A dynamical approach to the exterior geometry of a perfect fluid as a relativistic star
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.
- Publication:
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Chinese Physics C
- Pub Date:
- February 2013
- DOI:
- Bibcode:
- 2013ChPhC..37b5101M