THE ROTO-TORSIONAL SPECTRUM OF GLYCOLALDEHYDE

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2004

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Ohio State University

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Glycolaldehyde is the first interstellar monosaccharide, that has been detected in emission toward the Galactic center source Sgr B2(N). The molecule presents four conformers, three show Cs symmetry (I, II and IV) and one, III, represents a double minimum of C1 symmetry. Two minima I and IV are cis forms whereas II and III are trans-forms. Cis-I is the most stable geometry that stabilizes by the formation of a hydrogen bond between the OH and the C=O carbonyl group. The relative energies of the remaining minima have been determine to be 1278.2cm−1 (II), 1297.2cm−1 (III) and 1865.2cm−1 (IV) using MP4(SDTQ)/cc-pVQZ. The cis-trans transformation is hindered by a barrier of 1895cm−1 and carries out a significative change of the rotational constants. The roto-torsional energies are obtained by solving the roto-torsional Hamiltonian depending on two coordinates. The potential energy surface is calculated from the MP4/cc-pVQZ energies of a grid of 74 conformations. The rotational constants and the distortion centrifugal constants are obtained in the zero point torsional energies of the cis and the trans forms.

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Author Institution: Departamento de Astrofisica Molecular e Infrarroja, Instituto de Estructura de la Materia; Departamento de Quimica, Instituto de Estructura de la Materia; Departamento de Ingenieria Civil, Catedra de Quimica

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