https://doi.org/10.1051/epjconf/202226011041
Self-consistent energy density functional approaches to the crust of neutron stars
1 Center for Computational Sciences and Faculty of Pure and Applied Sciences, University of Tsukuba Tsukuba 305-8577, Japan
2 RIKEN Nishina Center, Wako 351-0198, Japan
Published online: 24 February 2022
In order to study structure of the crust in neutron stars, we develop a finite-temperature Skyrme-Hartree-Fock method in the full three-dimensional coordinate space using the Fermion operator expansion method. It provides us with a possible order-N approach to non-uniform neutron-star matters.
© The Authors, published by EDP Sciences, 2022
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
