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dc.contributor.authorChicone, Carmen Charleseng
dc.contributor.authorMashhoon, Bahrameng
dc.date.issued2004eng
dc.descriptiondoi: 10.1088/0264-9381/21/24/L01eng
dc.description.abstractIn the description of relative motion in accelerated systems and gravitational fields, inertial and tidal accelerations must be taken into account, respectively. These involve a critical speed that in the first approximation can be simply illustrated in the case of motion in one dimension. For one-dimensional motion, such first-order accelerations are multiplied by (1 − V2/V2c), where V_c=c/\sqrt{2} is the critical speed. If the speed of relative motion exceeds Vc, there is a sign reversal with consequences that are contrary to Newtonian expectations.eng
dc.identifier.citationC Chicone and B Mashhoon 2004 Class. Quantum Grav. 21 L139eng
dc.identifier.issn0264-9381eng
dc.identifier.urihttp://hdl.handle.net/10355/8556eng
dc.languageEnglisheng
dc.publisherAmerican Institute of Physicseng
dc.relation.ispartofMathematics publications (MU)eng
dc.relation.ispartofcollectionUniversity of Missouri-Columbia. College of Arts and Sciences. Department of Mathematics.eng
dc.rightsOpenAccess.eng
dc.rights.licenseThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License.
dc.subjectequations of motioneng
dc.subjectclassical general relativityeng
dc.subjectapproximation methodseng
dc.subject.lcshElectromagnetic fieldseng
dc.subject.lcshGravitationeng
dc.subject.lcshCosmologyeng
dc.titleSignificance of c /sqrt2 in relativistic physicseng
dc.typeArticleeng


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