Journal
PHYSICAL REVIEW D
Volume 64, Issue 12, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.64.124009
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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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