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dc.contributor.authorMaartens, R. (Roy)eng
dc.contributor.authorMashhoon, Bahrameng
dc.contributor.authorMatravers, Davideng
dc.date.issued2002eng
dc.descriptiondoi: 10.1088/0264-9381/19/2/301eng
dc.description.abstractWe analyse parallel transport of a vector field around an equatorial orbit in the Kerr and stationary axisymmetric spacetimes that are reflection symmetric about their equatorial planes. As in the Schwarzschild spacetime, there is a band structure of holonomy invariance. The new feature introduced by rotation is a shift in the timelike component of the vector, which is the holonomic manifestation of the gravitomagnetic clock effect.eng
dc.identifier.citationRoy Maartens et al 2002 Class. Quantum Grav. 19 195eng
dc.identifier.issn0264-9381eng
dc.identifier.urihttp://hdl.handle.net/10355/8578eng
dc.languageEnglisheng
dc.publisherAmerican Institute of Physicseng
dc.relation.ispartofcollectionUniversity of Missouri--Columbia. College of Arts and Sciences. Department of Physics and Astronomy. Physics and Astronomy publicationseng
dc.subject.lcshGravitationeng
dc.subject.lcshSpace and time -- Mathematical modelseng
dc.subject.lcshTopologyeng
dc.subject.lcshQuantum gravityeng
dc.subject.lcshGeometric quantizationeng
dc.titleHolonomy and gravitomagnetismeng
dc.typeArticleeng


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