A Dynamical Approach to the Exterior Geometry of a Perfect Fluid as a Relativistic Star

Details A Dynamical Approach to the Exterior Geometry of a Perfect Fluid as a Relativistic Star A Dynamical Approach to the Exterior Geometry of a Perfect Fluid as a Relativistic Star

2011-11-22

arxiv.org/abs/1111.5124v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

25 pages, 43 figures. The article had a major revision, a Lagrangian formalism used to simulate possible orbits in RN geometry

Scientific paper

In this article, we assume that a cold charged perfect fluid is constructing
a spherical relativistic star. Our purpose would be 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.

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