A near-equilibrium potential energy hypersurface has been calculated by CEPA-1 for H&NC, a molecule of astrochemical interest. Making use of experimental ground-state rotational constants and ab initio values for the vibration-rotation coupling constants, the equilibrium bond lengths have been deter
A theoretical investigation of HC3NH+
β Scribed by Peter Botschwina
- Publisher
- Elsevier Science
- Year
- 1987
- Tongue
- English
- Weight
- 652 KB
- Volume
- 139
- Category
- Article
- ISSN
- 0009-2614
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β¦ Synopsis
Using a large basis set of 140 contracted GTOs and the SCF and CEPA methods, various spectroscopic properties were calculated for H&NH+, a cation ofconsiderable astrophysicai importance. The origin of the vi band (approximately the NH stretch), which is the most intense stretching vibration of H&NH+, is predicted at 3513 cm-', in excellent agreement with a recent experimental value of 3.5 14.07 cm-'. The calculated equilibrium dipole moment is 1.75 D and the calculated equilibrium rotational constant is 4305 MHz. The theoretical proton affinity for cyanoacetylene is in close agreement with experiment.
π SIMILAR VOLUMES
Near-equilibrium four-dimensional potential energy surfaces (stretching coordinates only) have been calculated for the two lowest electronic states of HC,NC+ (B'II and A 'X). With a large dipole moment of A= -4.33 D and a B0 value of 4949( 10) MHz, the 3 \*l-l state appears to be a suitable candidat
A six-dimensional anharmonic potential and electric-dipole-moment surface have been calculated for H&H+, an ion of interest to combustion processes and astrochemistry, using CEPA-I and a basis set of 102 contracted Gaussian-type orbitals. Vibrational frequencies and IR intensities are calculated var