Boson Star Rotation: A Newtonian Approximation
arXiv:astro-ph/9508034 · doi:10.1103/PhysRevD.52.5724
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.
17 pages, Latex, 3 figures available upon request