Please use this identifier to cite or link to this item: http://ir.lib.seu.ac.lk/handle/123456789/6251
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dc.contributor.authorKomathiraj, K.-
dc.contributor.authorSharma, Ranjan-
dc.contributor.authorChanda, Samstuti-
dc.date.accessioned2022-09-28T06:21:13Z-
dc.date.available2022-09-28T06:21:13Z-
dc.date.issued2022-09-12-
dc.identifier.citationAstrophysics and Space Science,367(9):p.86,Sep,2022en_US
dc.identifier.issn1572-946X-
dc.identifier.urihttps://doi.org/10.1007/s10509-022-04119-5-
dc.identifier.urihttp://ir.lib.seu.ac.lk/handle/123456789/6251-
dc.description.abstractFor a static, spherically symmetric, anisotropic and charged distribution of matter, we present a new class of exact solutions to the Einstein-Maxwell system. By assuming specific forms of the electric field and anisotropy, we transform the master equation of the Einstein-Maxwell system to Bessel and modified Bessel differential equations. The subsequent solutions turn out to be generalizations of the isotropic and uncharged stellar model of Finch and Skea (1989), the isotropic and charged stellar model of Hansraj and Maharaj (2006) and the anisotropic and charged stellar model of Maharaj et al. (2017). We analyze the physical viability of the solutions and utilize one particular class of solutions to examine the effects of charge and anisotropy on the mass-radius relationship of compact stars.en_US
dc.language.isoen_USen_US
dc.publisherSpringer Natureen_US
dc.subjectEinstein-Maxwell systemen_US
dc.subjectExact solutionen_US
dc.subjectCompact staren_US
dc.subjectMass-radius relationshipen_US
dc.titleEffects of electric field and anisotropy on the mass-radius relationship of a particular class of compact stars.en_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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