{ "id": "0712.2991", "version": "v1", "published": "2007-12-18T16:23:00.000Z", "updated": "2007-12-18T16:23:00.000Z", "title": "Gravitational Waves From the End of Inflation: Computational Strategies", "authors": [ "Richard Easther", "John T. Giblin Jr", "Eugene A. Lim" ], "comment": "15 pages, 13 figures", "journal": "Phys.Rev.D77:103519,2008", "doi": "10.1103/PhysRevD.77.103519", "categories": [ "astro-ph" ], "abstract": "Parametric resonance or preheating is a plausible mechanism for bringing about the transition between the inflationary phase and a hot, radiation dominated universe. This epoch results in the rapid production of heavy particles far from thermal equilibrium and could source a significant stochastic background of gravitational radiation. Here, we present a numerical algorithm for computing the contemporary power spectrum of gravity waves generated in this post-inflationary phase transition for a large class of scalar-field driven inflationary models. We explicitly calculate this spectrum for both quartic and quadratic models of chaotic inflation, and low-scale hybrid models. In particular, we consider hybrid models with an ``inverted'' potential. These models have a very short and intense period of resonance which is qualitatively different from previous examples studied in this context, but we find that they lead to a similar spectrum of gravitational radiation.", "revisions": [ { "version": "v1", "updated": "2007-12-18T16:23:00.000Z" } ], "analyses": { "subjects": [ "04.30.Db", "98.80.Cq" ], "keywords": [ "gravitational waves", "computational strategies", "scalar-field driven inflationary models", "gravitational radiation", "heavy particles far" ], "tags": [ "journal article" ], "publication": { "publisher": "APS", "journal": "Physical Review D", "year": 2008, "month": "May", "volume": 77, "number": 10, "pages": 103519 }, "note": { "typesetting": "TeX", "pages": 15, "language": "en", "license": "arXiv", "status": "editable", "inspire": 770810, "adsabs": "2008PhRvD..77j3519E" } } }