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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3165
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dc.contributor.authorVishveshwara, C. V-
dc.date.accessioned2008-08-18T09:19:26Z-
dc.date.available2008-08-18T09:19:26Z-
dc.date.issued1999-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 20, No. 3 - 4, pp. 103 - 120en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3165-
dc.description.abstractIn this article, we first consider briefly the basic properties of the non –rotating schwarzschild black hole and the rotating Kerr Black hole rotational effects are then described in static and stationary spacetimes with arial symmetry by studying inertial forces , gyroscopic precession and gravi-electromagnetism. The results are applied to the black hole spacetimes.en
dc.format.extent1250736 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999JApA...20..103Ven
dc.subjectBlack holesen
dc.subjectRotationen
dc.subjectInertial forcesen
dc.subjectGyroscopic precessionen
dc.subjectGravi electromagnetismen
dc.titleBlack Holes and Rotationen
dc.typeArticleen
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