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多氧化氢的理论表征:HOOH、HOOOOH、HOOOOOH和HOOO。

Theoretical characterization of hydrogen polyoxides: HOOH, HOOOH, HOOOOH, and HOOO.

作者信息

Denis Pablo A, Ornellas Fernando R

机构信息

Computational Nanotechnology, DETEMA, Facultad de Química, UDELAR, Montevideo, Uruguay.

出版信息

J Phys Chem A. 2009 Jan 15;113(2):499-506. doi: 10.1021/jp808795e.

Abstract

We have investigated the polyoxides HOOH, HOOOH, HOOOOH, and HOOO employing the CCSD(T) methodology, and the correlation consistent basis sets. For all molecules, we have computed fundamental vibrational frequencies, structural parameters, rotational constants, and rotation-vibration corrections. For HOOOH, we have obtained a good agreement between our results and microwave and infrared spectra measurements, although for the symmetric OO stretch some important differences were found. Heats of formation were computed using atomization energies, and our recommendation is as follows: DeltaH(o)(f,298)(HOOOH) = -21.50 kcal/mol and DeltaH(o)(f,298)(HOOOOH) = -10.61 kcal/mol. In the case of HOOO, to estimate the heat of formation, we have constructed three isodesmic reactions to cancel high order correlation effects. The results obtained confirmed that the latter effects are very important for HOOO. The new DeltaH(o)(f,298)(HOOO) obtained is 5.5 kcal/mol. We have also calculated the zero-point energies of DO and DOOO to correct the experimental lower limit determined for the DeltaH(o)(f,298)(HOOO). The Delta(DeltaZPE) decreases the binding energy of HOOO by 0.56 kcal/mol. Employing the latter value, the new experimental lower limit for DeltaH(o)(f,298)(HOOO) is 3.07 kcal/mol, just 2.4 kcal/mol lower than our determination. We expect that the fundamental vibrational frequencies and rotational constants determined for HOOOOH and DOOOOD contribute to its identification in the gas phase. The vibrational spectrum of HOOOOH shows some overlapping with that of HOOOH thus indicating that one may encounter some difficulties in its characterization. We discuss the consequences of the thermochemical properties determined in this work, and suggest that the amount of HOOO present in the atmosphere is smaller than that proposed recently in this journal ( J. Phys. Chem A 2007, 111, 4727).

摘要

我们采用CCSD(T)方法和相关一致基组对多氧化物HOOH、HOOOH、HOOOOH和HOOO进行了研究。对于所有分子,我们计算了基本振动频率、结构参数、转动常数以及转动 - 振动校正。对于HOOOH,我们的结果与微波和红外光谱测量结果取得了良好的一致性,不过在对称OO伸缩振动方面发现了一些重要差异。使用原子化能计算了生成热,我们的推荐值如下:ΔH⁰(f,298)(HOOOH) = -21.50千卡/摩尔,ΔH⁰(f,298)(HOOOOH) = -10.61千卡/摩尔。对于HOOO,为了估算生成热,我们构建了三个等键反应以消除高阶相关效应。所得结果证实后一种效应对于HOOO非常重要。新得到的ΔH⁰(f,298)(HOOO)为5.5千卡/摩尔。我们还计算了DO和DOOO的零点能,以校正为ΔH⁰(f,298)(HOOO)确定的实验下限。Δ(ΔZPE)使HOOO的结合能降低了0.56千卡/摩尔。采用后一个值,ΔH⁰(f,298)(HOOO)的新实验下限为3.07千卡/摩尔,仅比我们的测定值低2.4千卡/摩尔。我们预计为HOOOOH和DOOOOD确定的基本振动频率和转动常数将有助于其在气相中的识别。HOOOOH的振动光谱与HOOOH的有一些重叠,这表明在其表征中可能会遇到一些困难。我们讨论了这项工作中确定的热化学性质的影响,并表明大气中HOOO的含量比本期刊最近提出的量(《物理化学杂志A》2007年,111卷,4727页)要少。

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