The initial phase of cosmological evolution and the formation of structure in the universe

Title:

The initial phase of cosmological evolution and the formation of structure in the universe

Creator:

Gottlöber, S., Haubold, H. J., Mücket, J. P., and Müller, V.

Identifier:

https://cdk.lib.cas.cz/client/handle/uuid:563503b3-d7f6-43bc-996f-a02489d2ae9a
uuid:563503b3-d7f6-43bc-996f-a02489d2ae9a

Subject:

cosmology and structure in the universe

Type:

model:article and TEXT

Format:

bez média and svazek

Description:

A singularity-free inflationary cosmological model driven by a coherent scalar field and/or R^2 terms in the gravitational Lagrangian is presented. The different mechanisms are compared and their observational restrictions are discussed. The dark matter problem and the mode coupling effect connecting the formation of very large structures and population III objects find a natural place in our model.

Language:

Czech

Rights:

http://creativecommons.org/publicdomain/mark/1.0/
policy:public

Coverage:

421-426

Source:

Publications of the Astronomical Institute of the Academy of Sciences of the Czech Republic | 1987 Volume:63-70 | Number:69

Harvested from:

CDK

Metadata only:

false