English

Neutron star composition in strong magnetic fields

Astrophysics 2009-11-07 v2

Abstract

We study the problem of neutron star composition in the presence of a strong magnetic field. The effects of the anomalous magnetic moments of both nucleons and electrons are investigated in relativistic mean field calculations for a β\beta-equilibrium system. Since neutrons are fully spin polarized in a large field, generally speaking, the proton fraction can never exceed the field free case. An extremely strong magnetic field may lead to a pure neutron matter instead of a proton-rich matter.

Keywords

Cite

@article{arxiv.astro-ph/0111374,
  title  = {Neutron star composition in strong magnetic fields},
  author = {G. Mao and V. N. Kondratyev and A. Iwamoto and Z. Li and X. Wu and W. Greiner and I. N. Mikhailov},
  journal= {arXiv preprint arXiv:astro-ph/0111374},
  year   = {2009}
}

Comments

12 pages, 3 postscript files included

R2 v1 2026-07-22T08:05:03.666Z