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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.contributor.departmentDepartment of Mathematics and Natural Sciences
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%2Fs10509-015-2462-9en_US
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.en_US
dc.description.versionPublished
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/s10509-015-2462-9en_US
dc.identifier.issn0004640X
dc.identifier.urihttp://hdl.handle.net/10361/7135
dc.language.isoesen_US
dc.publisher© 2015, Springer Science+Business Media Dordrechten_US
dc.relation.urihttp://link.springer.com/article/10.1007%2Fs10509-015-2462-9
dc.subjectAnisotropic fluid sphereen_US
dc.subjectCompact starsen_US
dc.subjectEquation of stateen_US
dc.subjectExact solutionen_US
dc.subjectGeneral relativityen_US
dc.subjectRelativistic astrophysicsen_US
dc.subjectRelativistic starsen_US
dc.titleRelativistic anisotropic stellar models with Tolman VII spacetimeen_US
dc.typeArticleen_US

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