Toward Radiation-Magnetohydrodynamic Simulations in Core-Collapse Supernovae
arXiv:astro-ph/0511826 · doi:10.1088/1742-6596/31/1/015
Abstract
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.
4 pages, 2 figures, Proceedings of the Third 21COE Symposium : Astrophysics as Interdisciplinary Science, Waseda University, Japan, September 1--3, 2005, to appear in IOP Conference Series
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