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

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

2011-09-17

arxiv.org/abs/1109.3783v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

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

Scientific paper

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.

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