General Solution of Static Sphere of Perfect Fluid and Dust of Uniform Density Using Isotropic Line Element

Relativity, Solution of Static Sphere

Authors

  • C.D. Marathe Dnyanasadhana College, Thane – 400604, India
  • J.J. Rawal The Indian Planetary Society, Mumbai – 400092, India
  • Bijan Nikouravan 3Department of Physics, Islamic Azad University (IAU),Varamin, Pishva Branch, Iran 4Department of Physics, University of Malaya, 50603, Kuala Lumpur, Malaysia

DOI:

https://doi.org/10.14331/ijfps.2012.330039

Keywords:

Dust, Cluster of stars, stars, Newtonian Approximation Astrophysics

Abstract

The general solution of a static sphere of perfect fluid of uniform density using isotropic line element has been obtained by using the additional condition of continuity at the boundary

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Author Biography

Bijan Nikouravan, 3Department of Physics, Islamic Azad University (IAU),Varamin, Pishva Branch, Iran 4Department of Physics, University of Malaya, 50603, Kuala Lumpur, Malaysia

 

 

REFERENCES


Eddington, A. S. (1924). The mathematical theory of relativity. Cambridge, England, 101. Shrivastav, M. K. (1999) Ph.D Thesis, University of Mumbai, India.

Rawal, J., Deshpande, V., Kelkar, V., & Shenoy, R. (1991). Axially symmetric Schwarzschild interior solution for a very slowly rotating star. Bulletin of the Astronomical Society of India, 19, 76.

Rawal, J., Kelkar, V., Deshpande, V., & Shenoy, R. (1989). Schwarzschild interior solution for a very slowly rotating star. Indian Journal of Physics Section B, 63, 362-366.

Wyman, M. (1946). Schwarzschild interior solution in an isotropic coordinate system. Physical review, 70, 74-76.

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Published

2012-12-31

Issue

Vol. 2 No. 4 (2012): IJFPS

Section

ORIGINAL ARTICLES

License

Copyright (c) 2020 International Journal of Fundamental Physical Science

Creative Commons License

This work is licensed under a Creative Commons Attribution 4.0 International License.

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