类地行星深层内部Fe3N的磁塌缩和低电导率

IF 2.7 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS American Mineralogist Pub Date : 2024-08-09 DOI:10.2138/am-2023-9251
Y. Zhuang, Jin Liu, Chaojia Lv, Liangxu Xu, Wenli Bi, Qingyang Hu, Dongzhou Zhang, Gaston Garbarino, Shengcai Zhu, Youjun Zhang
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引用次数: 0

摘要

由于地球内部可能存在深层氮库,氮化铁的高压行为引起了人们的极大关注。在此,我们使用多种探针并结合金刚石振荡池技术(包括同步辐射 X 射线衍射、同步辐射莫斯鲍尔光谱和电学测量),研究了高达 62 GPa 和 2100 K 的 Fe3N 的磁性、结构、电学和热学特性。确定的状态方程为:V0/Z = 42.8(1) Å3,K0 = 151.8(1) GPa,K′固定为 4。此外,在高压和高温条件下,Fe3N 表现出意想不到的低导电性和导热性。这一结果表明,深层氮循环可能有助于地球和其他陆地天体深层内部的热演化。
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Magnetic collapse and low conductivity of Fe3N in the deep interiors of Earth-like planets
The high-pressure behavior of iron nitrides has garnered significant attention due to the possibility of deep nitrogen reservoirs within the Earth’s interior. Here, we investigate the magnetic, structural, electrical, and thermal properties of Fe3N up to 62 GPa and 2100 K, using multiple probes coupled with the diamond-anvil cell technique (including synchrotron X-ray diffraction, synchrotron Mössbauer spectroscopy, and electrical measurements). Fe3N undergoes a magnetic phase transformation from the ferromagnetic to paramagnetic state at ~17-20 GPa, 300 K. The equation of state was determined as, V0/Z = 42.8(1) Å3, and K0 = 151.8(1) GPa, with K′ fixed at 4. Additionally, Fe3N exhibits unexpectedly low electrical and thermal conductivity under high-pressure and high-temperature conditions. This result suggests that deep nitrogen cycling may contribute to the thermal evolution of the deep interiors of Earth and other terrestrial bodies.
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来源期刊
American Mineralogist
American Mineralogist 地学-地球化学与地球物理
CiteScore
5.20
自引率
9.70%
发文量
276
审稿时长
1 months
期刊介绍: American Mineralogist: Journal of Earth and Planetary Materials (Am Min), is the flagship journal of the Mineralogical Society of America (MSA), continuously published since 1916. Am Min is home to some of the most important advances in the Earth Sciences. Our mission is a continuance of this heritage: to provide readers with reports on original scientific research, both fundamental and applied, with far reaching implications and far ranging appeal. Topics of interest cover all aspects of planetary evolution, and biological and atmospheric processes mediated by solid-state phenomena. These include, but are not limited to, mineralogy and crystallography, high- and low-temperature geochemistry, petrology, geofluids, bio-geochemistry, bio-mineralogy, synthetic materials of relevance to the Earth and planetary sciences, and breakthroughs in analytical methods of any of the aforementioned.
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