arXiv · 1410.2748
Magnetic susceptibility and magnetization properties of asymmetric nuclear matter under a strong magnetic field
Abstract
We study the effect of a strong magnetic field on the proton and neutron spin polarization and magnetic susceptibility of asymmetric nuclear matter within a relativistic mean-field approach. It is shown that magnetic fields $B \sim 10^{16} - 10^{17}$ G have already noticeable effects on the range of densities of interest for the study of the crust of a neutron star. Although the proton susceptibility is larger for weaker fields, the neutron susceptibility becomes of the same order or even larger for small proton fractions and subsaturation densities for $B > 10^{16}$ G. We expect that neutron superfluidity in the crust will be affected by the presence of magnetic fields.
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A. Rabhi, M. A. Pérez-García, C. Providência, I. Vidaña. 2015-04-02. Magnetic susceptibility and magnetization properties of asymmetric nuclear matter under a strong magnetic field. https://doi.org/10.1103/physrevc.91.045803
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