par Chamel, Nicolas 
Référence IAU Symposium 291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years(20-31 August, 2012: Beijing, China), Proceedings of the International Astronomical Union, Cambridge University Press, Vol. 8, page (73-76)
Publication Publié, 2013-03-20
Référence IAU Symposium 291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years(20-31 August, 2012: Beijing, China), Proceedings of the International Astronomical Union, Cambridge University Press, Vol. 8, page (73-76)
Publication Publié, 2013-03-20
Publication dans des actes
| Résumé : | The neutron superfluid permeating the inner crust of mature neutron stars is expected to play a key role in various astrophysical phenomena like pulsar glitches. Despite the absence of viscous drag, the neutron superfluid can still be coupled to the solid crust due to non-dissipative entrainment effects. Entrainment challenges the interpretation of pulsar glitches and suggests that a revision of the interpretation of other observed neutron-star phenomena might be necessary. |
