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Computational thermochemistry of glycolaldehyde

机译:乙醇醛的计算热化学

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We use a variant of the focal point analysis to refine estimates of the relative energies of the four low-energy torsional conformers of glycolaldehyde. The most stable form is the cis-cis structure which enjoys a degree of H-bonding from hydroxyl H to carbonyl O; here dihedral angles τ_1 (O=C-C-O) and τ_2 (C-C-O-H) both are zero. We optimized structures in both CCSD(T)/aug-cc-pVDZ and aug-cc-pVTZ; the structures agree within 0.01 ? for bond lengths and 1.0 degrees for valence angles, but the larger basis brings the rotational constants closer to experimental values. According to our extrapolation of CCSD(T) energies evaluated in basis sets ranging to aug-cc-pVQZ the trans-trans form (180°, 180°) has a relative energy of 12.6 kJ/mol. The trans-gauche conformer (160°, ±75°) is situated at 13.9 kJ/mol and the cis-trans form (0°, 180°) at 18.9 kJ/mol. Values are corrected for zero point vibrational energy by MP2/aug-cc-pVTZ frequencies. Modeling the vibrational spectra is best accomplished by MP2/aug-cc-pVTZ with anharmonic corrections. We compute the Watsonian parameters that define the theoretical vibrational-rotational spectra for the four stable conformers, to assist the search for these species in the interstellar medium. Six transition states are located by G4 and CBS-QB3 methods as well as extrapolation using energies for structures optimized in CCSD(T)/aug-cc-pVDZ structures. We use two isodesmic reactions with two well-established thermochemical computational schemes G4 and CBS-QB3 to estimate energy enthalpy and Gibbs energy of formation as well as the entropy of the gas phase system. Our extrapolated electronic energies of species appearing in the isodesmic reactions produce independent values of thermodynamic quantities consistent with G4 and CBS-QB3.
机译:我们使用焦点分析的一种变体来完善对乙醇醛的四个低能扭转构象异构体的相对能的估计。最稳定的形式是顺式-顺式结构,在羟基H到羰基O上具有一定程度的H键。这里,二面角τ_1(O = C-C-O)和τ_2(C-C-O-H)均为零。我们优化了CCSD(T)/ aug-cc-pVDZ和aug-cc-pVTZ中的结构;结构是否在0.01以内?对于键长,对于键长为1.0度;对于键长,为1.0度,但是更大的基础使旋转常数更接近实验值。根据我们对CCSD(T)能量的推断,以基数范围为aug-cc-pVQZ的形式评估,反式(180°,180°)的相对能量为12.6 kJ / mol。反式-顺式构象(160°,±75°)位于13.9 kJ / mol,顺式-反式(0°,180°)位于18.9 kJ / mol。通过MP2 / aug-cc-pVTZ频率校正零点振动能量的值。振动光谱建模最好通过具有非谐波校正的MP2 / aug-cc-pVTZ来完成。我们计算沃森参数,这些参数定义了四个稳定构象体的理论振动-旋转谱,以协助在星际介质中搜索这些物种。通过G4和CBS-QB3方法以及在CCSD(T)/ aug-cc-pVDZ结构中优化的结构的能量外推法确定了六个过渡态。我们使用具有两个完善的热化学计算方案G4和CBS-QB3的两个等渗反应来估计能量焓和吉布斯形成能以及气相系统的熵。我们在等渗反应中出现的外推物种电子产生与G4和CBS-QB3一致的独立热力学值。

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