Intermolecular interaction in deuterated hydrogen hydrate and its implications for the evolution of planets and protostars
| Project/Area Number |
22740298
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| Research Category |
Grant-in-Aid for Young Scientists (B)
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| Allocation Type | Single-year Grants |
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| Research Field |
Solid earth and planetary physics
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| Research Institution | Ehime University |
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Principal Investigator |
MACHIDA Shinichi 愛媛大学, 地球深部ダイナミクス研究センター, グローバルCOE助教 (30554373)
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| Project Period (FY) |
2010 – 2011
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| Project Status |
Completed (Fiscal Year 2011)
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| Budget Amount *help |
¥4,160,000 (Direct Cost: ¥3,200,000、Indirect Cost: ¥960,000)
Fiscal Year 2011: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
Fiscal Year 2010: ¥2,730,000 (Direct Cost: ¥2,100,000、Indirect Cost: ¥630,000)
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| Keywords | 水素ハイドレート / 高圧実験 / 同位体効果 / 分子間相互作用 / 惑星・原始星 / ダイヤモンドアンビルセル / 回折実験 / 中性子回折実験 / Raman分光 |
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| Research Abstract |
Hydrogen hydrate is solid crystal which is made of water and hydrogen molecules. I performed the high-pressure experiments for hydrogen hydrate, and high-pressure structural changes and their stabilities for hydrogen hydrate were examined. In order to detect the intermolecular interactions separately from the water and hydrogen molecules, the deuterated hydrogen was used for the sample. Recently, this hydrogen hydrate has been expected to play an important role for the reservoir of the hydrogen molecules in planets, their moons and protostar. Thus, the present research is important for the modeling of the formation and evolution of these bodies.
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Report
(3 results)
Research Products
(16 results)
