A Dynamical Approach to the Exterior Geometry of a Perfect Fluid as a Relativistic Star
arXiv:1111.5124
Abstract
In this article, we assume that a cold charged perfect fluid is constructing a spherical relativistic star. Our purpose is the investigation of the dynamical properties of its exterior geometry, through simulating the geodesic motion of a charged test particle, while moving on the star.
arXiv comment16 pages, 43 figures