Unified Relativistic Mean Field EoSs with density dependent couplings

This dataset, containing 447345 equations of state, was used or the Bayesian analysis on the properties of Neutron Stars in [1]. Each EoS includes an outer crust, an inner crust and a core.The outer crust used for all the EoSs is the BsK22[2], while each pair of inner crust and core was calculatedusing the same Relativistic Mean Field model and a Compressible Liquid Drop approximation for the clusters in the inner crust. The crust-core transition is determined for each model by the crossingof the energy density of crust and core. [1] L. Scurto, H. Pais and F. Gulminelli, arXiv:2402.15548 (2024)[2] J.M. Pearson, N. Chamel, A.Y. Potekhin, A.F. Fantina, C. Ducoin, A.K. Dutta, and S. Goriely, MNRAS 481, 2994 (2018)