{ "id": "0706.1314", "version": "v1", "published": "2007-06-10T13:59:11.000Z", "updated": "2007-06-10T13:59:11.000Z", "title": "When Did Cosmic Acceleration Start ?", "authors": [ "Alessandro Melchiorri", "Luca Pagano", "Stefania Pandolfi" ], "comment": "5 pages, 2 figures", "journal": "Phys.Rev.D76:041301,2007", "doi": "10.1103/PhysRevD.76.041301", "categories": [ "astro-ph", "gr-qc", "hep-ph" ], "abstract": "A precise determination, and comparison, of the epoch of the onset of cosmic acceleration, at redshift z_acc, and of dark energy domination, at z_eq, provides an interesting measure with which to parameterize dark energy models. By combining several cosmological datasets we place constraints on the redshift and age of cosmological acceleration. For a Lambda-CDM model, we find the constraint z_acc=0.76\\pm0.10 at 95% c.l., occurring 6.7\\pm0.4 Gyrs ago. Allowing a constant equation of state but different from -1 changes the constraints to z_acc=0.81\\pm0.12 (6.9\\pm0.5 Gyrs ago) and z_eq=0.48\\pm0.14(4.9\\pm0.9 Gyrs ago), while dynamical models markedly increase the error on the constraints with z_acc=0.81\\pm0.30 (6.8\\pm1.4 Gyrs ago) and z_eq=0.44\\pm0.20 (4.5\\pm1.0 Gyrs ago). Unified dark energy models as Silent Quartessence yield: z_acc=0.80\\pm0.16 (6.8\\pm0.6 Gyrs ago).", "revisions": [ { "version": "v1", "updated": "2007-06-10T13:59:11.000Z" } ], "analyses": { "subjects": [ "95.36.+x" ], "keywords": [ "cosmic acceleration start", "constraint", "dark energy domination", "parameterize dark energy models", "unified dark energy models" ], "tags": [ "journal article" ], "publication": { "publisher": "APS", "journal": "Physical Review D", "year": 2007, "month": "Aug", "volume": 76, "number": 4, "pages": "041301" }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 752771, "adsabs": "2007PhRvD..76d1301M" } } }