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.
Boson Star Rotation: A Newtonian Approximation
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abstract
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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Durgapal-Fuloria Bose-Einstein condensate stars within $ f(R,T) $ gravity theory
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.