{ "id": "1312.6877", "version": "v2", "published": "2013-12-24T19:28:28.000Z", "updated": "2015-04-20T23:05:11.000Z", "title": "Emergent universe scenario and the low CMB multipoles", "authors": [ "Pedro Labrana" ], "comment": "20 pages, 4 figures, typos corrected, some improvements in sections III and V, and comments added in conclusions. New appendix, references added. Accepted for publication in Phys.Rev.D", "categories": [ "astro-ph.CO", "gr-qc", "hep-th" ], "abstract": "In this work we study superinflation in the context of the emergent universe (EU) scenario. The existence of a superinflating phase before the onset of slow-roll inflation arises in any emergent universe model. We found that the superinflationary period in the EU scenario produces a suppression of the CMB anisotropies at large scale which could be responsible for the observed lack of power at large angular scales of the CMB.", "revisions": [ { "version": "v1", "updated": "2013-12-24T19:28:28.000Z", "title": "Emergent Universe Scenario and the Low CMB Multipoles", "abstract": "In this work we study super inflation in the context of the Emergent Universe (EU) scenario. The existence of a super inflating phase before the onset of slow roll inflation arises in any Emergent Universe model. We found that the super inflationary period in the EU scenario produces a suppression of the CMB anisotropies at large scale which could be responsible of the observed lack of power at large angular scales of the CMB.", "comment": "16 pages, 4 figures", "journal": null, "doi": null }, { "version": "v2", "updated": "2015-04-20T23:05:11.000Z" } ], "analyses": { "subjects": [ "98.80.Cq", "98.70.Vc" ], "keywords": [ "emergent universe scenario", "low cmb multipoles", "large angular scales", "emergent universe model", "slow-roll inflation arises" ], "publication": { "doi": "10.1103/PhysRevD.91.083534" }, "note": { "typesetting": "TeX", "pages": 20, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1273650, "adsabs": "2013arXiv1312.6877L" } } }