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dc.contributor.authorMurad, Mohammad Hassan
dc.contributor.authorFatema, Saba
dc.date.accessioned2018-10-16T06:17:59Z
dc.date.available2018-10-16T06:17:59Z
dc.date.issued2013-08-24
dc.identifier.urihttp://hdl.handle.net/20.500.11948/3396
dc.description.abstractIn continuation of recent work done by the present authors (Int. J. Theor. Phys. 2013, doi: 10.1007/s10773-013-1538-y, hereafter paper I) some new exact families of static spherically symmetric perfect fluid solution of Einstein–Maxwell gravitational field equations are presented. These solutions and the corresponding equations of state, presented in parametric form, may be astrophysically significant in constructing relativistic stellar models of electrically charged self-bound stars. Full Text Link:https://doi.org/10.1007/s10773-013-1752-7en_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.subjectGeneral relativityen_US
dc.subjectAstrophysicsen_US
dc.subjectEinstein–Maxwell Exact solutionen_US
dc.subjectCharged fluid sphereen_US
dc.subjectSchwarzschild coordinatesen_US
dc.subjectCompact starsen_US
dc.subjectReissner–Nordströmen_US
dc.subjectRelativistic starsen_US
dc.subjectSelf-bound starsen_US
dc.subjectEquation of stateen_US
dc.titleSome Exact Relativistic Models of Electrically Charged Self-bound Starsen_US
dc.typeArticleen_US


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