As we know, there are three structures-sⅠ, sⅡ, and sH, with hydrocarbonate gas hydrate.Because of those special structures characteristics and potentail large fossil energy resource, gas hydrate play an important ro...As we know, there are three structures-sⅠ, sⅡ, and sH, with hydrocarbonate gas hydrate.Because of those special structures characteristics and potentail large fossil energy resource, gas hydrate play an important role in natural carbonate cycle system. In this paper, CH4, CO2, C3H8, and CH4 +CO2 system have been experimental performed in order to model hydrate formation and discomposition and to obtain hydrate stability conditions of tempreature and pressure. The results from laboratory using Raman spectra show that Raman spectrascopy is a effective tool to identify hydrate structure. Raman spectra of clathrate hydrate guest molecules are presented for two structure (sⅠ and sⅡ) in the following systems: CH4, CO2, C3 H8. Relatively occupancy of CH4 in the large and small cavities of sⅠ were determined by deconvoluting the v1 symmetric bands, resulting in hydration numbers of 6.04±0.03. The freqyuency of the v1 bands for CH4 in structures Ⅰ and Ⅱ differ statistically. The large cavities were measured to be almost fully occupied by CH4 and CO2, whereas only a small fraction of the small cavities are occupied by CH4. No CO2 was found in the small cavities.展开更多
基于密度泛函理论(Density functional theory,DFT),M06-2X/6-311G(d,p)基组水平下对加替沙星分子的初始结构进行优化.计算其振动频率,采用VEDA4软件基于势能分布(Potential energy distribution,PED)计算结果对特征振动模式进行了归属...基于密度泛函理论(Density functional theory,DFT),M06-2X/6-311G(d,p)基组水平下对加替沙星分子的初始结构进行优化.计算其振动频率,采用VEDA4软件基于势能分布(Potential energy distribution,PED)计算结果对特征振动模式进行了归属指认,并和实验光谱进行了对比.绘制了分子表面静电势,分析分子可能发生亲电和亲核反应的位点.利用含时密度泛函理论(Time-dependent density functional theory,TDDFT)计算了加替沙星分子的激发态,讨论了加替沙星分子内的电子跃迁.该研究为分析加替沙星的光谱和电子结构提供了理论基础.展开更多
基金Supported by the National Natural Science Foundation of China (No. 49973024, 40272066)211 Projects of Xiamen University.
文摘As we know, there are three structures-sⅠ, sⅡ, and sH, with hydrocarbonate gas hydrate.Because of those special structures characteristics and potentail large fossil energy resource, gas hydrate play an important role in natural carbonate cycle system. In this paper, CH4, CO2, C3H8, and CH4 +CO2 system have been experimental performed in order to model hydrate formation and discomposition and to obtain hydrate stability conditions of tempreature and pressure. The results from laboratory using Raman spectra show that Raman spectrascopy is a effective tool to identify hydrate structure. Raman spectra of clathrate hydrate guest molecules are presented for two structure (sⅠ and sⅡ) in the following systems: CH4, CO2, C3 H8. Relatively occupancy of CH4 in the large and small cavities of sⅠ were determined by deconvoluting the v1 symmetric bands, resulting in hydration numbers of 6.04±0.03. The freqyuency of the v1 bands for CH4 in structures Ⅰ and Ⅱ differ statistically. The large cavities were measured to be almost fully occupied by CH4 and CO2, whereas only a small fraction of the small cavities are occupied by CH4. No CO2 was found in the small cavities.
文摘基于密度泛函理论(Density functional theory,DFT),M06-2X/6-311G(d,p)基组水平下对加替沙星分子的初始结构进行优化.计算其振动频率,采用VEDA4软件基于势能分布(Potential energy distribution,PED)计算结果对特征振动模式进行了归属指认,并和实验光谱进行了对比.绘制了分子表面静电势,分析分子可能发生亲电和亲核反应的位点.利用含时密度泛函理论(Time-dependent density functional theory,TDDFT)计算了加替沙星分子的激发态,讨论了加替沙星分子内的电子跃迁.该研究为分析加替沙星的光谱和电子结构提供了理论基础.
