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The equation of state (EoS) of the outer crust of a cold non-accretingmagnetar has been determined using the model of Lai and Shapiro (1991). Forthis purpose, we have made use of the latest experimental atomic mass datacomplemented with a Hartree-Fock-Bogoliubov (HFB) mass model. Magnetar crustsare found to be significantly different from the crusts of ordinary neutronstars.

Equation of state of magnetar crusts from Hartree-Fock-Bogoliubov atomic mass models