| Автор | G Lazzari |
| Автор | F V de Blasio |
| Дата выпуска | 1997-08-01 |
| dc.description | The specific heat of the superfluid neutrons in the inner crust of a neutron star, where neutron-rich nuclei in a Coulomb lattice are permeated by a gas of unbound neutrons, is studied in the framework of a semiclassical model, based on the local density approximation, in order to describe the nonuniform pairing gap in the Wigner-Seitz cell. We have found that the specific heat of this superfluid system in a relevant range of densities and temperatures for the crust, has a value considerably larger than that associated with a uniform neutron superfluid. This result may have relevance in the study of the thermal evolution of neutron stars. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | Thermodynamic properties of superfluid neutron star matter |
| Тип | paper |
| DOI | 10.1088/0031-8949/56/2/008 |
| Electronic ISSN | 1402-4896 |
| Print ISSN | 0031-8949 |
| Журнал | Physica Scripta |
| Том | 56 |
| Первая страница | 221 |
| Последняя страница | 224 |
| Аффилиация | G Lazzari; The Niels Bohr Institute, University of Coenhagen, Blegdamsvej 17, DK-2100 Copenhagen, Denmark |
| Аффилиация | F V de Blasio; The Niels Bohr Institute, University of Coenhagen, Blegdamsvej 17, DK-2100 Copenhagen, Denmark |
| Выпуск | 2 |
