Why do cosmological perturbations look classical to us? Auteur(s): Kiefer Claus, Polarski D. (Article) Publié: Advanced Science Letters, vol. 2 p.164-173 (2009) Texte intégral en Openaccess : Ref HAL: hal-00398336_v1 Ref Arxiv: 0810.0087 Ref. & Cit.: NASA ADS Exporter : BibTex | endNote Résumé: According to the inflationary scenario of cosmology, all structure in the Universe can be traced back to primordial fluctuations during an accelerated (inflationary) phase of the very early Universe. A conceptual problem arises due to the fact that the primordial fluctuations are quantum, while the standard scenario of structure formation deals with classical fluctuations. In this essay we present a concise summary of the physics describing the quantum-to-classical transition. We first discuss the observational indistinguishability between classical and quantum correlation functions in the closed system approach (pragmatic view). We then present the open system approach with environment-induced decoherence. We finally discuss the question of the fluctuations' entropy for which, in principle, the concrete mechanism leading to decoherence possesses observational relevance. Commentaires: 12 pages, Revtex, invited contribution to a special issue of Advanced Science Letters, final version |