A charged fluid sphere in D space-time dimensions with vanishing normal pressure

1992 ◽  
Vol 70 (5) ◽  
pp. 341-344 ◽  
Author(s):  
C. Wolf

The metric for a charged fluid sphere in D space-time dimensions is found for the case of vanishing normal pressure. The parameters in the solutions are found by matching the interior solution to the exterior Reissner–Nordstròm solution.






1975 ◽  
Vol 29 (2) ◽  
pp. 357-363 ◽  
Author(s):  
A. Banerjee ◽  
N. Chakravorty ◽  
S. B. Duttachoudhury


1979 ◽  
Vol 20 (10) ◽  
pp. 2455-2468 ◽  
Author(s):  
Bahram Mashhoon ◽  
M. Hossein Partovi


2021 ◽  
Vol 81 (1) ◽  
Author(s):  
Ranjan Sharma ◽  
Naresh Dadhich ◽  
Shyam Das ◽  
Sunil D. Maharaj

AbstractWe wish to construct a model for charged star as a generalization of the uniform density Schwarzschild interior solution. We employ the Vaidya and Tikekar ansatz (Astrophys Astron 3:325, 1982) for one of the metric potentials and electric field is chosen in such a way that when it is switched off the metric reduces to the Schwarzschild. This relates charge distribution to the Vaidya–Tikekar parameter, k, indicating deviation from sphericity of three dimensional space when embedded into four dimensional Euclidean space. The model is examined against all the physical conditions required for a relativistic charged fluid sphere as an interior to a charged star. We also obtain and discuss charged analogue of the Buchdahl compactness bound.



2019 ◽  
Vol 79 (11) ◽  
Author(s):  
Yan Peng

AbstractRecently, with numerical methods, Hod clarified the validity of Thorne hoop conjecture for spatially regular static charged fluid spheres, which were considered as counterexamples against the hoop conjecture. In this work, we provide an analytical proof on Thorne hoop conjecture in the spatially regular static charged fluid sphere spacetimes.





1976 ◽  
Vol 7 (6) ◽  
pp. 493-499 ◽  
Author(s):  
A. Nduka


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