Comment on "Equation of state of dense and magnetized fermion system"

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.

2 pages, to be published in Phys. Rev. C

References in corpus (1)

• Equation of State of a Dense and Magnetized Fermion System

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