Boson Star Rotation: A Newtonian Approximation

Preprint

8 August 1995

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9508034

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

NEWTONIAN APPROXIMATION
ANGULAR MOMENTUM
BOSONIC OBJECTS
STAR ROTATION
BOSON STAR
COMPACT

All Related Versions

Version 1, 1995-08-08, ArXiv
Published version: Physical Review D, 52 (10), 5724.

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