在地球核心条件下测定铁的电阻
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
概括
研究人员测量了铁
科学领域:
- 地质学
- 星球科学
- 材料科学
背景情况:
- 地球的磁场是由它的液态外核产生的.
- 金属铁的运输特性对于了解核心动力学至关重要,但仍有争议.
- 在极端条件下铁中的电子散射是行星核心特性的关键.
研究的目的:
- 在地球核心条件下实验性地确定铁的电阻.
- 在高压和高温下研究铁中的电子散射机制.
- 改进地球核心热进化和内核年龄的模型.
主要方法:
- 测量铁的电阻.
- 使用激光加热的钻石.
- 达到高温 (高达4,500K) 和高压 (兆巴).
主要成果:
- 测量到的铁电阻低于仅考虑电子-声子散射的模型所预测的.
- 由于高温的和效应,铁电阻的强烈抑制.
- 显示了地球核心的高导热率.
结论:
- 地球的核心可能会迅速冷却,这表明内核年轻 (年龄小于70亿年).
- 内核的诞生可能与13亿年前的古磁场强度增加无关.
- 在核心条件下铁的运输特性对于地力学和热进化模型至关重要.
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