dc.creatorLetelier, P
dc.creatorCoimbra-Araujo, CH
dc.date2012
dc.dateAPR
dc.date2014-07-30T17:51:20Z
dc.date2015-11-26T16:40:59Z
dc.date2014-07-30T17:51:20Z
dc.date2015-11-26T16:40:59Z
dc.date.accessioned2018-03-28T23:25:03Z
dc.date.available2018-03-28T23:25:03Z
dc.identifierBrazilian Journal Of Physics. Springer, v. 42, n. 41671, n. 100, n. 109, 2012.
dc.identifier0103-9733
dc.identifierWOS:000305562300013
dc.identifier10.1007/s13538-012-0059-0
dc.identifierhttp://www.repositorio.unicamp.br/jspui/handle/REPOSIP/68447
dc.identifierhttp://repositorio.unicamp.br/jspui/handle/REPOSIP/68447
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1272776
dc.descriptionCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.descriptionAny connection between dark matter and extra dimensions is revealed by the effective energy-momentum tensor associated with the theory. In order to investigate and test such a relationship, we examine a higher-dimensional space-time endowed with a factorizable general metric with a configuration such that its density profile coincides with the Newtonian potential for disk galaxies. An appropriate solution representing stratifications of mass in the central-bulge and disk part of galaxies, e.g., the Miyamoto-Nagai ansatz, is used to solve the Einstein equations. We compute the stable rotation curves of such systems and, with no adjustable parameters, accurately recover the observational data for flat or not asymptotically flat galaxy rotation curves. We present examples of density profiles and compare them to the profile obtained from purely Newtonian potentials.
dc.description42
dc.description41671
dc.description100
dc.description109
dc.descriptionCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.descriptionCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)
dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.descriptionCAPES [3874-07-9]
dc.languageen
dc.publisherSpringer
dc.publisherNew York
dc.publisherEUA
dc.relationBrazilian Journal Of Physics
dc.relationBraz. J. Phys.
dc.rightsfechado
dc.rightshttp://www.springer.com/open+access/authors+rights?SGWID=0-176704-12-683201-0
dc.sourceWeb of Science
dc.subjectGalaxies
dc.subjectMiyamoto-Nagai configurations
dc.subjectDark matter
dc.subjectRotation curves
dc.subjectRotation Curves
dc.subjectSpiral Galaxies
dc.subjectMass
dc.subjectClusters
dc.subjectModels
dc.titleGravity with Extra Dimensions and Dark Matter Interpretation: Phenomenological Example via Miyamoto-Nagai Galaxy
dc.typeArtículos de revistas


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