Evolution of the magnetic field in neutron stars
High Energy Astrophysical Phenomena
2018-08-08 v2
Abstract
We propose a general method to self-consistently study the quasistationary evolution of the magnetic field in the cores of neutron stars. The traditional approach to this problem is critically revised. Our results are illustrated by calculation of the typical timescales for the magnetic field dissipation as functions of temperature and the magnetic field strength.
Keywords
Cite
@article{arxiv.1705.00508,
title = {Evolution of the magnetic field in neutron stars},
author = {M. E. Gusakov and E. M. Kantor and D. D. Ofengeim},
journal= {arXiv preprint arXiv:1705.00508},
year = {2018}
}
Comments
22 pages, 2 figures, 1 table, Sec. IVD and Appendix B are added; published in PRD