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氢自由基(H*)与过渡金属氮化物的化学相互作用。

Chemical Interaction of Hydrogen Radicals (H*) with Transition Metal Nitrides.

作者信息

Rehman Abdul, van de Kruijs Robbert W E, van den Beld Wesley T E, Sturm Jacobus M, Ackermann Marcelo

机构信息

Industrial Focus Group XUV Optics, MESA+ Institute for Nanotechnology, University of Twente, Drienerlolaan 5, Enschede 7522NB, Netherlands.

出版信息

J Phys Chem C Nanomater Interfaces. 2023 Sep 6;127(36):17770-17780. doi: 10.1021/acs.jpcc.3c04490. eCollection 2023 Sep 14.

Abstract

Transition metal nitrides (TMNs) are reported as protective coatings in reactive hydrogen environments. Although the permeation of H through TMN coatings is well reported, their reducibility in H* environments is less investigated. In this work, we categorize the interaction of H* with ambient exposed TiN, ZrN, HfN, VN, NbN, and TaN thin films at 700 °C into three classes. We find that in TiN and VN samples, H*-induced reduction was limited to the surface (≈ top 2 nm). Significant denitridation was observed in ZrN and HfN samples beneath the surface, along with an increase in the transition metal oxide (TMO) fraction. Denitridation was observed in NbN and TaN samples as well, but the increase in the TMO content was less than for ZrN and HfN. We propose a model in three steps: hydrogenation, formation of volatile species, and diffusion of subsurface atoms to the surface. We show that the interaction of H* with TiN, ZrN, HfN, VN, NbN, and TaN with partially oxidized surfaces can be explained using the preferred hydrogenation pathway (based on the work functions) and the thermodynamic driver for forming volatile species (NH and HO; based on the change in Gibbs free energy).

摘要

过渡金属氮化物(TMNs)被报道为活性氢环境中的保护涂层。尽管氢透过TMN涂层的渗透情况已有充分报道,但它们在氢环境中的可还原性研究较少。在这项工作中,我们将700℃下氢与暴露于环境中的TiN、ZrN、HfN、VN、NbN和TaN薄膜的相互作用分为三类。我们发现,在TiN和VN样品中,氢诱导的还原仅限于表面(约顶部2纳米)。在ZrN和HfN样品的表面下方观察到显著的脱氮现象,同时过渡金属氧化物(TMO)含量增加。在NbN和TaN样品中也观察到了脱氮现象,但TMO含量的增加小于ZrN和HfN。我们提出了一个分三步的模型:氢化、挥发性物种的形成以及次表面原子向表面的扩散。我们表明,氢与具有部分氧化表面的TiN、ZrN、HfN、VN、NbN和TaN的相互作用可以用优先氢化途径(基于功函数)和形成挥发性物种(NH和HO;基于吉布斯自由能变化)的热力学驱动力来解释。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/eef2/10510390/7e4371f1c848/jp3c04490_0002.jpg

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