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.

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Keywords: semiclassical gravity, electron as a black hole, Wilson loops, radiating Kerr solution, QED, supersymmetry, Kerr—Newman electrons, classical relativistic strings, bare electrons, dressed electrons PACS: 04.60.−m, 04.70.−s, 11.25.−w (all) DOI: 10.3367/UFNe.2024.05.039684 URL: https://ufn.ru/en/articles/2024/10/e/ Citation: Burinskii A Ya "Kerr—Newman solution unites gravitation with quantum theory" Phys. Usp. 67 (10) (2024) Received: 5th, December 2023, revised: 23rd, April 2024, accepted: 22nd, May 2024 Оригинал: Буринский А Я «Решение Керра—Ньюмана объединяет гравитацию с квантовой теорией» УФН 194 1095–1107 (2024); DOI: 10.3367/UFNr.2024.05.039684