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首页> 外文期刊>The Journal of Chemical Physics >he photodissociation of oxetane at 193 nm as the reverse of theaterno-Buchi reaction
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he photodissociation of oxetane at 193 nm as the reverse of theaterno-Buchi reaction

机译:193 nm处氧杂环丁烷的光解离是戏剧性布奇反应的逆过程

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We investigated the photodissociation of oxetane (1,3-trimethylene oxide) at 193.3 nm in amolecular-beam apparatus using photofragment-translational spectroscopy and selectivephotoionization. We measured time-of-flight (TOF) spectra and angular anisotropy parameters /3(t)as a function of flight time of products at m/ z =26-30 u utilizing photoionization energies from 9.8to 14.8 eV. The TOF distributions of the products alter greatly with the employed photon energy,whereas their β(t) distributions are insensitive to the photon energy. Dissociation to H_2CO+C_2H_4isthe major channel in the title reaction. Three distinct dissociation paths with branching ratios0.923:0.058:0.019 are responsible for the three features observed in the distribution of kineticenergy released in the channel H_2CO+C_2H_4. The observation ofH_2and H atoms, ~1% inbranching, indicates that products H_2COand C_2H_4spontaneously decompose to only a small extent.Most HCO, C_2H_3, and C_2ions originate from dissociative photoionization of products H_2CO andC_2H_4. Except atomic H andH_2,the photoproducts have large angular anisotropies, β≥-0.8, whichreflects rapid dissociation of oxetane following optical excitation at 193.3 nm. The mechanisms ofdissociation of oxetane are addressed. Our results confirm the quantum-chemical calculations ofPalmer et al. and provide profound insight into the Paterno-Buchi reaction.
机译:我们使用分子碎片-平移光谱法和选择性光电离技术研究了在分子束装置中氧杂环丁烷(1,3-三甲撑氧化物)在193.3 nm处的光解离。我们使用9.8至14.8 eV的光电离能测量了飞行时间(TOF)光谱和角各向异性参数/ 3(t)作为m / z = 26-30 u时产品飞行时间的函数。产物的TOF分布随所采用的光子能量而发生很大变化,而它们的β(t)分布对光子能量不敏感。离解为H_2CO + C_2H_4是标题反应中的主要通道。分支比为0.923:0.058:0.019的三个不同的解离路径是通道H_2CO + C_2H_4释放的动能分布中观察到的三个特征的原因。观察到H_2和H原子的支化程度约为1%,表明产物H_2CO和C_2H_4仅在很小的程度上分解。大多数HCO,C_2H_3和C_2离子源自产物H_2CO和C_2H_4的解离光电离。除原子H和H_2以外,光产物具有较大的角各向异性β≥-0.8,这反映了在193.3 nm处的光激发后氧杂环丁烷快速解离。研究了氧杂环丁烷的离解机理。我们的结果证实了Palmer等人的量子化学计算。并提供对Paterno-Buchi反应的深刻见解。

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