A Semi-classical Upper Limit For Magnetic Fields Strength And the Case of Magnetars
Solar and Stellar Astrophysics
2021-07-27 v2 High Energy Astrophysical Phenomena
Abstract
In the pass from classical to modern physics, the idea of supposing some quantities having distinct or bounded values and keeping the rest continuous has been useful in treating many problems. In this paper, we suppose an upper limit for velocity of the classical particles and show applying this assumption to electromagnetism leads us to a maximum strength for magnetic fields which reveals an acceptable coincidence with the highest strengths in the cosmos, observed in magnetars.
Keywords
Cite
@article{arxiv.1511.06679,
title = {A Semi-classical Upper Limit For Magnetic Fields Strength And the Case of Magnetars},
author = {Amir A. E. Shafig},
journal= {arXiv preprint arXiv:1511.06679},
year = {2021}
}
Comments
The paper has been reviewed by quite a few referees and has many problems that need to be fixed. Therefore, I plan to submit a completely new, revised version and make the older problematic version inaccessible