Multigroup flux-limited diffusion neutrino transport simulations for magnetized and rotating core-collapse supernovae

被引：0

作者：

Kotake, Kei ^{[1
]}

Ohnishi, Naofumi ^{[2
]}

Yamada, Shoichi ^{[3
]}

Sato, Katsuhiko ^{[4
]}

机构：

[1] Waseda Univ, Shinjuku Ku, 3-4-1 Okubo, Tokyo 1698555, Japan

[2] Tohoku Univ, Dept Aerosp Engn, Aoba Ku, Sendai, Miyagi 9808579, Japan

[3] Waseda Univ, Adv Sci & Engn Res Inst, Tokyo 1698555, Japan

[4] Univ Tokyo, Sch Sci, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan

来源：

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES | 2006年 / 847卷

关键词：

supernovae : general-neutrinos-radiative transfer-magnetohydrodynamics-methods : numerical;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 supemovae.

引用

页码：421 / +

页数：2

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