| Project/Area Number |
23840038
|
|---|
| Research Category |
Grant-in-Aid for Research Activity Start-up
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| Allocation Type | Single-year Grants |
|---|
| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
|
|---|
| Research Institution | Tokyo University of Science |
|---|
Principal Investigator |
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| Project Period (FY) |
2011 – 2012
|
| Project Status |
Completed (Fiscal Year 2012)
|
| Budget Amount *help |
¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
Fiscal Year 2012: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2011: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
|
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| Keywords | 超新星ニュートリノ / 超新星爆発 / 原始中性子星 / 重力崩壊 / ブラックホール |
|---|
| Research Abstract |
In this study, to follow the long term evolution of supernova neutrino spectra for various progenitor stars, we combine the results of neutrino-radiation hydrodynamic simulations for the early phase and quasi-static evolutionary calculations of neutrino diffusion for the late phase. The supernova neutrino data computed in this study are publicly available on the internet.
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