Relativistic anisotropic stellar models with Tolman VII spacetime

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dc.contributor.authorBhar, Piyali
dc.contributor.authorMurad, Mohammad Hassan
dc.contributor.authorPant, Neeraj
dc.date.accessioned2016-12-07T03:50:41Z
dc.date.available2016-12-07T03:50:41Z
dc.date.issued2015-09
dc.descriptionThis 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
dc.description.abstractIn 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.
dc.identifier.citationBhar, 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
dc.identifier.otherhttps://dspace.bracu.ac.bd/server/api/core/items/53bfc07b-8bfa-408d-8ba3-63dcd5edf569
dc.identifier.urihttp://hdl.handle.net/10361/7135
dc.language.isoes
dc.publisher© 2015, Springer Science+Business Media Dordrecht
dc.sourceBRAC University Institutional Repository
dc.subjectAnisotropic fluid sphere
dc.subjectCompact stars
dc.subjectEquation of state
dc.subjectExact solution
dc.subjectGeneral relativity
dc.subjectRelativistic astrophysics
dc.subjectRelativistic stars
dc.titleRelativistic anisotropic stellar models with Tolman VII spacetime
dc.typeArticle

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