Impact of binary interactions on the diffuse supernova neutrino background

DOI DOI HANDLE HANDLE HANDLE ほか3件をすべて表示 一部だけ表示 被引用文献9件 参考文献121件

この論文をさがす

説明

Binary interactions, especially mass transfer and mergers, can strongly influence the evolution of massive stars and change their final properties and the occurrence of supernovae. Here, we investigate how binary interactions affect predictions of the diffuse flux of neutrinos. By performing stellar population syntheses including prescriptions for binary interactions, we show that the resulting detection rates of the diffuse supernova neutrino background is enhanced by 15%-20% compared to estimates without binary considerations. A source of significant uncertainty arises due to the presently sparse knowledge of the evolution of rapidly rotating carbon-oxygen cores, especially those created as a result of mergers near the white dwarf to core collapse boundary. The enhancement effect may be as small as a few percent if the effects of rotation in postmerger systems are neglected, or as large as 75% if trends are extrapolated. Our estimates serve to highlight that binary effects can be important.

12 pages, 8 figures, matches published version

収録刊行物

  • Physical Review D

    Physical Review D 103 (4), 043003-, 2021-02-02

    American Physical Society (APS)

被引用文献 (9)*注記

もっと見る

参考文献 (121)*注記

もっと見る

関連プロジェクト

もっと見る

問題の指摘

ページトップへ