Accelerated Expansion: Theory & Observations Auteur(s): Polarski D. (Article) Publié: Journal Of Low Temperature Physics, vol. 124 p.17-24 (2001) Texte intégral en Openaccess : Ref Arxiv: astro-ph/0109349 DOI: 10.1023/A:1017509430993 WoS: 000170496900003 Ref. & Cit.: NASA ADS 1 Citation Résumé: The present paradigm in cosmology is the usual Big-Bang Cosmology in which two stages of accelerated expansion are incorporated: the inflationary phase in the very early universe which produces the classical inhomogeneities observed in the universe, and a second stage of acceleration at the present time as the latest Supernovae observations seem to imply. Both stages could be produced by a scalar field and observations will strongly constrain the microscopic lagrangian of any proposed model. |