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首页> 外文期刊>The Journal of Chemical Physics >Vacuum ultraviolet photodissociation dynamics of CO2 near 133 nm: The spin-forbidden O(P-3(j=2,1,0)) + CO(X-1 Sigma(+)) channel
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Vacuum ultraviolet photodissociation dynamics of CO2 near 133 nm: The spin-forbidden O(P-3(j=2,1,0)) + CO(X-1 Sigma(+)) channel

机译:FO2的真空紫外线光积极性动态133 nm:旋转禁止O(P-3(J = 2,1,0))+ CO(x-1 sigma(+))通道

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Understanding vacuum ultraviolet (VUV) photodissociation dynamics of CO2 is of considerable importance in the study of atmospheric chemistry and planetary chemistry. Yet, photodissociation dynamics of the spin-forbidden O(P-3(j=2,1,0)) + CO(X-1 Sigma(+)) channel has not been clearly understood so far. Here, we study the O(P-3(j)) + CO(X-1 Sigma(+)) dissociation processes in the VUV photodissociation of CO2 at the photolysis wavelengths between 129.02 and 134.67 nm by using the time-sliced velocity-mapped ion imaging technique. From the vibrational-resolved images of the O(P-3(j=2,1,0)) photofragment, the total kinetic energy releases, the CO(X-1 Sigma(+)) cofragment vibrational state distributions, and the product angular distributions have been derived, respectively. The experimental observations show that the total kinetic energy releases for the three P-3(j) spin-orbit states (j = 2, 1, 0) exhibit a broad CO(X-1 Sigma(+)) vibrational energy distribution with significant inverted characteristics, especially at short photoexcitation wavelengths, indicating that the VUV photodissociation could take place in a relatively linear geometry of the triplet state, with one C-O bond extended and the other compressed. Furthermore, a notable photolysis wavelength dependent feature has also been found in the product angular distributions of all three spin-orbit channels (j = 2, 1, 0): Only the vibrational-state specific anisotropy parameter beta values at 130.18 nm behave more anisotropic, while all those at other photolysis wavelengths are near the value ss = 0.5 for O(P-3(j=2,1)) channels or beta = 0.25 for the O(P-3(j=0)) channel, with small fluctuations. This anomalous phenomenon suggests that the different nonadiabatic interactions, such as singlet-triplet coupling, may play a key role in the formation of O(P-3(j=2,1,0)) + CO(X-1 Sigma(+)) products, with strong photolysis wavelength dependence. Published under license by AIP Publishing.
机译:了解FO2的真空紫外线(VUV)光度解码动力学在大气化学和行星化学研究中具有重要的重要性。然而,到目前为止,旋转禁止O(P-3(J = 2,1,0))+ CO(x-1 sigma(+))通道的光度划分动态尚未清楚地理解。在此,我们通过使用时切速度在129.02和134.67nm之间的光解波长下,研究O(p-3(j))+ co(x-1 sigma(+))解离过程。映射离子成像技术。从o的振动分辨图像(P-3(J = 2,1,0)),PhotoFragment,总动能释放,CO(X-1 sigma(+))纤巧振动状态分布,以及产品分别是从角度分布推导出来的。实验观察结果表明,三种P-3(J)旋转轨道态(J = 2,1,0)的总动能释放表现出广泛的CO(X-1 Sigma(+))振动能量分布,具有重要倒置特性,尤其是在短透射波长下,表明VUV光解离可以在三重态状态的相对线性几何形状中进行,其中一个CO键延伸,另一个压缩。此外,在所有三个自旋轨道通道的产品角分布(J = 2,1,0)中也发现了一个值得注意的光解波长依赖性特征:仅在130.18nm处的振动状态特异性各向异性参数β值表现出更各向异性,虽然其他光解波长的所有那些都接近O(p-3(j = 2,1))通道的值SS = 0.5(P-3(j = 0))通道,具有小波动。这种异常现象表明,不同的非双重相互作用,例如单次三态偶联,可以在o的形成中发挥关键作用(p-3(j = 2,1,0))+ co(x-1 sigma(+ ))产品,具有强烈的光解波长依赖性。通过AIP发布在许可证下发布。

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