{ "id": "1404.3467", "version": "v2", "published": "2014-04-14T06:28:15.000Z", "updated": "2014-05-02T06:18:12.000Z", "title": "Constraints on the extensions to the base $Λ$CDM model from BICEP2, Planck and WMAP", "authors": [ "Cheng Cheng", "Qing-Guo Huang", "Wen Zhao" ], "comment": "6 pages, 3 figures; minor revised and refs added", "journal": "Sci China-Phys Mech Astron, 57(8), 1460 (2014)", "categories": [ "astro-ph.CO", "gr-qc", "hep-ph", "hep-th" ], "abstract": "Recently Background Imaging of Cosmic Extragalactic Polarization (B2) discovered the relic gravitational waves at $7.0\\sigma$ confidence level. However, the other cosmic microwave background (CMB) data, for example Planck data released in 2013 (P13), prefer a much smaller amplitude of the primordial gravitational waves spectrum if a power-law spectrum of adiabatic scalar perturbations is assumed in the six-parameter $\\Lambda$CDM cosmology. In this paper, we explore whether the $w$CDM model and the running spectral index can relax the tension between B2 and other CMB data. In particular, we find that a positive running of running of spectral index is preferred at $1.7\\sigma$ level from the combination of B2, P13 and WMAP Polarization data.", "revisions": [ { "version": "v2", "updated": "2014-05-02T06:18:12.000Z" } ], "analyses": { "keywords": [ "cdm model", "constraints", "spectral index", "extensions", "primordial gravitational waves spectrum" ], "tags": [ "journal article" ], "publication": { "doi": "10.1007/s11433-014-5514-1", "journal": "Science China Physics, Mechanics, and Astronomy", "year": 2014, "month": "Aug", "volume": 57, "number": 8, "pages": 1460 }, "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1290303, "adsabs": "2014SCPMA..57.1460C" } } }