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dc.contributor.authorCiufolini, I.eng
dc.contributor.authorKopeikin, Sergei M.eng
dc.contributor.authorMashhoon, Bahrameng
dc.contributor.authorRicci, F.eng
dc.date.issued2002eng
dc.description.abstractWe study the gravitational time delay in ray propagation due to rotating masses in the linear approximation of general relativity. Simple expressions are given for the gravitomagnetic time delay that occurs when rays of radiation cross a slowly rotating shell, equation (14), and propagate in the field of a distant rotating source, equation (16). Moreover, we calculate the local gravitational time delay in the G¨odel universe. The observational consequences of these results in the case of weak gravitational lensing are discussed.eng
dc.identifier.citationarXiv:gr-qc/0210015v2eng
dc.identifier.urihttp://hdl.handle.net/10355/6959eng
dc.languageEnglisheng
dc.publisherarXiveng
dc.relation.ispartofcollectionUniversity of Missouri--Columbia. College of Arts and Sciences. Department of Physics and Astronomy. Physics and Astronomy publicationseng
dc.source.urihttp://arxiv.org/PS_cache/gr-qc/pdf/0210/0210015v2.pdfeng
dc.subjectgravitomagnetismeng
dc.subjecttime delayeng
dc.subjectgravitational lensingeng
dc.subject.lcshGravitational fieldseng
dc.subject.lcshElectromagnetismeng
dc.subject.lcshGravitational lenseseng
dc.titleOn the Gravitomagnetic Time Delayeng
dc.typeArticleeng


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