Newtonian limit of axially-symmetric spacetimes

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dc.contributor.authorBohun, C. Sean
dc.contributor.authorPerry, G. Phillip
dc.date.accessioned2010-04-15T23:09:32Z
dc.date.available2010-04-15T23:09:32Z
dc.date.copyright1992en
dc.date.issued2010-04-15T23:09:32Z
dc.description.abstractWe illustrate how the Ehlers' formal mathematical definition of the Newtonian limit requires additional information to successfully determine the Newtonian limit. This information can be obtained through the physical arguments of Cooperstock's definition. We show that Ehlers' formalism is equivalent to Cooperstock's derivation of the Newtonian limit when the physical arguments are included in the former definition.en
dc.identifier.urihttp://hdl.handle.net/1828/2610
dc.language.isoenen
dc.relation.ispartofseriesDMS-614-IRen
dc.subjecttechnical reports (mathematics and statistics)
dc.subject.departmentDepartment of Mathematics and Statistics
dc.subject.departmentDepartment of Physics and Astronomy
dc.titleNewtonian limit of axially-symmetric spacetimesen
dc.typeTechnical Reporten

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