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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/23391
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dc.contributor.authorDe Lorenci, V. A.-
dc.contributor.authorKlippert, R.-
dc.contributor.authorObukhov, Y. N.-
dc.date.accessioned2014-05-20T14:06:38Z-
dc.date.available2014-05-20T14:06:38Z-
dc.date.issued2003-09-15-
dc.identifierhttp://dx.doi.org/10.1103/PhysRevD.68.061502-
dc.identifier.citationPhysical Review D. College Pk: American Physical Soc, v. 68, n. 6, 4 p., 2003.-
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/11449/23391-
dc.description.abstractWe study the optical paths of the light rays propagating inside a nonlinear moving dielectric medium. For rapidly moving dielectrics we show the existence of a distinguished surface which resembles, as far as the light propagation is concerned, the event horizon of a black hole. Our analysis clarifies the physical conditions under which electromagnetic analogues of gravitational black holes can eventually be obtained in laboratory.en
dc.format.extent4-
dc.language.isoeng-
dc.publisherAmerican Physical Soc-
dc.sourceWeb of Science-
dc.titleOptical black holes in moving dielectricsen
dc.typeoutro-
dc.contributor.institutionUniv Fed Itajuba-
dc.contributor.institutionUniversidade Estadual Paulista (UNESP)-
dc.description.affiliationUniv Fed Itajuba, Inst Ciências, BR-37500903 Itajuba, MG, Brazil-
dc.description.affiliationUniv Estadual Paulista, Inst Fis Teor, BR-01404900 São Paulo, Brazil-
dc.description.affiliationUnespUniv Estadual Paulista, Inst Fis Teor, BR-01404900 São Paulo, Brazil-
dc.identifier.doi10.1103/PhysRevD.68.061502-
dc.identifier.wosWOS:000185830200005-
dc.rights.accessRightsAcesso restrito-
dc.identifier.fileWOS000185830200005.pdf-
dc.relation.ispartofPhysical Review D-
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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