MIXMASTER NUMERICAL BEHAVIOR AND GENERALIZATIONS

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T15:29:14Z
dc.date.accessioned2022-10-05T16:52:55Z
dc.date.available2014-05-20T15:29:14Z
dc.date.available2022-10-05T16:52:55Z
dc.date.created2014-05-20T15:29:14Z
dc.date.issued1992-02-15
dc.identifierPhysical Review D. College Pk: American Physical Soc, v. 45, n. 4, p. 1158-1162, 1992.
dc.identifier0556-2821
dc.identifierhttp://hdl.handle.net/11449/38863
dc.identifier10.1103/PhysRevD.45.1158
dc.identifierWOS:A1992HE35200017
dc.identifierWOSA1992HE35200017.pdf
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3910102
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.
dc.languageeng
dc.publisherAmerican Physical Soc
dc.relationPhysical Review D
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.titleMIXMASTER NUMERICAL BEHAVIOR AND GENERALIZATIONS
dc.typeArtigo


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