The magnetic structure of neutron stars and their surface-to-core temperature relation
Astrophysics
2007-05-23 v2
Abstract
We study the relation between the mean effective surface temperature T_s and the internal temperature T_b for magnetic neutron stars, assuming that the magnetic field near the surface has a presumably small-scale structure. The heavy-element (iron) and light-element (accreted) heat-blanketing envelopes are considered, and the results are compared with the case of a dipole magnetic field. We argue that the difference in the T_b(T_s)-relation for different magnetic configurations is always much smaller than a possible difference caused by variations of the chemical composition in the envelope.
Keywords
Cite
@article{arxiv.astro-ph/0508415,
title = {The magnetic structure of neutron stars and their surface-to-core temperature relation},
author = {A. Y. Potekhin and V. Urpin and G. Chabrier},
journal= {arXiv preprint arXiv:astro-ph/0508415},
year = {2007}
}
Comments
5 pages, 2 figures. V2: a typo corrected. Accepted by A&A