dc.contributorMaria Carolina Nemes
dc.contributorWalter F. Wreszinski
dc.contributorRicardo Schwartz Schor
dc.contributorRonald Dickman
dc.creatorGustavo Gazzola de Lima
dc.date.accessioned2019-08-14T08:17:07Z
dc.date.accessioned2022-10-03T22:17:52Z
dc.date.available2019-08-14T08:17:07Z
dc.date.available2022-10-03T22:17:52Z
dc.date.created2019-08-14T08:17:07Z
dc.date.issued2009-08-07
dc.identifierhttp://hdl.handle.net/1843/ESCZ-7YSJH2
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3798526
dc.description.abstractWe assume that Dark Energy" (of a fixed small region of space at the present cosmic time) may be identified with the system consisting of the vacuum and of a few one-particle states of zero momentum of a scalar quantum field of mass u different 0. Under this assumption we show that local quantum field theory yields a corresponding energy momentum tensor of the perfect fuid form, and that a strictly positive energycan be localized only in regions of linear dimension L of the order of the particle Compton wave-length 1/u. Some early conjectured values for the \axion" rest-mass yield an estimate 1:44x10-56+4GeV4 for the dark energy density. In this way, we hope to have "made a case" for revisiting the Casimir theory of dark energy, proposed in 2002 by M. Turner.
dc.publisherUniversidade Federal de Minas Gerais
dc.publisherUFMG
dc.rightsAcesso Aberto
dc.subjectTeoria de Casimir
dc.subjectEnergia escura
dc.titleTeoria de Casimir para a energia escura revisitada
dc.typeDissertação de Mestrado


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