Radiation-Hydrodynamic Simulations of Core-collapse Supernovae with 6 Dimensional Boltzmann Neutrino Transport

Hiroki Nagakura, Shun Furusawa, Hajime Togashi, Kohsuke Sumiyoshi, Shoichi Yamada

研究成果: Conference article

抄録

Core-collapse supernovae (CCSNe) are intrinsically multi-scale, multi-physics and multi-dimensional phenomena. Because of the enormous complexity, the first-principles numerical simulations under realistic input physics are strongly required to uncover the explosion mechanism, predict observational signals (neutrinos, gravitational waves and electromagnetic waves) and prove physical state in extremely hot and dense matter of supernova core. We have tackled the development of multi-dimensional radiation-hydrodynamic code with full Boltzmann neutrino transport and performed several scientific CCSNe simulations in the last few years. In this article, we report the recent progress of our CCSNe numerical simulations with the most up-to-date equation-of-state (EOS) and nuclear weak interactions. We also present preliminary results of non-rotating CCSNe simulations in spatial axisymmetry.

本文言語English
論文番号012003
ジャーナルJournal of Physics: Conference Series
1225
1
DOI
出版ステータスPublished - 2019 6 5
イベント13th International Conference on Numerical Modeling of Space Plasma Flows, ASTRONUM 2018 - Panama City Beach, United States
継続期間: 2018 6 252018 6 29

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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