{ "id": "astro-ph/0602594", "version": "v2", "published": "2006-02-27T20:17:29.000Z", "updated": "2006-04-08T01:53:27.000Z", "title": "Prospects for direct detection of primordial gravitational waves", "authors": [ "Sirichai Chongchitnan", "George Efstathiou" ], "comment": "11 pages, 3 figures. Minor amendments. Accepted by Phys. Rev. D", "journal": "Phys.Rev. D73 (2006) 083511", "doi": "10.1103/PhysRevD.73.083511", "categories": [ "astro-ph", "hep-th" ], "abstract": "We study the primordial gravitational wave background produced in models of single field inflation. Using the inflationary flow approach, we investigate the amplitude of gravitational wave spectrum in the frequency range 1 mHz - 1 Hz pertinent to future space-based laser interferometers. For models that satisfy the current observational constraint on the tensor-to-scalar ratio, r<0.36, we derive a strict upper bound of omega_{gw}<1.6 x 10^{-15}, independent of the form of the inflationary potential. Applying, in addition, the observational constraints on the spectral index and its running, omega_{gw} is expected to be considerably lower than this bound unless the shape of the potential is finely tuned. We contrast our numerical results with those based on simple power-law extrapolation of the tensor power spectrum from CMB scales. In addition to single field inflation, we summarise a number of other possible cosmological sources of primordial gravitational waves and assess what might be learnt from direct detection experiments such as LISA, Big Bang Observer and beyond.", "revisions": [ { "version": "v2", "updated": "2006-04-08T01:53:27.000Z" } ], "analyses": { "subjects": [ "98.80.Cq" ], "keywords": [ "single field inflation", "primordial gravitational wave background", "big bang observer", "gravitational wave spectrum" ], "tags": [ "journal article" ], "publication": { "publisher": "APS", "journal": "Phys. Rev. D" }, "note": { "typesetting": "TeX", "pages": 11, "language": "en", "license": "arXiv", "status": "editable", "inspire": 711271 } } }