Mixmaster numerical behavior and generalizations

Detalhes bibliográficos
Autor(a) principal: Ferraz, K. [UNESP]
Data de Publicação: 1992
Outros Autores: Francisco, G. [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1103/PhysRevD.45.1158
http://hdl.handle.net/11449/223854
Resumo: The 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.
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spelling Mixmaster numerical behavior and generalizationsThe 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.Instituto de Física Tearica (Universidade Estadual Paulista), Rua Pamplona 145, 01405 Sao Paulo, Sao PauloInstituto de Física Tearica (Universidade Estadual Paulista), Rua Pamplona 145, 01405 Sao Paulo, Sao PauloUniversidade Estadual Paulista (UNESP)Ferraz, K. [UNESP]Francisco, G. [UNESP]2022-04-28T19:53:24Z2022-04-28T19:53:24Z1992-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article1158-1162http://dx.doi.org/10.1103/PhysRevD.45.1158Physical Review D, v. 45, n. 4, p. 1158-1162, 1992.0556-2821http://hdl.handle.net/11449/22385410.1103/PhysRevD.45.11582-s2.0-0004365354Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengPhysical Review Dinfo:eu-repo/semantics/openAccess2022-04-28T19:53:24Zoai:repositorio.unesp.br:11449/223854Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T23:18:34.304654Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Mixmaster numerical behavior and generalizations
title Mixmaster numerical behavior and generalizations
spellingShingle Mixmaster numerical behavior and generalizations
Ferraz, K. [UNESP]
title_short Mixmaster numerical behavior and generalizations
title_full Mixmaster numerical behavior and generalizations
title_fullStr Mixmaster numerical behavior and generalizations
title_full_unstemmed Mixmaster numerical behavior and generalizations
title_sort Mixmaster numerical behavior and generalizations
author Ferraz, K. [UNESP]
author_facet Ferraz, K. [UNESP]
Francisco, G. [UNESP]
author_role author
author2 Francisco, G. [UNESP]
author2_role author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
dc.contributor.author.fl_str_mv Ferraz, K. [UNESP]
Francisco, G. [UNESP]
description The 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.
publishDate 1992
dc.date.none.fl_str_mv 1992-01-01
2022-04-28T19:53:24Z
2022-04-28T19:53:24Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1103/PhysRevD.45.1158
Physical Review D, v. 45, n. 4, p. 1158-1162, 1992.
0556-2821
http://hdl.handle.net/11449/223854
10.1103/PhysRevD.45.1158
2-s2.0-0004365354
url http://dx.doi.org/10.1103/PhysRevD.45.1158
http://hdl.handle.net/11449/223854
identifier_str_mv Physical Review D, v. 45, n. 4, p. 1158-1162, 1992.
0556-2821
10.1103/PhysRevD.45.1158
2-s2.0-0004365354
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Physical Review D
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 1158-1162
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
_version_ 1808129505908228096

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