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

[1]

Straumann N, Bieri L. Discovering the Expanding Universe. Cambridge: Cambridge University Press, 2009[2] Zel'dovich Ya B, Novikov I D. Relativistic Astrophysics, Vol. I: Stars and Relativity. Chicago: University of Chicago Press, 1971[3] Guilfoyle B S. Gen. Rel. Grav., 1999, 31: 1645[4] ZHAI Xiang-Hau, YAUN Ning-Yi, LI Xin-Zhou. Chin. Phys. Lett., 1999, 16(5): 321[5] Blaga P, Mioc V. Europhys. Lett., 1992, 17(3): 275[6] Stuchlik Z. Bull. Astron. Inst. Czechosl., 1983, 34: 129[7] Jorge C, Crispino Luís C B, Rodrigo R M et al. Braz. J. Phys., 2005, 35(4B)[8] Prasanna A R, Vishveshwara C V. Pramana, 1978, 11(4): 359[9] Chandrasekhar S. The Mathematical Theory of Black Holes. New York: Oxford University Press, 1983[10] Hackmann E, Lmmerzahl C. Phys. Rev. Lett., 2008, 100: 171101[11] Hackmann E, Kagramanova V, Kunz J et al. Phys. Rev. D. 2008, 78: 124018[12] Hackmann E, Kagramanova V, Kunz J et al. Europhys. Lett., 2009, 88: 30008[13] Hackmann E, Lmmerzahl C, Kagramanova V et al. Phys. Rev. D, 2010, 81: 044020[14] Hackmann E, Hartmann B, Lmmerzahl C et al. Phys. Rev. D, 2010, 81: 064016[15] Kagramanova V, Kunz J, Hackmann E et al. Phys. Rev. D, 2010, 81: 124044[16] Hackmann E, Hartmann B, Lmmerzahl C et al. Phys. Rev. D, 2010, 82: 044024[17] Hackmann E, Lmmerzahl C. Phys. Rev. D, 2012, 85: 044049[18] Wald Robert M. General Relativity. London: The University of Chicago Press, 1984[19] Nakahara M. Geometry, Topology and Physics. Second Edition. London: Ihstitute of Physics (IOP), 2003[20] Misner C W, Thorne K S, Wheeler J A. Gravitation. Freeman, 1973[21] Greiner W. Classical Mechanics: Sytem of Particles and Hamiltonian Dynamics. New York: Springer-Verlag, 2003[22] Weyl H. Ann. Phys. (Berlin), 1917, 359: 117[23] Lemos José P S, Zanchin Vilson T. Phys. Rev. D, 2010, 81: 124016[24] Majumdar S D. Phys. Rev., 1947, 72: 390[25] Papapetrou A. Proc. R. Irish Acad. A, 1947, 51: 191[26] Schutz Bernard F. A First Course in General Relativity. Second Edition. Cambridge: Cambridge University Press, 2009

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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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