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Magnetic fields of order $10^{15}$ G have been measured at the surface ofsome neutron stars, and much stronger magnetic fields are expected to bepresent in the solid region beneath the surface. The effects of the magneticfield on the equation of state and on the composition of the crust due toLandau-Rabi quantization of electron motion are studied. Both the outer andinner crustal regions are described in a unified and consistent way within thenuclear-energy density functional theory.

Role of Landau-Rabi quantization of electron motion on the crust of magnetars within the nuclear energy density functional theory