par Pearson, Michael J.;Chamel, Nicolas ;Pastore, Alessandro ;Goriely, Stéphane
Référence Physical review. C. Nuclear physics, 91, page (018801)
Publication Publié, 2015-01-14
Article révisé par les pairs
Résumé : The TETFSI (temperature-dependent extended Thomas-Fermi plus Strutinsky integral) method for calculating the properties of the inner crust of neutron stars is here extended in the zero-temperature limit to include proton pairing. The main effect is to smooth out the proton shell effects, although the energetically favored value of Z, the number of protons per Wigner-Seitz cell, remains at, or close to, 40.

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