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Boson Star Rotation: A Newtonian Approximation

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arxiv astro-ph/9508034 v1 pith:Y74KAC5M submitted 1995-08-08 astro-ph gr-qc

Vanda Silveira , Claudio M. G. de Sousa (Universidade de Brasilia) This is my paper · ORCID
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keywords approximationnewtonianangularapplicabilitybosonbosoniccompactconstructed
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Using the Newtonian approximation, we study rotating compact bosonic objects. The equations which describe stationary states with non-zero angular momentum are constructed and some numerical results are presented as examples. Limits on the applicability of the Newtonian approximation are discussed.

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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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