par Magierski, Piotr;Bulgac, Aurel;Heenen, Paul-Henri 
Référence International Journal of Modern Physics A, 17, 1, page (1059-1064)
Publication Publié, 2002
Référence International Journal of Modern Physics A, 17, 1, page (1059-1064)
Publication Publié, 2002
Article révisé par les pairs
| Résumé : | The inner crust of neutron stars consists of nuclei of various shapes immersed in a neutron gas and stabilized by the Coulomb interaction in the form of a crystal lattice. The scattering of neutrons on nuclear inhomegeneities leads to the quantum correction to the total energy of the system. This correction resemble the Casimir energy and turn out to have a large influence on the structure of the crust. |
