Magnetized BEC stars with boundary conditions depending on magnetic field

TL;DR

This paper investigates how boundary conditions influenced by magnetic fields affect the structure and stability of magnetized Bose-Einstein condensate stars, highlighting differences in their physical properties and observable characteristics.

Contribution

It introduces a detailed analysis of boundary condition effects on magnetized BEC star solutions, considering distinct physical scenarios and their impact on star stability and observables.

Findings

Boundary conditions significantly affect star stability.

Mass-radius relationships vary with magnetic boundary conditions.

Magnetic field embedding alters observable star properties.

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.