Comment on "Equation of state of dense and magnetized fermion system"
Solar and Stellar Astrophysics
2015-05-30 v1
Abstract
Contrary to what is claimed by Ferrer et al. [Phys. Rev. C 82, 065802 (2010)], the magnetic field of a neutron star cannot exceed 10^{19} G and the thermodynamic pressure of dense magnetized fermion gas is isotropic.
Cite
@article{arxiv.1109.3783,
title = {Comment on "Equation of state of dense and magnetized fermion system"},
author = {A. Y. Potekhin and D. G. Yakovlev},
journal= {arXiv preprint arXiv:1109.3783},
year = {2015}
}
Comments
2 pages, to be published in Phys. Rev. C