A Dynamical Approach to the Exterior Geometry of a Perfect Fluid as a Relativistic Star
Mohsen Fathi
TL;DR
This paper investigates the exterior geometry of a spherical relativistic star composed of a cold charged perfect fluid by simulating the geodesic motion of charged test particles to understand its dynamical properties.
Contribution
It introduces a dynamical approach to analyze the exterior geometry of charged relativistic stars through geodesic simulations.
Findings
Charged test particles exhibit specific geodesic behaviors around the star.
The exterior geometry influences particle trajectories significantly.
The study provides insights into the star's gravitational and electromagnetic field interactions.
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.
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