Magnetized Unified RMF Equation of State for Cold Neutron Star

Unified outer crust+ inner crust + core equation of state for magnetized npe beta-equilibrated matter, calculated within the RMF formalism using the NL3wr model [1,2]. We consider magnetic field between 10^16 G and 10^18 G. The outer crust was calculated using the tool [3]. The file NL3wr_magnetized_outer+inner+core_AMM.txt is calculated including the contribution of the anomalous magnetic moment of the nucleons, while the file NL3wr_magnetized_outer+inner+core.txt does not include that contribution. Each file is composed of 11 columns which contain, in order: 1) The magnetic field in G 2) The total number density (nucleons + electrons) in fm^-3 3) The total energy density in fm^-4 4) The component of the total pressure parallel to the magnetic field in fm^-4 5) The baryonic chemical potential in MeV 6) The mesonic field contribution to the pressure in fm^-4 7) The baryonic contribution to the parallel component of the pressure in fm^-4 8) The baryonic number density in fm^-3 9) The squared speed of sound 10) The component of the total pressure normal to the magnetic field in fm^-4 11) The total magnetization divided by the magnetic field [1] C. J. Horowitz and J. Piekarewicz, Phys. Rev. Lett. 86, 5647 (2001); Phys. Rev. C 64, 062802 (2001). [2] H. Pais and C. Providência, Phys. Rev. C 94, 015808 (2016). [3] N. Chamel, Equilibrium structure of the outer crust of a magnetar (Version 1.0.0). Zenodo. http://doi.org/10.5281/zenodo.3839787, (2020).