2010/06/15 by Hoang Sy Than, E. Khan, Nguyen Van Giai · 18 citations
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics #Atomic physics #Condensed matter physics #Crust #Geophysics #Hartree–Fock method #High-pressure geophysics and materials #Materials science #Neutron #Neutron star #Nuclear physics #Nuclear physics research studies #Pairing #Physics #Pulsars and Gravitational Waves Research #Range (aeronautics) #Stars #Superconductivity #nucl-th
paper · pdf · doi:10.1088/0954-3899/38/2/025201
published in Journal of Physics G Nuclear and Particle Physics 38(2), 025201 (IOP Publishing) · 11 pages, 5 figures
arxiv created 2010/06/15 · openalex publication_date 2011/01/05 · arxiv updated 2011/01/17 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
The structure of Wigner–Seitz cells in the inner crust of neutron stars is investigated using a microcospic Hartree–Fock-BCS approach with finite-range D1S and M3Y–P4 interactions. Large effects on the densities are found compared to previous predictions using Skyrme interactions. Pairing effects are investigated using finite-range interactions in the mean field.