par Chamel, Nicolas 
;Pearson, Michael J.;Goriely, Stéphane
Editeur scientifique Lewandowski, Wojciech;Maron, Olaf;Kijak, Jaroslaw
Référence Electromagnetic Radiation from Pulsars and Magnetars(24-27 April 2012: Zielona Gora, Poland), Electromagnetic Radiation from Pulsars and Magnetars, Astronomical Society of the Pacific Conference Series, San Francisco, Vol. 466, page (203)
Publication Publié, 2013-01-09
;Pearson, Michael J.;Goriely, Stéphane Editeur scientifique Lewandowski, Wojciech;Maron, Olaf;Kijak, Jaroslaw
Référence Electromagnetic Radiation from Pulsars and Magnetars(24-27 April 2012: Zielona Gora, Poland), Electromagnetic Radiation from Pulsars and Magnetars, Astronomical Society of the Pacific Conference Series, San Francisco, Vol. 466, page (203)
Publication Publié, 2013-01-09
Publication dans des actes
| Résumé : | Despite the absence of viscous drag, the neutron superfluid permeating the inner crust of a neutron star can still be strongly coupled to nuclei due to non-dissipative entrainment effects. Neutron superfluidity and entrainment have been systematically studied in all regions of the inner crust of a cold non-accreting neutron star in the framework of the band theory of solids. It is shown that in the intermediate layers of the inner crust a large fraction of “free” neutrons are actually entrained by the crust. The results suggest that a revision of the interpretation of many observable astrophysical phenomena might be necessary. |
