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Interior Black-Hole Solution with Anisotropic Fluid
A.H. Hasmaniahhasmani@gmail.comDepartment of MathematicsSardar Patel UniversityVallabh Vidyanagar, IndiaView full profile → , V.G. Khambholjavrajassp@gmail.comDepartment of MathematicsB.V.M. Engineering CollegeVallabh Vidyanagar, IndiaView full profile →
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- Received:
- 07 Nov 2011
- Accepted:
- 06 Jan 2012
- Published Online:
- 03 Jun 2013
- Article type:
- Original Articles
- Language:
- EN
- Article no.:
- 1726037X.2012.10698606
- Pages:
- 47–52
Abstract
The result of gravitational collapse of a compact body is believed to be a singularity hidden beyond its Schwarzschild radius known as a black hole. In the interior black hole region, a remarkable change occurs in the nature of the spacetime, namely the external spatial radial and temporal coordinates exchange their characters. So, the interior black hole solution is represented by a non-static spacetime. With the assumption that the material content of the spherical body is an anisotropic fluid, we have carried out a brief study of the annular space time metric. The case of isotropic pressures is discussed as a particular case and a regular solution has been obtained.
Keywords
References
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- Khambholja, Vrajeshkumar. , Depatment of Mathematics, Sardar Patel University . (Unpublished)
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