Relativistic model of anisotropic charged fluid sphere in general relativity

2015 ◽  
Vol 361 (1) ◽  
Author(s):  
Neeraj Pant ◽  
N. Pradhan ◽  
Rajeev K. Bansal
Keyword(s):  
General Relativity ◽  
Fluid Sphere ◽  
Relativistic Model ◽  
Charged Fluid ◽  
Charged Fluid Sphere

Nonstatic charged fluid sphere in general relativity

1975 ◽  
Vol 29 (2) ◽  
pp. 357-363 ◽  
Author(s):  
A. Banerjee ◽  
N. Chakravorty ◽  
S. B. Duttachoudhury
Keyword(s):  
General Relativity ◽  
Fluid Sphere ◽  
Charged Fluid ◽  
Charged Fluid Sphere

Charged fluid sphere in general relativity

1979 ◽  
Vol 20 (12) ◽  
pp. 2537-2539 ◽  
Author(s):  
D. N. Pant ◽  
A. Sah
Keyword(s):  
General Relativity ◽  
Fluid Sphere ◽  
Charged Fluid ◽  
Charged Fluid Sphere

Gravitational collapse of a charged fluid sphere

1979 ◽  
Vol 20 (10) ◽  
pp. 2455-2468 ◽  
Author(s):  
Bahram Mashhoon ◽  
M. Hossein Partovi
Keyword(s):  
Gravitational Collapse ◽  
Fluid Sphere ◽  
Charged Fluid ◽  
Charged Fluid Sphere

scholarly journals Analytical studies on the hoop conjecture in charged curved spacetimes

2019 ◽  
Vol 79 (11) ◽  
Author(s):  
Yan Peng
Keyword(s):  
Numerical Methods ◽  
Fluid Sphere ◽  
Charged Fluid ◽  
Charged Fluid Sphere ◽  
Analytical Studies ◽  
Curved Spacetimes ◽  
Analytical Proof ◽  
Hoop Conjecture ◽  
Fluid Spheres

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.

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

1992 ◽  
Vol 70 (5) ◽  
pp. 341-344 ◽  
Author(s):  
C. Wolf
Keyword(s):  
Normal Pressure ◽  
Space Time ◽  
Fluid Sphere ◽  
Interior Solution ◽  
Charged Fluid ◽  
Charged Fluid Sphere

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.

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