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

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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.

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hep-ph 1

years

2019 1

verdicts

CONDITIONAL 1

representative citing papers

Dense Quark-Gluon Plasma in strong magnetic fields

hep-ph · 2019-08-02 · conditional · novelty 6.0

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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  • Dense Quark-Gluon Plasma in strong magnetic fields hep-ph · 2019-08-02 · conditional · none · ref 38 · internal anchor

    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.