Physics – Nuclear Physics – Nuclear Theory
Scientific paper
2001-12-05
Phys.Rev. C65 (2002) 045804
Physics
Nuclear Physics
Nuclear Theory
20 pages, 5 figures
Scientific paper
10.1103/PhysRevC.65.045804
We investigate the inner crust structure of neutron stars using the Skyrme-Hartree-Fock approach with the Coulomb interaction treated beyond the Wigner-Seitz approximation. Our results suggest that the shell effects associated with unbound neutrons play an important role and, in particular, lead to complicated phase transition pattern between various nuclear phases (as a function of the density). Namely, we show that the relative energies of different phases are rapidly oscillating functions of the neutron density. In the semiclassical approach this behavior is explained as an interference effect due to periodic orbits of similar lengths. We discuss also the dependence of the shell effects on pairing correlations.
Heenen Paul-Henri
Magierski Piotr
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