Magnetized BEC stars with boundary conditions depending on magnetic field

Abstract

In this paper we analyze the impact of the boundary conditions on the solutions of the $\gamma$-structure equations for magnetized Bose-Einstein condensate stars (BECs). We consider two cases: a pure BECs and a BECs embedded in a magnetic field. Since they correspond to different physical situations, they lead to different numerical behavior, 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.

arXiv comment6 pages, 5 figures, conference paper

References in corpus (8)

• Neutron Star Observations: Prognosis for Equation of State Constraints
• BCS-BEC Crossover and the Unitary Fermi Gas
• Bose-Einstein Condensate general relativistic stars
• ROTATING NEUTRON STAR MODELS WITH MAGNETIC FIELD
• Boson star at finite temperature
• Modeling anisotropic magnetized White Dwarfs with $\gamma$ metric
• A theory of finite-temperature Bose-Einstein condensates in neutron stars
• (Self-)Magnetized Bose-Einstein Condensate stars

Cited by in corpus (1)

• Bose-Einstein Condensate dark matter models in the presence of baryonic matter and random confining potentials