Toward Radiation-Magnetohydrodynamic Simulations in Core-Collapse Supernovae

Details Toward Radiation-Magnetohydrodynamic Simulations in Core-Collapse Supernovae Toward Radiation-Magnetohydrodynamic Simulations in Core-Collapse Supernovae

2005-11-30

arxiv.org/abs/astro-ph/0511826v1

J.Phys.Conf.Ser.31:95-98,2006

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, Proceedings of the Third 21COE Symposium : Astrophysics as Interdisciplinary Science, Waseda University, J

Scientific paper

10.1088/1742-6596/31/1/015

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.

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