par Chamel, Nicolas ;Pavlov, Rossen;Mihailov, L.M.;Velchev, Ch. J.;Stoyanov, Zh. K.;Mutafchieva, Y. D.;Ivanovich, M. D.;Fantina, Anthea ;Pearson, Michael J.;Goriely, Stéphane
Editeur scientifique Lewandowski, Wojciech;Maron, Olaf;Kijak, Jaroslaw
Référence Electromagnetic Radiation from Pulsars and Magnetars(April 24-27, 2012: Zielona Gora, Poland), Electromagnetic Radiation from Pulsars and Magnetars, Astronomical Society of the Pacific Conference Series, San Francisco, Vol. 466, page (249-250)
Publication Publié, 2013-01-09
Publication dans des actes
Résumé : The equation of state (EoS) of the outer crust of a cold non-accreting magnetar has been determined using the model of Lai & Shapiro (1991). For this purpose, we have made use of the latest experimental atomic mass data complemented with a Hartree-Fock-Bogoliubov (HFB) mass model. Magnetar crusts are found to be significantly different from the crusts of ordinary neutron stars.