Tolman - Bayin type static charged fluid spheres in general relativity

dc.contributor.authorRay, Saibal
dc.contributor.authorDas, Basanti
dc.date.accessioned2012-03-12T05:11:52Z
dc.date.available2012-03-12T05:11:52Z
dc.date.issued2011-07-05
dc.description.abstractIn a static spherically symmetric Einstein-Maxwell spacetime the class of astrophysical solu- tion found out by Ray and Das (2002) and Pant and Sah (1979) are revisited here in connection to the phenomenological relationship between the gravitational and electromagnetic fields. It is qualitatively shown that the charged relativistic stars of Tolman (1939) and Bayin (1978) type are of purely electromagnetic origin. The existence of this type of astrophysical solutions is a probable extension of Lorentz’s conjecture that electron-like extended charged particle possesses only ‘electromagnetic mass’ and no ‘material mass’.en_US
dc.description.sponsorshipStars : interior.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1173
dc.language.isoenen_US
dc.relation.ispartofseriesIUCAA Preprints;41/03
dc.subjectGravitationen_US
dc.subjectRelativityen_US
dc.titleTolman - Bayin type static charged fluid spheres in general relativityen_US
dc.typeArticleen_US

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