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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/24275
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dc.contributor.authorDe Melo, C. A. M.-
dc.contributor.authorResende, S. T.-
dc.date.accessioned2013-09-30T18:55:14Z-
dc.date.accessioned2014-05-20T14:10:14Z-
dc.date.accessioned2016-10-25T17:20:53Z-
dc.date.available2013-09-30T18:55:14Z-
dc.date.available2014-05-20T14:10:14Z-
dc.date.available2016-10-25T17:20:53Z-
dc.date.issued2009-04-10-
dc.identifier.citationInternational Journal of Modern Physics A. Singapore: World Scientific Publ Co Pte Ltd, v. 24, n. 8-9, p. 1669-1673, 2009.-
dc.identifier.issn0217-751X-
dc.identifier.urihttp://hdl.handle.net/11449/24275-
dc.identifier.urihttp://acervodigital.unesp.br/handle/11449/24275-
dc.description.abstractWe develop a model for spiral galaxies based on a nonlinear realization of the Newtonian dynamics starting from the momentum and mass conservations in the phase space. The radial solution exhibits a rotation curve in qualitative accordance with the observational data.en
dc.format.extent1669-1673-
dc.language.isoeng-
dc.publisherWorld Scientific Publ Co Pte Ltd-
dc.sourceWeb of Science-
dc.subjectGalactic rotation curvesen
dc.subjectdark matteren
dc.subjectmathematical modelingen
dc.titleGALACTIC NONLINEAR DYNAMIC MODELen
dc.typeoutro-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.contributor.institutionUniv Vale Rio Verde-
dc.description.affiliationSão Paulo State Univ, UNESP, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.description.affiliationUniv Vale Rio Verde, BR-37410000 Tres Coracoes, MG, Brazil-
dc.description.affiliationUnespSão Paulo State Univ, UNESP, Inst Fis Teor, BR-01405900 São Paulo, Brazil-
dc.identifier.wosWOS:000265092600040-
dc.rights.accessRightsAcesso restrito-
dc.relation.ispartofInternational Journal of Modern Physics A-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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