首页> 外文期刊>Physical chemistry chemical physics: PCCP >State-to-state vacuum ultraviolet photodissociation study of CO2 on the formation of state-correlated CO(X-1 Sigma(+); v) with O(D-1) and O(S-1) photoproducts at 11.95-12.22 eV
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State-to-state vacuum ultraviolet photodissociation study of CO2 on the formation of state-correlated CO(X-1 Sigma(+); v) with O(D-1) and O(S-1) photoproducts at 11.95-12.22 eV

机译:二氧化碳在11.95-12.22 eV上与O(D-1)和O(S-1)光产物形成状态相关的CO(X-1 Sigma(+); v)的状态间真空紫外光解离研究

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摘要

The state-to-state photodissociation of CO2 is investigated in the VUV range of 11.94-12.20 eV by using two independently tunable vacuum ultraviolet (VUV) lasers and the time-sliced velocity-map-imagingphotoion (VMI-PI) method. The spin-allowed CO(X-1 Sigma(+); v = 0-18) + O(D-1) and CO(X-1 Sigma(+); v = 0-9) + O(S-1) photoproduct channels are directly observed from the measurement of time-sliced VMI-PI images of O(D-1) and O(S-1). The total kinetic energy release (TKER) spectra obtained based on these VMI-PI images shows that the observed energetic thresholds for both the O(D-1) and O(S-1) channels are consistent with the thermochemical thresholds. Furthermore, the nascent vibrational distributions of CO(X-1 Sigma(+); v) photoproducts formed in correlation with O(D-1) differ significantly from that produced in correlation with O(S-1), indicating that the dissociation pathways for the O(D-1) and O(S-1) channels are distinctly different. For the O(S-1) channel, CO(X-1 Sigma(+); v) photoproducts are formed mostly in low vibrational states (v = 0-2), whereas for the O(D-1) channel, CO(X-1 Sigma(+); v) photoproducts are found to have significant populations in high vibrationally excited states (v = 10-16). The anisotropy b parameters for the O(D-1) + CO(X-1 Sigma(+); v = 0-18) and O(S-1) + CO(X-1 Sigma(+); v = 0-9) channels have also been determined from the VMI-PI measurements, indicating that CO2 dissociation to form the O(D-1) and O(S-1) channels is faster than the rotational periods of the VUV excited CO2 molecules. We have also calculated the excited singlet potential energy surfaces (PESs) of CO2, which are directly accessible by VUV excitation, at the ab initio quantum multi-reference configuration interaction level of theory. These calculated PESs suggest that the formation of CO(X-1 Sigma(+)) + O(S-1) photoproducts occurs nearly exclusively on the 4(1)A' PES, which is generally repulsive with minor potential energy ripples along the OC-O stretching coordinate. The formation of CO(X-1 Sigma(+)) + O(D-1) photofragments can proceed by non-adiabatic transitions from the 4(1)A' PES to the lower 3(1)A' PES of CO2 via the seam of conical intersections at a near linear OCO configuration, followed by the direct dissociation on the 3(1)A' PES. The theoretical PES calculations are consistent with the experimental observation of prompt CO2 dissociation and high rotational and vibrational excitations for CO(X-1 Sigma(+)) photoproducts.
机译:通过使用两个独立可调的真空紫外(VUV)激光器和时间切片速度图成像光电离(VMI-PI)方法,研究了在11.94-12.20 eV的VUV范围内CO2的状态间光解离。自旋允许的CO(X-1 Sigma(+); v = 0-18)+ O(D-1)和CO(X-1 Sigma(+); v = 0-9)+ O(S-1从O(D-1)和O(S-1)的时间切片VMI-PI图像的测量中直接观察到光产物通道。基于这些VMI-PI图像获得的总动能释放(TKER)光谱显示,对于O(D-1)和O(S-1)通道观察到的高能阈值与热化学阈值一致。此外,与O(D-1)相关形成的CO(X-1 Sigma(+); v)光产物的新生振动分布与与O(S-1)相关产生的光产物显着不同,这表明解离途径O(D-1)和O(S-1)的通道明显不同。对于O(S-1)通道,CO(X-1 Sigma(+); v)的光产物主要在低振动状态下形成(v = 0-2),而对于O(D-1)通道,CO (X-1 Sigma(+); v)在高振动激发态(v = 10-16)中发现有大量光产品。 O(D-1)+ CO(X-1 Sigma(+); v = 0-18)和O(S-1)+ CO(X-1 Sigma(+); v = 0的各向异性b参数-9)通道也已从VMI-PI测量中确定,表明CO2分解形成O(D-1)和O(S-1)通道的速度比VUV激发的CO2分子的旋转周期快。我们还计算了从理论上从头算起的量子多参比配置相互作用水平,可以通过VUV激发直接访问的CO2的激发单重态势能面(PESs)。这些计算得出的PES表明,CO(X-1 Sigma(+))+ O(S-1)光产物的形成几乎完全在4(1)A'PES上发生,通常具有排斥力,并且沿该方向有较小的势能波动OC-O拉伸坐标。 CO(X-1 Sigma(+))+ O(D-1)光片段的形成可以通过从4(1)A'PES到CO2的较低3(1)A'PES的非绝热转变来进行圆锥形相交处的接缝处呈接近线性OCO构型,然后在3(1)A'PES上直接解离。 PES的理论计算与CO(X-1 Sigma(+))光产物迅速CO2分解以及高旋转和振动激发的实验观察结果一致。

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