Magnetized Bose–Einstein condensate stars with boundary conditions depending on magnetic field

Abstract

In this article, we analyze the impact of the magnetic field-dependent boundary conditions on the solutions of the -structure equations for magnetized Bose-Einstein condensate stars (BECs). We consider two cases: pure BECs and BECs surrounded by a magnetic field. As they correspond to different physical situations, they lead to different numerical behaviors, having important effects on the stability of the solutions, as well as on the observables of the star. The differences between the mass-radii curves obtained in each situation are presented and discussed. K E Y W O R D Sanisotropic equation of state, Bose-Einstein condensate, magnetic field, structure equations