| Project/Area Number |
15H03719
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| Research Category |
Grant-in-Aid for Scientific Research (B)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Solid earth and planetary physics
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| Research Institution | National Astronomical Observatory of Japan |
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Principal Investigator |
Oshino Shoichi 国立天文台, 天文シミュレーションプロジェクト, 特任専門員 (80631655)
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| Co-Investigator(Kenkyū-buntansha) |
岩澤 全規 国立研究開発法人理化学研究所, 計算科学研究機構, 研究員 (10650038)
堀 安範 国立天文台, 光赤外研究部, 特任助教 (40724084)
藤井 通子 東京大学, 大学院理学系研究科(理学部), 准教授 (90722330)
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| Project Period (FY) |
2015-04-01 – 2018-03-31
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| Project Status |
Completed (Fiscal Year 2017)
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| Budget Amount *help |
¥17,680,000 (Direct Cost: ¥13,600,000、Indirect Cost: ¥4,080,000)
Fiscal Year 2017: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2016: ¥7,020,000 (Direct Cost: ¥5,400,000、Indirect Cost: ¥1,620,000)
Fiscal Year 2015: ¥10,010,000 (Direct Cost: ¥7,700,000、Indirect Cost: ¥2,310,000)
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| Keywords | 惑星形成 / 重力多体問題 / ハイパフォーマンスコンピューティング / GPUコンピューティング / GPGPU / 数値シミュレーション / N体計算 / 理論天文学 / 惑星起源・進化 / 天文 |
|---|
| Outline of Final Research Achievements |
The purpose of this research is to develop a new calculation method and to study the planetary formation process by using the largest number of particles and the latest accelerators. By this study, it became possible to calculate the planetary formation of N-body simulations more than 1 million particles for the first time. In the N-body calculation using the large number of particles (10 million particles), the result of earlier growth of the planet has been obtained than ever, and this process will be clarified in detail in the future.
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