General Relativistic Study of Thin Disk with Radial Flow in Kerr – Newman Geometry
American Journal of Astronomy and Astrophysics
Volume 5, Issue 6, November 2017, Pages: 57-62
Received: Dec. 23, 2017;
Accepted: Jan. 8, 2018;
Published: Jan. 19, 2018
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Kameshwar Nath Mishra, Department of Applied Mathematics, Bhilai Institute of Technology, Durg, India
Varull Mishra, Department of Electrical Engineering, National Institute of Technology, Raipur, India
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A detailed general relativistic formulation of the thin disk with the radial flow in Kerr – Newman geometry. The effects of rotation through an angular momentum a and charge Q were obtained on pressure, velocity and density for co rotating and counter rotating thin disk.
Kerr – Newman Black Hole, Thin Disk, Radial Flow
To cite this article
Kameshwar Nath Mishra,
General Relativistic Study of Thin Disk with Radial Flow in Kerr – Newman Geometry, American Journal of Astronomy and Astrophysics.
Vol. 5, No. 6,
2017, pp. 57-62.
Copyright © 2017 Authors retain the copyright of this article.
This article is an open access article distributed under the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/
) which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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