Structure and Stability of C20H3 Radical

Density functional theory B3LYP with 6-31G∗ basis set has been used to investigate the geometries, rotational constants, dipole moments, energy gaps and vibrational frequencies of nine series of isomers of C20H3 radical. The result shows that the bowl-like structure with C1 symmetry is the most stable structure, in which the three hydrogen atoms locate on the edge carbon atoms, and the two hydrogen atoms are neighbouring and the other one has a two- carbon atom interval to the neighbouring hydrogen. In addition, the relationship between the energy and the position of one hydrogen atom from end to middle on the linear structures of C20H3 radical with two hydrogens atoms located on two ends was obtained, which shows the energy increase monotonously. Furthermore, hydrogenation can relax the strain and make the isomer of C20 more stable.

[1]  Congjie Zhang Structure, stability, and spectra of C9H3, C11H3, and C13H3 radicals. , 2004, The Journal of chemical physics.

[2]  Z. Cao,et al.  Linear and nonlinear feature of electronic excitation energy in carbon chains HC2n+1H and HC2nH , 2004 .

[3]  F. Güthe,et al.  Isomeric structures and visible electronic spectrum of the C7H3 radicals. , 2003, Journal of the American Chemical Society.

[4]  T. Schmidt,et al.  Optical detection of C9H3, C11H3, and C13H3 from a hydrocarbon discharge source , 2003 .

[5]  T. Schmidt,et al.  Methyl Substitution in Hydrocarbon Discharge Chemistry: Diagnosis by Laser Spectroscopy , 2003 .

[6]  Xin Xu,et al.  Geometry optimization of Cn (n=2–30) with genetic algorithm , 2002 .

[7]  A. B. Fialkov,et al.  Large molecules, ions, radicals, and small soot particles in fuel-rich hydrocarbon flames: Part VI: positive ions of aliphatic and aromatic hydrocarbons in a low-pressure premixed flame of n-butane and oxygen , 2001 .

[8]  P. Thaddeus,et al.  Microwave and laser spectroscopy of carbon chains and rings , 2001 .

[9]  F. Güthe,et al.  Electronic spectra of the chains HC2nH (n=8–13) in the gas phase , 2001 .

[10]  Kazuyoshi Tanaka,et al.  Thermodynamic stability in [36-D6h]fullerene , 2000 .

[11]  C. Ball,et al.  Cavity ringdown spectroscopy of the linear carbon chains HC7H, HC9H, HC11H, and HC13H , 2000 .

[12]  E. Herbst,et al.  The Physics and Chemistry of Small Translucent Molecular Clouds. XIII. The Basic Hydrocarbon Chemistry , 2000 .

[13]  T. Henning,et al.  Infrared Spectroscopy of Nano-sized Carbon Grains Produced by Laser Pyrolysis of Acetylene: Analog Materials for Interstellar Grains , 1999 .

[14]  J. Maier,et al.  Electronic Absorption Spectra of the Polyacetylene Chains HC2nH, HC2nH-, and HC2n-1N- (n = 6−12) in Neon Matrixes , 1998 .

[15]  A. Mebel,et al.  Theoretical Study on the Mechanism of the Dissociation of Benzene. The C5H3 + CH3 Product Channel , 1997 .

[16]  K. Kawaguchi,et al.  Pulsed discharge nozzle Fourier transform microwave spectroscopy of the propargyl radical (H2CCCH) , 1997 .

[17]  A. Douglas Origin of diffuse interstellar lines , 1977, Nature.