Are f(R) dark energy models cosmologically viable ? Auteur(s): Amendola L., Polarski D., Tsujikawa S. (Article) Publié: Physical Review Letters, vol. 98 p.131302 (2007) Texte intégral en Openaccess : Ref HAL: in2p3-00115618_v1 PMID 17501182 Ref Arxiv: astro-ph/0603703 DOI: 10.1103/PhysRevLett.98.131302 WoS: 000245331500015 Ref. & Cit.: NASA ADS Exporter : BibTex | endNote 420 Citations Résumé: We show that all f(R) modified gravity theories are conformally identical to models of quintessence in which matter is coupled to dark energy with a large coupling. This strong coupling induces a cosmological evolution radically different from standard cosmology. We find that in all f(R) theories that behave as a power of R at large or small R (which include all those proposed so far in the literature) the scale factor during the matter phase grows as t^{1/2} instead of the standard law t^{2/3}. This behaviour is grossly inconsistent with cosmological observations (e.g. WMAP), thereby ruling out these models even if they pass the supernovae test and can escape the local gravity constraints. Commentaires: 4 pages |