The surface and inner temperatures of magnetars
High Energy Astrophysical Phenomena
2013-12-09 v1
Abstract
Assuming that the timescale of the magnetic field decay is approximately equal to that of the stellar cooling via neutrino emission, we obtain a one-to-one relationship between the effective surface thermal temperature and the inner temperature. The ratio of the effective neutrino luminosity to the effective X-ray luminosity decreases with decaying magnetic field.
Keywords
Cite
@article{arxiv.1312.1774,
title = {The surface and inner temperatures of magnetars},
author = {Z. F. Gao and N. Wang and Q. H. Peng},
journal= {arXiv preprint arXiv:1312.1774},
year = {2013}
}
Comments
3 Pages, 3 Figures, Published in IAU Symposium, 2013, V.291 p.386-388. 2013IAU Symposium