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Towards an Analytic Construction of the Wavefunction of Boson Stars

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arxiv 1706.04272 v2 pith:OHPTD5DD submitted 2017-06-13 hep-th astro-ph.COgr-qc

Felix Kling , Arvind Rajaraman This is my paper · ORCID
classification hep-thastro-ph.COgr-qc
keywords bosonstarsequationsprofilescalarsolutionaccuracyanalytic
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abstract

Light scalar fields can form gravitationally bound compact objects called boson stars. The profile of boson stars in the Newtonian limit is described by the Gross-Pitaevskii-Poisson equations. We present a semi-analytic solution to these equations and construct the profile of boson stars formed by a non-interacting scalar field. Our solution is stable with respect to numerical errors and has accuracy better than $10^{-6}$ over the entire range.

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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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