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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/38863
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dc.contributor.authorFerraz, K.-
dc.contributor.authorFrancisco, G.-
dc.date.accessioned2014-05-20T15:29:14Z-
dc.date.accessioned2016-10-25T18:04:28Z-
dc.date.available2014-05-20T15:29:14Z-
dc.date.available2016-10-25T18:04:28Z-
dc.date.issued1992-02-15-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.45.1158-
dc.identifier.citationPhysical Review D. College Pk: American Physical Soc, v. 45, n. 4, p. 1158-1162, 1992.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/38863-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/38863-
dc.description.abstractThe numerical simulation of the mixmaster universe serves the purpose of suggesting two kinds of results. The intrinsic time evolution, during contraction, will be seen to be nonchaotic. This is a necessary feature of relativistic cosmological models undergoing this kind of motion. The mixmaster model also provides a clue on how to define chaoticity for systems described by nonautonomous sets of differential equations.en
dc.format.extent1158-1162-
dc.language.isoeng-
dc.publisherAmerican Physical Soc-
dc.sourceWeb of Science-
dc.titleMIXMASTER NUMERICAL BEHAVIOR AND GENERALIZATIONSen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405 SAO PAULO,BRAZIL-
dc.description.affiliationUnespUNIV ESTADUAL PAULISTA,INST FIS TEOR,RUA PAMPLONA 145,BR-01405 SAO PAULO,BRAZIL-
dc.identifier.doi10.1103/PhysRevD.45.1158-
dc.identifier.wosWOS:A1992HE35200017-
dc.rights.accessRightsAcesso restrito-
dc.identifier.fileWOSA1992HE35200017.pdf-
dc.relation.ispartofPhysical Review D-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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