GALACTIC NONLINEAR DYNAMIC MODEL

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dc.contributor.authorDe Melo, C. A. M. [UNESP]
dc.contributor.authorResende, S. T.
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionUniv Vale Rio Verde
dc.date.accessioned2013-09-30T18:55:14Z
dc.date.accessioned2014-05-20T14:10:14Z
dc.date.available2013-09-30T18:55:14Z
dc.date.available2014-05-20T14:10:14Z
dc.date.issued2009-04-10
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.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.format.extent1669-1673
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.wosWOS:000265092600040
dc.language.isoeng
dc.publisherWorld Scientific Publ Co Pte Ltd
dc.relation.ispartofInternational Journal of Modern Physics A
dc.relation.ispartofjcr1.291
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.subjectGalactic rotation curvesen
dc.subjectdark matteren
dc.subjectmathematical modelingen
dc.titleGALACTIC NONLINEAR DYNAMIC MODELen
dc.typeArtigo
dcterms.licensehttp://www.worldscientific.com/page/authors/author-rights
dcterms.rightsHolderWorld Scientific Publ Co Pte Ltd
unesp.author.orcid0000-0001-5096-1297[1]
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Física Teórica (IFT), São Paulopt

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Artigos - Instituto de Física Teórica (IFT)