wells and equilibrium points tied to the spin parameters. The results strengthen the electron–Kerr–Newman analogy through multipole coincidences and spin-topology insights, and they point to broader implications for classical spin interactions and the double-copy relation between gravity and electromagnetism.
Abstract
In this paper, we study some of the properties of the $G \to 0$ limit of the Kerr-Newman solution of Einstein-Maxwell equations. Noting Carter's observation of the near equality between the $g = 2$ gyromagnetic ratio in the Kerr-Newman solution and that of the electron, we discuss additional such coincidences relating to the Kerr-Newman multipoles and properties of the electron. In contrast to the Coulomb field, this spinning Maxwell field has a finite Lagrangian. Moreover, by evaluating the Lagrangian for the superposition of two such Kerr-Newman electromagnetic fields on a flat background, we are able to find their interaction potential. This yields a correction to the Coulomb interaction due to the spin of the field.
