Abstract

The structural, electronic, and mechanical properties of FeH binary compound under 0–300 GPa were investigated by first-principles calculation. It is proved that the FeH is stable under 0–300 GPa using mechanically stable criteria and phonon spectra. Firstly, the electronic properties of Fe–H compounds were studied by density of states and the band structures. FeH shows its metallic properties under extreme pressure. Secondly, the elastic constant, bulk modulus and shear modulus of FeH increase with the increase of pressure, and the values of above physical quantities for Fe–H binary compounds decrease with the higher content of H. In addition, Poisson's ratio revealed its essence of ionic crystal. Thirdly, Vickers hardness(Hv) and Young's modulus(E) of FeH increase with the pressure, and the smaller content of H in Fe–H binary compound implies the bigger Hv and E. Last but not least, the existence of H in Fe might increase the Vp compared with that of pure Fe which is higher than PREM's. Therefore, Fe–H binary compounds might not be a suitable model for Earth's core. There might be some other elements in the earth interior.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.