Nonlinear Gravitational Waves: Their Form and Effects

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.contributorUniversidade Federal do ABC (UFABC)
dc.date.accessioned2013-09-30T18:53:10Z
dc.date.accessioned2014-05-20T14:09:17Z
dc.date.accessioned2022-10-05T15:04:57Z
dc.date.available2013-09-30T18:53:10Z
dc.date.available2014-05-20T14:09:17Z
dc.date.available2022-10-05T15:04:57Z
dc.date.created2013-09-30T18:53:10Z
dc.date.created2014-05-20T14:09:17Z
dc.date.issued2010-03-01
dc.identifierInternational Journal of Theoretical Physics. New York: Springer/plenum Publishers, v. 49, n. 3, p. 549-563, 2010.
dc.identifier0020-7748
dc.identifierhttp://hdl.handle.net/11449/24138
dc.identifier10.1007/s10773-009-0236-2
dc.identifierWOS:000274904000012
dc.identifier1599966126072450
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3897338
dc.description.abstractA gravitational wave must be nonlinear to be able to transport its own source, that is, energy and momentum. A physical gravitational wave, therefore, cannot be represented by a solution to a linear wave equation. Relying on this property, the second-order solution describing such physical waves is obtained. The effects they produce on free particles are found to consist of nonlinear oscillations along the direction of propagation.
dc.languageeng
dc.publisherSpringer/plenum Publishers
dc.relationInternational Journal of Theoretical Physics
dc.relation0.968
dc.relation0,285
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectGravitational waves
dc.subjectNonlinear gravitational waves
dc.titleNonlinear Gravitational Waves: Their Form and Effects
dc.typeArtigo


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