UDK 53 Физика
UDK 520 Инструменты, приборы и методы астрономических наблюдений, измерений и анализа
UDK 521 Теоретическая астрономия. Небесная механика. Фундаментальная астрономия. Теория динамической и позиционной астрономии
UDK 523 Солнечная система
UDK 524 Звезды и звездные системы. Вселенная Солнце и Солнечная система
UDK 52-1 Метод изучения
UDK 52-6 Излучение и связанные с ним процессы
GRNTI 41.00 АСТРОНОМИЯ
GRNTI 29.35 Радиофизика. Физические основы электроники
GRNTI 29.31 Оптика
GRNTI 29.33 Лазерная физика
GRNTI 29.27 Физика плазмы
GRNTI 29.05 Физика элементарных частиц. Теория полей. Физика высоких энергий
OKSO 03.06.01 Физика и астрономия
OKSO 03.05.01 Астрономия
OKSO 03.04.03 Радиофизика
BBK 2 ЕСТЕСТВЕННЫЕ НАУКИ
BBK 223 Физика
TBK 614 Астрономия
TBK 6135 Оптика
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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