| Budget Amount *help |
¥4,680,000 (Direct Cost: ¥3,600,000、Indirect Cost: ¥1,080,000)
Fiscal Year 2019: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2018: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2017: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2016: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2015: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
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| Outline of Final Research Achievements |
Core-collapse supernovae are the explosive phenomena at the end of life of massive stars. In order to clarify the mechanism of explosion, which has been elusive in nuclear astrophysics for decades, it is essential to solve the neutrino-radiation hydrodynamics at extreme conditions. In this research project, we enabled the first-principle calculations of neutrino transfer by our new method for the first time in the world, successfully performed numerical simulations of multi-dimensional explosions through neutrino heating, and clarified the influence of neutrino and nuclear physics.
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