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首页> 外文期刊>The Journal of Chemical Physics >Attractive and repulsive interactions among methanol molecules in supercritical state investigated by Raman spectroscopy and perturbed hard-sphere theory
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Attractive and repulsive interactions among methanol molecules in supercritical state investigated by Raman spectroscopy and perturbed hard-sphere theory

机译:拉曼光谱和扰动硬球理论研究超临界状态下甲醇分子之间的吸引和排斥相互作用

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The short-range structure of supercritical methanol(CH_3OH)is investigated by measuring the spontaneous Raman spectra of the C-O stretching mode.The spectra are obtained at a reduced temperature,T_T=T/T_0=1.02(522.9 K),which permits the neat fluid to be studied isothermally as a function of density.As the density increases,the spectral peaks shift toward the lower energy side and the spectra broaden.In the supercritical region,the amount of shifting shows nonlinear density dependence and the width becomes anomalously large.We use the perturbed hard-sphere model to analyze these density dependencies along the vibrational coordinate.The amount of shifting is decomposed into attractive and repulsive components,and the changes in attractive and repulsive energies are evaluated as functions of density and packing fraction,both of which are continuously varied by a factor of 120.Here we show that the shift amount consists principally of the attractive component at all densities,since the attractive energy is about eight times the repulsive energy.The density dependence of the widths is analyzed by calculating homogeneous and inhomogeneous widths as a function of density.The results show that,although vibrational dephasing and density inhomogeneity contribute similarly to the width at low and middle densities,at high density the main contributor turns out to be the vibrational dephasing.We estimate the local density enhancements of supercritical CH_3OH as function of bulk density by two methods.The results of these analyses show common features,and both the estimated local density enhancements of CH_3OH are considerably larger than the local density enhancements of simple fluids,i.e.,those having nonhydrogen bonding.It is revealed that the local density of supercritical CH_3OH is 40%-60%greater than the local densities of the simple fluids.We also estimate the local density fluctuation using the obtained values of attractive shift,inhomogeneous width,and local density.The density fluctuation in the vicinity of a vibrating molecule is compared to the fluctuation of bulk density,which is obtained from the thermodynamic calculation.
机译:通过测量CO拉伸模式的自发拉曼光谱研究了超临界甲醇(CH_3OH)的短程结构。该光谱是在降低的温度T_T = T / T_0 = 1.02(522.9 K)下获得的,可以得到整齐的随着密度的增加,光谱峰向低能侧移动,光谱变宽。在超临界区,位移量显示出非线性的密度依赖性,宽度异常增大。我们使用摄动的硬球模型来分析沿振动坐标的这些密度依赖性。将位移量分解为吸引和排斥的分量,并将吸引和排斥的能量的变化作为密度和堆积分数的函数进行评估,连续变化120倍。在这里,我们表明,偏移量主要是由所有密度下的吸引分量组成,因为无功能量大约是排斥能量的八倍。通过计算均匀和不均匀宽度随密度的变化,分析了宽度的密度依赖性。结果表明,尽管振动移相和密度不均匀性与中低宽度的贡献相似。密度,在高密度时,主要起因是振动相移。我们通过两种方法估算超临界CH_3OH的局部密度随体积密度的变化。这些分析的结果显示出共同的特征,并且两种估算的局部密度增强CH_3OH的总密度比简单流体的局部密度增加(即具有非氢键的那些)大得多。揭示了超临界CH_3OH的局部密度比简单流体的局部密度大40%-60%。利用所获得的吸引位移,不均匀宽度和局部密度值计算局部密度波动。将振动分子附近的密度波动与通过热力学计算获得的堆积密度波动进行比较。

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