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

2); (2) CRAL (UMR CNRS No. 5574); 3) ((1) Ioffe Physical-Technical Institute; (3) Saint-Petersburg State Polytechnical University); A. Y. Potekhin (1; D. G. Yakovlev (1; ENS-Lyon; France; Russia; Saint Petersburg

arxiv: 1109.3783 · v1 · pith:XZY2UUAAnew · submitted 2011-09-17 · 🌌 astro-ph.SR

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

A. Y. Potekhin (1 , 2) , D. G. Yakovlev (1 , 3) ((1) Ioffe Physical-Technical Institute , Saint Petersburg , Russia , (2) CRAL (UMR CNRS No. 5574) , ENS-Lyon

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France (3) Saint-Petersburg State Polytechnical University)

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keywords densefermionmagnetizedcannotclaimedcommentcontraryequation

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

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