Relativistic anisotropic stellar models with Tolman VII spacetime
No Thumbnail Available
Date
2015-09
Journal Title
Journal ISSN
Volume Title
Publisher
© 2015, Springer Science+Business Media Dordrecht
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.
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
Keywords
Anisotropic fluid sphere, Compact stars, Equation of state, Exact solution, General relativity, Relativistic astrophysics, Relativistic stars
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