Nucleosynthesis inside supernova-driven supercritical accretion disks

Shin Ichirou Fujimoto, Kenzo Arai, Ryuichi Matsuba, Masa Aki Hashimoto, Osamu Koike, Shin Mineshige

研究成果: ジャーナルへの寄稿学術誌査読

13 被引用数 (Scopus)

抄録

We have investigated nucleosynthesis in a supercritical accretion disk around a compact object of 1.4 M, using the self-similar solution of an optically thick advection dominated flow. Supercritical accretion is expected to occur in a supernova with fallback material accreting onto a new-born compact object. It has been found that appreciable nuclear reactions take place even for a reasonable value of the viscosity parameter, αvis ≃ 0.01, when the accretion rate ṁ = Ṁc2/(16LEdd) > 105, where LEdd is the Eddington luminosity. If ṁ ≥ 4 × 106, all heavy elements are destroyed to 4He through photodisintegrations at the inner part of the disk. Even 4He is also disintegrated to protons and neutrons near the inner edge when ṁ ≥ 2 × 107. If the fallback matter of the supernova explosion has the composition of a helium-rich layer of the progenitor, a considerable amount of 44Ti could be ejected via a jet from the disk.

本文言語英語
ページ(範囲)509-515
ページ数7
ジャーナルPublications of the Astronomical Society of Japan
53
3
DOI
出版ステータス出版済み - 6月 25 2001

!!!All Science Journal Classification (ASJC) codes

  • 天文学と天体物理学
  • 宇宙惑星科学

フィンガープリント

「Nucleosynthesis inside supernova-driven supercritical accretion disks」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル