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

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arxiv 1109.3783 v1 pith:XZY2UUAA submitted 2011-09-17 astro-ph.SR

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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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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  1. Dense Quark-Gluon Plasma in strong magnetic fields

    hep-ph 2019-08 conditional novelty 6.0 of 10

    Analytic expressions for quark pressure and magnetic susceptibility of dense quark-gluon plasma in strong magnetic fields are derived within the Field Correlator Method, predicting strong paramagnetism.

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