Finite temperature effects on magnetized Bose-Einstein condensate stars

Understand

We study the role of temperature and magnetic field on the equation of state and macroscopic properties of Bose-Einstein condensate stars.

• These compact objects are composed of a condensed gas of interacting neutral vector bosons coupled to a uniform and constant magnetic field.
• We found that the main consequence of a finite temperature in the magnetized equations of state is to increase the inner pressure of the star.
• As a consequence, magnetized hot Bose-Einstein condensate stars are larger and heavier than their zero-temperature counterparts.