Pandey Shobhit, Goldfine Elise A, Sinha Shriya, Zhang Chi, Wenderott Jill K, Kaczmarczyk Lucien, Dabrowiecki Ksawery, Dravid Vinayak P, González Gabriela B, Haile Sossina M
Materials Science and Engineering, Northwestern University, Evanston, IL 60208, USA.
Physics and Astrophysics, DePaul University, Chicago, IL 60614, USA.
Materials (Basel). 2025 May 17;18(10):2340. doi: 10.3390/ma18102340.
A common route for the synthesis of molybdenum nitrides is through the temperature-programmed reaction of molybdenum oxides with NH, or ammonolysis. In this work, the role of precursor phase, gas phase chemistry (impact of HO), and temperature profile on the reaction outcome (700 °C) was examined, which resulted in varying amounts of MoO, HMoO, and the nitride phases-cubic γ (nominally MoN) and hexagonal δ (nominally MoN). The phase fraction of the δ phase increased with precursor in the sequence MoO > MoO > HMoO. Steam in the reaction gas also favored the production of δ over γ, but with too much steam, MoO was obtained in the product. Synthesis conditions for obtaining nearly phase-pure δ were identified: MoO as the precursor, 2% HO in the gas stream, and a moderate heating rate (3 °C/min). In situ X-ray diffraction provided insights into the reaction pathway. Extensive physico-chemical analysis of the δ phase, including synchrotron X-ray and neutron diffraction, electron microscopy, thermogravimetric analysis, X-ray photoelectron spectroscopy, and prompt gamma activation analysis, revealed its stoichiometry to be MoONH, indicating non-trivial oxygen incorporation. The presence of N/O ordering and an impurity phase MoN were also revealed, detectable only by neutron diffraction. Notably, a computationally predicted MoON phase (doi: 10.1103/PhysRevLett.123.236402), of interest due to its potential to display a metal-insulator transition, did not appear under any reaction condition examined.
氮化钼合成的常见途径是通过氧化钼与NH₃的程序升温反应或氨解反应。在这项工作中,研究了前驱体相、气相化学(H₂O的影响)和温度分布对反应结果(700℃)的作用,这导致生成了不同量的MoO₃、H₂MoO₄以及氮化物相——立方γ相(标称MoN)和六方δ相(标称Mo₂N)。δ相的相分数以前驱体按MoO₃ > MoO₂ > H₂MoO₄的顺序增加。反应气体中的蒸汽也有利于生成δ相而非γ相,但蒸汽过多时,产物中会得到MoO₃。确定了获得近纯相δ相的合成条件:以MoO₃作为前驱体,气流中含2%的H₂O,以及适中的升温速率(3℃/min)。原位X射线衍射为反应途径提供了深入了解。对δ相进行了广泛的物理化学分析,包括同步加速器X射线和中子衍射、电子显微镜、热重分析、X射线光电子能谱和瞬发伽马活化分析,结果表明其化学计量比为MoO₀.₉N₀.₉H₀.₂,表明有非平凡的氧掺入。还揭示了N/O有序性和杂质相Mo₄N的存在,只有通过中子衍射才能检测到。值得注意的是,由于其可能显示金属-绝缘体转变而受到关注的一种通过计算预测的MoO₀.₅N相(doi: 10.1103/PhysRevLett.123.236402),在任何研究的反应条件下都未出现。