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Boson star at finite temperature

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arxiv 1412.1556 v1 pith:WMLRKJQY submitted 2014-12-04 astro-ph.SR hep-phnucl-th

S. Latifah , A. Sulaksono , T. Mart This is my paper · ORCID
classification astro-ph.SRhep-phnucl-th
keywords bosonstartemperaturebose-einsteinchavaniscondensateharkohowever
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By using a simple thermodynamical method we confirm the finding of Chavanis and Harko that stable Bose-Einstein condensate stars can form. However, by using a thermodynamically consistent boson equation of state, we obtain a less massive Bose-Einstein condensate star compared to the one predicted by Chavanis and Harko. We also obtain that the maximum mass of a boson star is insensitive to the change of matter temperature. However, the mass of boson star with relatively large radius depends significantly on the temperature of the boson matter.

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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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