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.
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页码：421 / +
页数：2
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