UDC 53
UDC 520
UDC 521
UDC 523
UDC 524
UDC 52-1
UDC 52-6
CSCSTI 41.00
CSCSTI 29.35
CSCSTI 29.31
CSCSTI 29.33
CSCSTI 29.27
CSCSTI 29.05
Russian Classification of Professions by Education 03.06.01
Russian Classification of Professions by Education 03.05.01
Russian Classification of Professions by Education 03.04.03
Russian Library and Bibliographic Classification 2
Russian Library and Bibliographic Classification 223
Russian Trade and Bibliographic Classification 614
Russian Trade and Bibliographic Classification 6135
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
The presence of even simple magnetized wormholes may have observable consequences. If the wormhole and its surrounding magnetic fields are static, symmetrical, and spherical, and gas in the vicinity falls radially into the wormhole, the resulting spectrum would feature bright cyclotron or synchrotron lines caused by interactions between charged plasma particles and the magnetic field. This radiation would be non-polarized due to the symmetry of the system. The emission of this exotic, non-thermal yet non-polarized type of radiation could serve as a signature for wormholes. Additionally, in this scenario, the formation of an accretion disk is still possible at some distance from the wormhole; however, a monopole magnetic field may complicate this process and lead to the emergence of asymmetrical and one-sided relativistic jets.
accretion, accretion disks, magnetic fields, gravitation
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