Abstract:
The model of the Kerr–Newman (KN) electron generated by the superrotating gravitational field of a black hole is modified to a radiating black–white hole that both absorbs and emits electromagnetic waves. Following quantum electrodynamics (QED), we consider the KN solution to be either a bare electron model or a dressed electron model, where the bare electron forms a classical massless relativistic string responsible for the wave properties of the electron as a quantum particle, while the dressed electron forms a heavy electron–positron vacuum core dressed by the KN gravitational field due to the formation of electron and positron Wilson loops. Within the framework of the Kerr–Schild formalism, a class of radiating KN solutions is considered, whereby the electromagnetic field is absorbed by the black hole and at the same time radiated away by its white side.
Keywords:semiclassical gravity, electron as a black hole, Wilson loops, radiating Kerr solution, QED, supersymmetry, Kerr–Newman electrons, classical relativistic strings, bare electron, dressed electron.
PACS:04.60.-m, 04.70.-s, 11.25.-w
Received:December 5, 2023 Revised:April 23, 2024 Accepted: May 22, 2024
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