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在常压和室温条件下,固态立方氨在玻璃物质中的稳定化。

Stabilisation of solid-state cubic ammonia confined in a glass substance at ambient temperature under atmospheric pressure.

作者信息

Morishita Masao, Miyoshi Hayate, Kawasaki Haruto, Yanagita Hidefumi

机构信息

National Institute of Materials Science (NIMS) (Formerly Department of Chemical Engineering and Materials Science), University of Hyogo Japan

Department of Chemical Engineering and Materials Science, University of Hyogo Japan.

出版信息

RSC Adv. 2024 May 20;14(23):16128-16137. doi: 10.1039/d4ra00229f. eCollection 2024 May 15.

Abstract

Ammonia, a widely available compound, exhibits structural transitions from solid to liquid to gas depending on temperature, pressure, and chemical interactions with adjacent atoms, offering valuable insights into planetary science. It serves as a significant hydrogen storage medium in environmental science, mitigating carbon dioxide emissions from fossil fuels. However, its gaseous form, NH(g), poses health risks, potentially leading to fatalities. The sublimation pressure () of solid cubic ammonia, NH(cr), below 195.5 K is minimal. In this study, we endeavoured to stabilise NH(cr) at room temperature for the first time. Through confinement within a boric acid glass matrix, we successfully synthesised and stabilised cubic crystal NH(cr) with a lattice constant of 0.5165 nm under atmospheric pressure. Thermodynamic simulations affirmed the stabilisation of NH(cr), indicating its quasi-equilibrium state based on the estimated standard Gibbs energy of formation, . Despite these advancements, the extraction of H(g) from NH(cr) within the boric acid glass matrix remains unresolved. The quest for an external matrix with catalytic capabilities to decompose inner NH(cr) into H(g) and N(g) presents a promising avenue for future research. Achieving stability of the low-temperature phase at ambient conditions could significantly propel exploration in this field.

摘要

氨是一种广泛存在的化合物,根据温度、压力以及与相邻原子的化学相互作用,会呈现从固态到液态再到气态的结构转变,这为行星科学提供了有价值的见解。在环境科学中,它是一种重要的储氢介质,可减少化石燃料产生的二氧化碳排放。然而,其气态形式NH(g)会带来健康风险,甚至可能导致死亡。低于195.5 K时,固体立方氨NH(cr)的升华压力极小。在本研究中,我们首次尝试在室温下稳定NH(cr)。通过将其限制在硼酸玻璃基质中,我们在大气压下成功合成并稳定了晶格常数为0.5165 nm的立方晶体NH(cr)。热力学模拟证实了NH(cr)的稳定性,根据估计的标准吉布斯生成能表明其处于准平衡状态。尽管取得了这些进展,但从硼酸玻璃基质中的NH(cr)提取H(g)的问题仍未解决。寻找具有催化能力的外部基质将内部的NH(cr)分解为H(g)和N(g),是未来研究的一个有前景的途径。在环境条件下实现低温相的稳定性可能会显著推动该领域的探索。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/6d74/11103458/8ec2e8ab0f30/d4ra00229f-f1.jpg

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