化学学报 ›› 2002, Vol. 60 ›› Issue (11): 1981-1985. 上一篇    下一篇

研究论文

星际尘埃HC_(3-x)NC_x(x=0~3)与HC_(5-x)NC_x(x=0~5)分子的DFT研究

王进;张允武;盛六四   

  1. 中国科学技术大学,合肥(230026)
  • 发布日期:2002-11-15

Study of Interstellar Medium HC_(3-x)NC_x(x = 0~3) and HC_(5-x) NC_x (x = 0~5) by Density Functional Theory

Wang Jin;Zhang Yunwu;Sheng Liusi   

  1. National Synchrotron Radiation Laboratory, University of Science and Technology of China,Hefei(230026)
  • Published:2002-11-15

运用密度泛函理论(DFT)中的B3LYP方法,计算了星际尘埃HC_3N,HC_5N分子 及它们的同分异构体的分子结构、相对稳定性、偶极矩、转动常数等,对于HC_(3- x)NC_x(x = 0~3),HC_3N分子比其它的异构体要稳定,将计算所得的HC_3N, HC_2NC的转动常数B_0与实际的观测值B_0相比较,发现两者能较好地吻合。比较 HC_(5-x)NC_x(x = 0~5)的各同分异构体的总能量,发现HC_5N的相对稳定性最高 ,但它的偶极矩相对较低。将HC_5N的转动常数B_0的理论计算值与实际观测值进行 比较,其相对标准误差仅0.6%。

关键词: 丙炔 P, 腈, 密度泛函理论, 偶极矩

The molecular structures, relative stabilities, dipole moments and rotational constants of HC_3N, HC_5N and their isomers are calculated by B3LYP/6-311++G~(**). In HC_(3-x)NC_x (x = 0~3), HC_3N is found to be the most stable structure. The rotational constants B_0 values of HC_3N and HC_2NC which are obtained from B3LYP/6-311++G~(**) are almost exactly in accordance with the experimental values. In HC_(5-x) NC_x(x = 0~5), HC_5N is found to be more stable than other isomers, but its dipole moment is relatively small. For the rotational constants B_0 of HC_5N, the relative standard deviation between the calculated value and the experimental value is only 0.6%.

Key words: PROPYNE P, NITRILE, density functional theory, dipole moment

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