TITLE:
Magnetism in the World-Universe Cosmology
AUTHORS:
Vladimir S. Netchitailo
KEYWORDS:
World-Universe Cosmology, Cosmic Medium, Universe-Created Particles, DIRAC Dipoles, Dark Magnetic Field, Magnetic Field Intermittency
JOURNAL NAME:
Journal of High Energy Physics, Gravitation and Cosmology,
Vol.11 No.4,
October
22,
2025
ABSTRACT: In electromagnetics, the term magnetic field refers to two distinct but closely related vector fields: magnetic flux density B and magnetic field intensity H. These fields differ in how they account for the medium and magnetization M. In a vacuum, they are related by
B=
μ
0
H
. In a magnetized material, this relation becomes
B=
μ
0
(
H+M
)
. Within the framework of the World-Universe Cosmology (WUC), the Cosmic Medium (CM)—comprising protons, electrons, photons, neutrinos, and Universe-Created Particles (UCPs)—acts as a universal agent governing all physical processes and is inherently a magnetized medium. UCPs, conceptualized as DIRAC dipoles formed by Dirac’s magnetic monopoles, possess a magnetic dipole moment proportional to the Bohr magneton. Any local concentration of DIRACs within any material, including CM, induces both a magnetization field M and a magnetic field intensity H. This approach to magnetic fields within WUC offers a framework for explaining a wide range of observed magnetic phenomena, including the dark magnetic field, the large-scale structure of the Milky Way’s magnetic field, and other magnetic effects that are only partially correlated with objects observable in other spectral ranges.