{ "id": "1502.03898", "version": "v1", "published": "2015-02-13T06:49:42.000Z", "updated": "2015-02-13T06:49:42.000Z", "title": "Binary population synthesis for the core-degenerate scenario of type Ia supernova progenitors", "authors": [ "Weihong Zhou", "Bo Wang", "Xiangcun Meng", "Dongdong Liu", "Gang Zhao" ], "comment": "12 pages, 10 figures, resubmitted to Research in Astronomy and Astrophysics after review by referee", "categories": [ "astro-ph.SR" ], "abstract": "The core-degenerate (CD) scenario has been suggested to be a possible progenitor model of type Ia supernovae (SNe Ia), in which a carbon-oxygen white dwarf (CO WD) merges with the hot CO core of a massive asymptotic giant branch (AGB) star during their common-envelope phase. However, the SN Ia birthrates for this scenario are still uncertain. We conducted a detailed investigation into the CD scenario and then gave the birthrates for this scenario using a detailed Monte Carlo binary population synthesis approach. We found that the delay times of SNe Ia from this scenario are ~70Myrs-1400Myrs, which means that the CD scenario contributes to young SN Ia populations. The Galactic SN Ia birthrates for this scenario are in the range of ~7.4*10^{-5} yr^{-1}-3.7*10^{-4}yr^{-1}, which roughly accounts for ~2-10% of all SNe Ia. This indicates that, under the assumptions made here, the CD scenario only contributes a small portion of all SNe Ia, which is not consistent with the results of Ilkov & Soker (2013).", "revisions": [ { "version": "v1", "updated": "2015-02-13T06:49:42.000Z" } ], "analyses": { "keywords": [ "type ia supernova progenitors", "core-degenerate scenario", "sne ia", "monte carlo binary population", "binary population synthesis approach" ], "publication": { "doi": "10.1088/1674-4527/15/10/007", "journal": "Research in Astronomy and Astrophysics", "year": 2015, "month": "Oct", "volume": 15, "number": 10, "pages": 1701 }, "note": { "typesetting": "TeX", "pages": 12, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1345122, "adsabs": "2015RAA....15.1701Z" } } }