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Relativistic anisotropic stellar models with Tolman VII spacetime

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Date

2015-09

Publisher

© 2015, Springer Science+Business Media Dordrecht

Authors

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URI

http://hdl.handle.net/10361/7135

Citation

Bhar, P., Murad, M. H., & Pant, N. (2015). Relativistic anisotropic stellar models with tolman VII spacetime. Astrophysics and Space Science, 359(1) doi:10.1007/s10509-015-2462-9

Abstract

In this paper we have studied the behavior of static spherically symmetric relativistic objects with locally anisotropic matter distribution considering the Tolman VII form for the gravitational potential grr in curvature coordinates together with the linear relation between the energy density and the radial pressure. The interior spacetime has been matched continuously to the exterior Schwarzschild geometry. We have investigated and analyzed different physical properties of the stellar model and presented graphically.

Keywords

Anisotropic fluid sphere, Compact stars, Equation of state, Exact solution, General relativity, Relativistic astrophysics, Relativistic stars

Description

This article was published in the Astrophysics and Space Science [© 2015, Springer Science+Business Media Dordrecht] and the definite version is available at : http://dx.doi.org/10.1007/s10509-015-2462-9. The Journal's website is at: http://link.springer.com/article/10.1007%2Fs10509-015-2462-9

Publisher Link

http://link.springer.com/article/10.1007%2Fs10509-015-2462-9

Department

Department of Mathematics and Natural Sciences

Type

Article

Collections

Article