Nuclei in Strongly Magnetised Neutron Star Crusts
Rana Nandi, Debades Bandyopadhyay

TL;DR
This paper investigates how strong magnetic fields influence the composition and properties of neutron star crusts, revealing larger nuclei and altered proton fractions, with implications for magnetar oscillations.
Contribution
It provides a detailed analysis of nuclear compositions in neutron star crusts under strong magnetic fields using updated models and interactions, highlighting significant differences from zero-field cases.
Findings
Nuclei in the inner crust have larger mass and charge numbers under strong magnetic fields.
SLy4 interaction significantly affects proton fractions and nuclear properties.
Magnetic field effects may influence magnetar shear mode oscillations.
Abstract
We discuss the ground state properties of matter in outer and inner crusts of neutron stars under the influence of strong magnetic fields. In particular, we demonstrate the effects of Landau quantization of electrons on compositions of neutron star crusts. First we revisit the sequence of nuclei and the equation of state of the outer crust adopting the Baym, Pethick and Sutherland (BPS) model in the presence of strong magnetic fields and most recent versions of the theoretical and experimental nuclear mass tables. Next we deal with nuclei in the inner crust. Nuclei which are arranged in a lattice, are immersed in a nucleonic gas as well as a uniform background of electrons in the inner crust. The Wigner-Seitz approximation is adopted in this calculation and each lattice volume is replaced by a spherical cell. The coexistence of two phases of nuclear matter - liquid and gas, is…
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