A dynamical approach to the exterior geometry of a perfect fluid as a relativistic star

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Mohsen Fathi. A dynamical approach to the exterior geometry of a perfect fluid as a relativistic star[J]. Chinese Physics C, 2013, 37(2): 025101. doi: 10.1088/1674-1137/37/2/025101
Mohsen Fathi. A dynamical approach to the exterior geometry of a perfect fluid as a relativistic star[J]. Chinese Physics C, 2013, 37(2): 025101.  doi: 10.1088/1674-1137/37/2/025101 shu
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Received: 2012-03-27
Revised: 2012-05-30
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A dynamical approach to the exterior geometry of a perfect fluid as a relativistic star

    Corresponding author: Mohsen Fathi,
  • Department of Physics, Islamic Azad University, Central Tehran Branch, Tehran, Iran

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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