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Generalized Durgapal–Fuloria relativistic stellar models

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dc.contributor.author Komathiraj, K.
dc.contributor.author Sharma, Ranjan
dc.contributor.author Das, Shyam
dc.contributor.author Maharaj, Sunil D.
dc.date.accessioned 2020-01-27T05:18:03Z
dc.date.available 2020-01-27T05:18:03Z
dc.date.issued 2019-10
dc.identifier.citation Komathiraj, K., Sharma, R., Das, S. et al. Generalized Durgapal–Fuloria relativistic stellar models. J Astrophys Astron 40, 37 (2019). https://doi.org/10.1007/s12036-019-9605-2 en_US
dc.identifier.issn 0973-7758
dc.identifier.issn 0250-6335
dc.identifier.other https://doi.org/10.1007/s12036-019-9605-2
dc.identifier.uri https://link.springer.com/article/10.1007/s12036-019-9605-2
dc.identifier.uri http://ir.lib.seu.ac.lk/handle/123456789/4312
dc.description.abstract We present a new class of closed-form solutions to the Einstein–Maxwell system of equations for a static spherically symmetric anisotropic star in the presence of an electric field by generalizing earlier approaches. The field equations are integrated by specifying the form of the electric field, anisotropic factor, and one of the gravitational potentials which are physically reasonable. We regain some of the earlier solutions of Durgapal and Fuloria (1985), Gupta and Maurya (2011) and Maurya et al. (2015) as special cases. A detailed physical analysis of the solution indicates the physical viability for modelling anisotropic charged superdense stars. en_US
dc.language.iso en_US en_US
dc.publisher Springer India en_US
dc.subject Einstein–Maxwell system en_US
dc.subject Exact solution en_US
dc.subject Relativistic stars en_US
dc.title Generalized Durgapal–Fuloria relativistic stellar models en_US
dc.type Article en_US


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