Cold Bose stars: Self-gravitating Bose-Einstein condensates

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Self-Gravitating Systems, Continuous Media And Classical Fields In Curved Spacetime, Boson Systems, Other Topics On Stars

Scientific paper

Using the Gross-Pitaevskii equation and the Thomas-Fermi approximation, we study a cold star composed of a dilute Bose-Einstein condensate. The exact solution of the mass distribution of a nonrotating star is obtained. For a slowly rotating star, the second-order perturbative solutions are obtained. It is found that one solution is stable and the other is metastable.

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