Comment on Equation of state of dense and magnetized fermion system
published by Alexander Potekhin
in 2011
in Physics
and research's language is
English
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Abstract in English
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.