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Self-gravitating bosons at nonzero temperature

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arxiv gr-qc/0006065 v2 pith:67N4TVBS submitted 2000-06-19 gr-qc astro-phhep-ph

Neven Bilic , Hrvoje Nikolic (Rudjer Boskovic Institute , Zagreb , Croatia) This is my paper · ORCID
classification gr-qcastro-phhep-ph
keywords temperaturesystembosonbosonscondensateassumechargedchemical
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abstract

A system of charged bosons at finite temperature and chemical potential is studied in a general-relativistic framework. We assume that the boson fields interact only gravitationally. At sufficiently low temperature the system exists in two phases: the gas and the condensate. By studying the condensation process numerically we determine the critical temperature $T_c$ at which the condensate emerges. As the temperature decreases, the system eventually settles down in the ground state of a cold boson star.

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Cited by 1 Pith paper

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  1. Durgapal-Fuloria Bose-Einstein condensate stars within $ f(R,T) $ gravity theory

    gr-qc 2025-06 reject novelty 3.0 of 10

    A claimed stable BEC star solution in f(R,T) gravity based on the Durgapal-Fuloria metric, but the derivation is opaque and internally inconsistent.

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