Formation of Iron-Helium Compounds under High Pressure
Haruki Takezawa, Han Hsu, Kei Hirose, Fumiya Sakai, Suyu Fu, Hitoshi, Gomi, Shiro Miwa, and Naoya Sakamoto

TL;DR
This study combines experiments and first-principles calculations to demonstrate the formation and stability of iron-helium compounds under high pressure, suggesting Earth's core may contain primordial helium.
Contribution
It provides new experimental and theoretical evidence for stable iron-helium compounds at high pressures, revealing helium's potential role in Earth's core composition.
Findings
FeHex compounds form at 5-54 GPa and ~1000-2820 K.
FeHex remains stable after pressure release at room temperature.
Helium occupies interstitial sites in FeHex, stable up to 50 GPa.
Abstract
We report the formations of fcc and distorted hcp iron-helium compounds with x in FeHex up to 0.13 and 0.48, respectively, based on experiments at 5-54 GPa and ~1000-2820 K. Upon releasing pressure under room temperature, these fcc and distorted hcp FeHex were still observed by XRD and SIMS measurements. Our first-principles calculations indicate that fcc and hcp FeHex, with helium atoms occupying the tetrahedral and trigonal-planar interstitial sites (instead of the octahedral sites), are dynamically stable throughout 0-50 GPa. These results support that the Earth's core can be a large reservoir of primordial 3He.
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Taxonomy
TopicsNuclear Materials and Properties · Quantum, superfluid, helium dynamics · Fusion materials and technologies
