A family of solutions to the Einstein–Maxwell system of equations describing relativistic charged fluid spheres

Pramana ◽  
2018 ◽  
Vol 90 (5) ◽  
Author(s):  
K Komathiraj ◽  
Ranjan Sharma
2000 ◽  
Vol 41 (7) ◽  
pp. 4752-4764 ◽  
Author(s):  
T. Harko ◽  
M. K. Mak

2006 ◽  
Vol 21 (09) ◽  
pp. 751-757 ◽  
Author(s):  
A. N. ALIEV

Black hole solutions in higher dimensional Einstein and Einstein–Maxwell gravity have been discussed by Tangherlini as well as Myers and Perry a long time ago. These solutions are the generalizations of the familiar Schwarzschild, Reissner–Nordström and Kerr solutions of four-dimensional general relativity. However, higher dimensional generalization of the Kerr–Newman solution in four dimensions has not been found yet. As a first step in this direction we shall report on a new solution of the Einstein–Maxwell system of equations that describes an electrically charged and slowly rotating black hole in five dimensions.


2013 ◽  
Vol 350 (1) ◽  
pp. 293-305 ◽  
Author(s):  
Mohammad Hassan Murad ◽  
Saba Fatema

1966 ◽  
Vol 44 (10) ◽  
pp. 2403-2409 ◽  
Author(s):  
Kwok-Kee Tam

The system of equations governing the behavior of an ideal, relativistic charged, fluid are derived by a variational principle, through the introduction of a generalized Clebsch transform. Some simple applications are considered.


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