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dc.contributor.authorKopeikin, Sergei M.eng
dc.date.issued2002eng
dc.description.abstractWe study the effect of retardation of gravity in binary pulsars. It appears in pulsar timing formula as a periodic excess time delay to the Shapiro effect. The retardation of gravity effect can be large enough for observation in binary pulsars with the nearly edgewise orbits and relatively large ratio of the projected semimajor axis, x, to the orbital period of the pulsar, Pb. If one succeeds in measuring the retardation of gravity it will give further experimental evidence in favor of General Relativity.eng
dc.identifier.citationarXiv:gr-qc/0210076v1eng
dc.identifier.urihttp://hdl.handle.net/10355/6964eng
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/0210/0210076v1.pdfeng
dc.subjectgeneral relativityeng
dc.subjectbinary pulsarseng
dc.subjectretardation of gravityeng
dc.subject.lcshPulsars -- Researcheng
dc.subject.lcshGravitational fieldseng
dc.subject.lcshGeneral relativity (Physics) -- Experimentseng
dc.titleRetardation of Gravity in Binary Pulsarseng
dc.typeArticleeng


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