The Relativistically Spinning Charged Sphere
Donald Lynden-Bell

TL;DR
This paper explores the electromagnetic field structure of a relativistically spinning charged sphere, revealing charge confinement effects, field configurations, and classical electron model implications as the spin velocity approaches the speed of light.
Contribution
It introduces a detailed analysis of charge distribution and electromagnetic fields in a relativistically spinning charged sphere, connecting to Kerr-Newman black hole fields and classical electron models.
Findings
Charge concentrates at the equator as v approaches c.
Total charge in the belt diverges as (1-v^2/c^2)^(-1/4).
Electromagnetic properties resemble classical electron models with relativistic spin.
Abstract
When the equatorial spin velocity, , of a charged conducting sphere approaches , the Lorentz force causes a remarkable rearrangement of the total charge . Charge of that sign is confined to a narrow equatorial belt at latitudes while charge of the opposite sign occupies most of the sphere's surface. The change in field structure is shown to be a growing contribution of the `magic' electromagnetic field of the charged Kerr-Newman black hole with Newton's G set to zero. The total charge within the narrow equatorial belt grows as and tends to infinity as approaches . The electromagnetic field, Poynting vector, field angular momentum and field energy are calculated for these configurations. Gyromagnetic ratio, g-factor and electromagnetic mass are illustrated in terms of a 19th Century electron model.…
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