Boson Star Rotation: A Newtonian Approximation
Astrophysics
2009-10-28 v1 General Relativity and Quantum Cosmology
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.
Keywords
Cite
@article{arxiv.astro-ph/9508034,
title = {Boson Star Rotation: A Newtonian Approximation},
author = {Vanda Silveira and Claudio M. G. de Sousa},
journal= {arXiv preprint arXiv:astro-ph/9508034},
year = {2009}
}
Comments
17 pages, Latex, 3 figures available upon request