Mixmaster numerical behavior and generalizations

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dc.contributor.authorFerraz, K. [UNESP]
dc.contributor.authorFrancisco, G. [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)
dc.date.accessioned2022-04-28T19:53:24Z
dc.date.available2022-04-28T19:53:24Z
dc.date.issued1992-01-01
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. © 1992 The American Physical Society.en
dc.description.affiliationInstituto de Física Tearica (Universidade Estadual Paulista), Rua Pamplona 145, 01405 Sao Paulo, Sao Paulo
dc.description.affiliationUnespInstituto de Física Tearica (Universidade Estadual Paulista), Rua Pamplona 145, 01405 Sao Paulo, Sao Paulo
dc.format.extent1158-1162
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.45.1158
dc.identifier.citationPhysical Review D, v. 45, n. 4, p. 1158-1162, 1992.
dc.identifier.doi10.1103/PhysRevD.45.1158
dc.identifier.issn0556-2821
dc.identifier.scopus2-s2.0-0004365354
dc.identifier.urihttp://hdl.handle.net/11449/223854
dc.language.isoeng
dc.relation.ispartofPhysical Review D
dc.sourceScopus
dc.titleMixmaster numerical behavior and generalizationsen
dc.typeArtigo
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulopt

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São Paulo - IFT - Instituto de Física Teórica