dc.contributor | Maria Carolina Nemes | |
dc.contributor | Walter F. Wreszinski | |
dc.contributor | Ricardo Schwartz Schor | |
dc.contributor | Ronald Dickman | |
dc.creator | Gustavo Gazzola de Lima | |
dc.date.accessioned | 2019-08-14T08:17:07Z | |
dc.date.accessioned | 2022-10-03T22:17:52Z | |
dc.date.available | 2019-08-14T08:17:07Z | |
dc.date.available | 2022-10-03T22:17:52Z | |
dc.date.created | 2019-08-14T08:17:07Z | |
dc.date.issued | 2009-08-07 | |
dc.identifier | http://hdl.handle.net/1843/ESCZ-7YSJH2 | |
dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/3798526 | |
dc.description.abstract | We 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.publisher | Universidade Federal de Minas Gerais | |
dc.publisher | UFMG | |
dc.rights | Acesso Aberto | |
dc.subject | Teoria de Casimir | |
dc.subject | Energia escura | |
dc.title | Teoria de Casimir para a energia escura revisitada | |
dc.type | Dissertação de Mestrado | |