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

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

Research output: Contribution to journalConference article

Abstract

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.

Original languageEnglish
Article number012003
JournalJournal of Physics: Conference Series
Volume1225
Issue number1
DOIs
Publication statusPublished - 2019 Jun 5
Event13th International Conference on Numerical Modeling of Space Plasma Flows, ASTRONUM 2018 - Panama City Beach, United States
Duration: 2018 Jun 252018 Jun 29

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supernovae
neutrinos
hydrodynamics
radiation
simulation
physics
gravitational waves
explosions
electromagnetic radiation
equations of state
symmetry

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Radiation-Hydrodynamic Simulations of Core-collapse Supernovae with 6 Dimensional Boltzmann Neutrino Transport. / Nagakura, Hiroki; Furusawa, Shun; Togashi, Hajime; Sumiyoshi, Kohsuke; Yamada, Shoichi.

In: Journal of Physics: Conference Series, Vol. 1225, No. 1, 012003, 05.06.2019.

Research output: Contribution to journalConference article

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