Effect of Cage Occupancies on Molecular Vibrations of Methane in Structure H Clathrate Hydrate: Ab Initio Molecular Dynamics Simulation

IF 2.8 2区 化学 Q3 CHEMISTRY, PHYSICAL The Journal of Physical Chemistry B Pub Date : 2024-06-04 DOI:10.1021/acs.jpcb.4c01790
Ken Yoshida*, Shinnosuke Suhara and Naoki Noguchi*, 
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Abstract

The structure H (sH) of methane hydrate, which has a distinctive structure with large (LL) cages capable of encapsulating multiple methane molecules, has been suggested as a methane reservoir in large icy bodies such as Titan, making it important in planetary science. This high-pressure phase, which exists in the GPa range, lends itself to the study of methane states and dynamics using powerful experimental techniques such as IR and Raman spectroscopy. However, the interpretation of the vibrational spectra of methane in the sH structure has been challenging because of the spectral complexities. The signals attributed to the methane molecules in the LL cage, as well as those of the other two cage types, overlap in the spectra. In this study, we investigated the microscopic origins of the shape of the C–H stretching vibration spectrum of methane in the LL cage using ab initio molecular dynamics (AIMD) simulations. For a single methane molecule in the LL cage, the ν3 band of the C–H stretching mode was observed at a higher frequency typical of isolated molecules in vacuum due to the large size of the LL cage. As the number of methane molecules in the LL cage increased beyond one, a tendency to blue-shift with increasing methane occupancy was observed, consistent with a loose-cage–tight-cage model. By characterizing the time correlation function of methane stretching vibrations based on the solvation number of methane and water molecules proximal to methane within the LL cage, we showed that the complicated spectral line shape observed in cases of higher methane occupancy in the LL cage resulted from the wider variation of the solvation shell states. Analysis of the solvation structures of the AIMD trajectories provided interpretations of the experimental spectral line shape, demonstrating the complementary nature of AIMD to the experiment and its effectiveness in analysis.

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H 型水合物结构中笼子占位对甲烷分子振动的影响:Ab Initio 分子动力学模拟。
甲烷水合物的结构 H(sH)具有独特的大笼子(LL)结构,能够封装多个甲烷分子,被认为是土卫六等大型冰体中的甲烷储层,因此在行星科学中具有重要意义。这种存在于 GPa 范围内的高压相适合利用红外和拉曼光谱等强大的实验技术来研究甲烷的状态和动力学。然而,由于光谱的复杂性,解释 sH 结构中甲烷的振动光谱一直是一项挑战。归因于 LL 笼中甲烷分子以及其他两种笼型的信号在光谱中重叠。在本研究中,我们利用 ab initio 分子动力学(AIMD)模拟研究了 LL 笼中甲烷 C-H 伸展振动光谱形状的微观起源。对于 LL 笼中的单个甲烷分子,由于 LL 笼的尺寸较大,C-H 拉伸模式的 ν3 频带被观测到,其频率较高,是真空中孤立分子的典型频率。当 LL 笼中的甲烷分子数增加到一个以上时,观察到随着甲烷占有率的增加而蓝移的趋势,这与松笼-紧笼模型相一致。通过根据 LL 笼中甲烷和甲烷近旁水分子的溶解数来表征甲烷伸缩振动的时间相关函数,我们发现在 LL 笼中甲烷占有率较高的情况下观察到的复杂谱线形状是由较宽的溶解壳状态变化造成的。对 AIMD 轨迹的溶解结构分析为实验光谱线形提供了解释,证明了 AIMD 与实验的互补性及其分析的有效性。
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来源期刊
CiteScore
5.80
自引率
9.10%
发文量
965
审稿时长
1.6 months
期刊介绍: An essential criterion for acceptance of research articles in the journal is that they provide new physical insight. Please refer to the New Physical Insights virtual issue on what constitutes new physical insight. Manuscripts that are essentially reporting data or applications of data are, in general, not suitable for publication in JPC B.
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