{ "id": "0905.3470", "version": "v4", "published": "2009-05-21T11:43:19.000Z", "updated": "2009-08-09T08:29:27.000Z", "title": "1/R Correction to Gravity in the Early Universe", "authors": [ "Shi Pi", "Tower Wang" ], "comment": "27 pages, 7 figures, even more references added", "categories": [ "astro-ph.CO", "gr-qc", "hep-th" ], "abstract": "To explain the accelerated expansion of late universe, the 1/R correction to Einstein gravity is usually considered, where R is the Ricci scalar. This correction term is generally believed to be negligible in the early universe. However, if the 1/R term is inflaton-dependent, it will dramatically change the story of inflation. The entropy perturbation will naturally appear and drive the evolution of curvature perturbation outside the Hubble horizon. In a large class of models, the entropy perturbation can be made nearly scale-invariant. In Einstein gravity the single-field inflation with a quartic potential has been ruled out by recent observations, but it revives when the 1/R term is turned on. The evolution of non-Gaussianities on large scale are also studied and applied to inflation with 1/R correction. In some specific models, a large non-Gaussianity can be naturally generated outside the horizon.", "revisions": [ { "version": "v4", "updated": "2009-08-09T08:29:27.000Z" } ], "analyses": { "subjects": [ "04.50.Kd", "98.80.Cq" ], "keywords": [ "early universe", "einstein gravity", "entropy perturbation", "curvature perturbation outside", "quartic potential" ], "tags": [ "journal article" ], "publication": { "doi": "10.1103/PhysRevD.80.043503", "journal": "Physical Review D", "year": 2009, "month": "Aug", "volume": 80, "number": 4, "pages": "043503" }, "note": { "typesetting": "TeX", "pages": 27, "language": "en", "license": "arXiv", "status": "editable", "inspire": 821006, "adsabs": "2009PhRvD..80d3503P" } } }