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.
| Original language | English |
|---|---|
| Title of host publication | AIP Conference Proceedings |
| Pages | 421-423 |
| Number of pages | 3 |
| Volume | 847 |
| DOIs | |
| Publication status | Published - 2006 |
| Event | ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology - Tokyo Duration: 2005 Nov 8 → 2005 Nov 11 |
Other
| Other | ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: International Symposium on Origin of Matter and Evolution of Galaxies 2005: New Horizon of Nuclear Astrophysics and Cosmology |
|---|---|
| City | Tokyo |
| Period | 05/11/8 → 05/11/11 |
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Keywords
- General-neutrinos-radiative transfer-magnetohydrodynamics- methods
- Numerical
- Supernovae
ASJC Scopus subject areas
- Physics and Astronomy(all)
Cite this
Multigroup flux-limited diffusion neutrino transport simulations for magnetized and rotating core-collapse supernovae. / Kotake, Kei; Ohnishi, Naofumi; Yamada, Shoichi; Sato, Katsuhiko.
AIP Conference Proceedings. Vol. 847 2006. p. 421-423.Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
}
TY - GEN
T1 - Multigroup flux-limited diffusion neutrino transport simulations for magnetized and rotating core-collapse supernovae
AU - Kotake, Kei
AU - Ohnishi, Naofumi
AU - Yamada, Shoichi
AU - Sato, Katsuhiko
PY - 2006
Y1 - 2006
N2 - 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.
AB - 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.
KW - General-neutrinos-radiative transfer-magnetohydrodynamics- methods
KW - Numerical
KW - Supernovae
UR - http://www.scopus.com/inward/record.url?scp=33846359228&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=33846359228&partnerID=8YFLogxK
U2 - 10.1063/1.2234445
DO - 10.1063/1.2234445
M3 - Conference contribution
AN - SCOPUS:33846359228
SN - 0735403422
SN - 9780735403420
VL - 847
SP - 421
EP - 423
BT - AIP Conference Proceedings
ER -