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

Mohsen Fathi

doi:10.1088/1674-1137/37/2/025101

Chinese Physics C> 2013, Vol. 37> Issue(2) : 025101 DOI: 10.1088/1674-1137/37/2/025101

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

Mohsen Fathi ^,

Department of Physics, Islamic Azad University, Central Tehran Branch, Tehran, Iran

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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.

References

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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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沈阳化工大学材料科学与工程学院沈阳 110142

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

Received Date: 2012-03-27

Accepted Date: 2012-05-30

Available Online: 2013-02-05

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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