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借助密度泛函理论计算,通过X射线衍射和红外光谱对玻璃形成性近晶液晶进行结构与动力学研究。

Structural and dynamical investigation of glassforming smectogen by X-ray diffraction and infra-red spectroscopy aided by density functional theory calculations.

作者信息

Deptuch Aleksandra, Górska Natalia, Baran Stanisław, Urbańska Magdalena

机构信息

Institute of Nuclear Physics Polish Academy of Sciences, Radzikowskiego 152, PL-31342 Kraków, Poland.

Faculty of Chemistry, Jagiellonian University, Gronostajowa 2, PL-30387 Kraków, Poland.

出版信息

Spectrochim Acta A Mol Biomol Spectrosc. 2025 Apr 5;330:125723. doi: 10.1016/j.saa.2025.125723. Epub 2025 Jan 7.

DOI:10.1016/j.saa.2025.125723
PMID:39809014
Abstract

Molecular arrangement in the chiral smectic phases of the glassforming (S)-4'-(1-methylheptylcarbonyl)biphenyl-4-yl 4-[7-(2,2,3,3,4,4,4-heptafluorobutoxy) heptyl-1-oxy]benzoate is investigated by X-ray diffraction. An increased correlation length of the positional short-range order in the supercooled state agrees with the previous assumption of the hexatic smectic phase. However, the registered X-ray diffraction patterns are not typical for the hexatic phases. Comparison of the smectic layer spacing and optical tilt angle indicates a strongly non-linear shape of molecules, which enables choice of the molecular models obtained by DFT calculations, used subsequently to interpret the infra-red spectra. The presumption of the hexatic smectic F* or I* phase is supported by the splitting of the absorption bands related to the CO stretching in the supercooled state, which is absent in the smectic C* phase above the melting temperature. The glass transition affects the temperature dependence of the smectic layer spacing but only subtly impacts the infra-red spectra. Application of the k-means cluster analysis enables distinction between the infra-red spectra below and above the glass transition temperature, but only for certain spectral ranges.

摘要

通过X射线衍射研究了玻璃形成性(S)-4'-(1-甲基庚基羰基)联苯-4-基 4-[7-(2,2,3,3,4,4,4-七氟丁氧基)庚基-1-氧基]苯甲酸酯在手性近晶相中的分子排列。过冷状态下位置短程有序的关联长度增加,这与之前关于六方近晶相的假设一致。然而,记录的X射线衍射图谱并非六方相的典型图谱。近晶层间距和光学倾斜角的比较表明分子具有强烈的非线性形状,这使得能够选择通过密度泛函理论(DFT)计算获得的分子模型,随后用于解释红外光谱。过冷状态下与CO伸缩相关的吸收带分裂支持了六方近晶F或I相的推测,而在高于熔点温度的近晶C*相中则不存在这种分裂。玻璃化转变影响近晶层间距的温度依赖性,但仅对红外光谱有微妙影响。应用k均值聚类分析能够区分玻璃化转变温度以下和以上的红外光谱,但仅适用于某些光谱范围。

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