Astrophysics

    

Magnetic Fields of White Dwarfs and Neutron Stars

Authors: Kiyoung Kim

Neutron stars and white dwarfs are known to be the final stages in the life cycle of stars. These celestial objects are characterized by immense gravitational pressure, extremely high temperatures, and exceptionally high density. Additionally, some of them are known to possess extraordinarily strong magnetic fields under these extreme conditions. However, the precise mechanisms behind the generation of such strong magnetic fields remain unclear. The primitive virtual negative (PVN) charge dynamo mechanism proposed for solar planets in 2008, which involves the interaction between gravitational mass and electric charges, is applied to compact objects like white dwarfs and neutron stars because it is considered comprehensive and consistent.

Comments: 16 Pages.

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[v1] 2025-03-14 21:02:53

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