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Nota de FísicaPublicado

Geometrized Instantons and the Creation of the Universe

M. Novello; L. A. R. Oliveira; J. M. Salim; E. Elbaz

1991

Dados da publicação

Autores
M. Novello; L. A. R. Oliveira; J. M. Salim; E. Elbaz
Tipo
Nota de Física
Status
Publicado
Data de publicação
1991
Descrição
A non-singular cosmological scenario is presented in which currently observed Riemannian configuration of space-time originates from a primordial Weylian "stiff matter" phase driven by a geometrized inflaton-like field. In the particular case of a Friedman-Robertson-Walker line element, it is shown that an unstable original Minkowski vacuum starts to collapse adiabatically at a remote past and bounces when a minimum radius is attained. Throughout the collapsing stage this matter-free Universe is accelerated (or "inflationary") As in models of spontaneous quantum creation, the bouncing phase can be shown to correspond to the propagation of a Weyl instanton in an Euclideanized, classically forbidden region. In the course of the bouncing period, concurrent to the maximal deviation of the Riemannian configuration, a geometry-driven amplification mechanism operates causing the exponential increase of entropy and matter fluctuations. Once the environment temperature is always bounded, this non-adiabatical process stands for a "Big - but finite - Bang" creation event, followed by a standard radiation-dominated era. The model describes an eternal, Friedman-like open Universe, free of many problems that hinder standard cosmology; the observed existence of a baryon excess also naturally within the proposed scheme.
Ano
1991
Número
CBPF-NF-049/91
Vínculo com tese
Não
Vínculo com bolsa
Não
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