dorsal/arxiv
View SchemaMean field and pairing properties in the crust of neutron stars
| Authors | F. Montani, C. May, H. Müther |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0401024 |
| URL | https://arxiv.org/abs/nucl-th/0401024 |
| DOI | 10.1103/PhysRevC.69.065801 |
| Journal | Phys.Rev. C69 (2004) 065801 |
Abstract
Properties of the matter in the inner crust of a neutron star are investigated in a Hartree-Fock plus BCS approximation employing schematic effective forces of the type of the Skyrme forces. Special attention is paid to differences between a homogenous and inhomogeneous description of the matter distribution. For that purpose self-consistent Hartree Fock calculations are performed in a spherical Wigner-Seitz cell. The results are compared to predictions of corresponding Thomas Fermi calculations. The influence of the shell structure on the formation of pairing correlations in inhomogeneous matter are discussed.
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"abstract": "Properties of the matter in the inner crust of a neutron star are\ninvestigated in a Hartree-Fock plus BCS approximation employing schematic\neffective forces of the type of the Skyrme forces. Special attention is paid to\ndifferences between a homogenous and inhomogeneous description of the matter\ndistribution. For that purpose self-consistent Hartree Fock calculations are\nperformed in a spherical Wigner-Seitz cell. The results are compared to\npredictions of corresponding Thomas Fermi calculations. The influence of the\nshell structure on the formation of pairing correlations in inhomogeneous\nmatter are discussed.",
"arxiv_id": "nucl-th/0401024",
"authors": [
"F. Montani",
"C. May",
"H. M\u00fcther"
],
"categories": [
"nucl-th"
],
"doi": "10.1103/PhysRevC.69.065801",
"journal_ref": "Phys.Rev. C69 (2004) 065801",
"title": "Mean field and pairing properties in the crust of neutron stars",
"url": "https://arxiv.org/abs/nucl-th/0401024"
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