抄録
We report a current status of our radiation-magnetohydrodynamic code for the study of core-collapse supernovae. In this contribution, we discuss the accuracy of our newly developed numerical code by presenting the test problem in a static background model. We also present the application to the spherically symmetric core-collapse simulations. Since close comparison with the previously published models is made, we are now applying it for the study of magnetorotational core-collapse supernovae.
本文言語 | English |
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ページ(範囲) | 95-98 |
ページ数 | 4 |
ジャーナル | Journal of Physics: Conference Series |
巻 | 31 |
号 | 1 |
DOI | |
出版ステータス | Published - 2006 3月 22 |
ASJC Scopus subject areas
- 物理学および天文学(全般)