地球の核条件における鉄の電気抵抗性の実験的決定
Kenji Ohta1, Yasuhiro Kuwayama2, Kei Hirose3,4
1Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo 152-8551, Japan.
Nature
|June 3, 2016
まとめ
研究者は鉄を測定した
科学分野:
- 地理学
- 惑星科学
- 材料科学
背景:
- 地球の磁場は 液体の外核によって生成されます
- 金属鉄の輸送特性は,コアダイナミクスを理解するために不可欠ですが,議論の余地があります.
- 極限条件下での 鉄の電子散乱は 惑星の核の性質の鍵です
研究 の 目的:
- 地球の核条件下での鉄の電気抵抗性を実験的に決定する.
- 鉄の電子散乱メカニズムを高圧と高温で調査する.
- 地球の中核の熱的進化と内核の年齢のモデルを精査する
主な方法:
- 鉄の電気抵抗を測定する
- レーザーで加熱された ダイヤモンド・アンビル・セルを使いました
- 高温 (最大4,500K) と高圧 (メガバー) を達成する.
主要な成果:
- 測定された鉄の抵抗性は,電子-フォノン散乱のみを考慮するモデルによって予測されるよりも低い.
- 高温での飽和効果による鉄抵抗の強い抑制が観察された.
- 地球の核の熱伝導性が高いことが示されています
結論:
- 地球の核は急速に冷却され,若い内核 (<70億年) を示唆している.
- 内核の誕生は 13億年前の 磁場強度の増加と相関しないかもしれません
- 核条件下での鉄の輸送特性は,ジオダイナモと熱進化モデルにとって重要です.
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