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去质子化苯甲腈的光电子能谱。

Photoelectron spectroscopy of deprotonated benzonitrile.

作者信息

Ashworth Eleanor K, Bull James N

机构信息

School of Chemistry, Norwich Research Park, University of East Anglia, Norwich NR4 7TJ, United Kingdom.

Centre for Photonics and Quantum Science, University of East Anglia, Norwich NR4 7TJ, United Kingdom.

出版信息

J Chem Phys. 2024 Sep 21;161(11). doi: 10.1063/5.0231206.

Abstract

The recent discovery of cyano-substituted aromatic and two-ring polycyclic aromatic hydrocarbon molecules in Taurus Molecular Cloud-1 has prompted questions on how the electronic structure and excited-state dynamics of these molecules are linked with their existence and abundance. Here, we report a photodetachment and frequency- and angle-resolved photoelectron spectroscopy study of jet-cooled para-deprotonated benzonitrile (p-[Bzn-H]-). The adiabatic detachment energy was determined as 1.70 ± 0.01 eV, in good agreement with CCSD(T)/aug-cc-pVTZ calculations. The spectra across the first few electron-volts above threshold are dominated by prompt autodetachment processes associated with excitation of at least five short-lived (tens of femtoseconds) temporary anion shaped resonances since excitation cross sections are several orders of magnitude larger than direct photodetachment cross sections. The photoexcitation vibronic profile is dominated by a ≈640 cm-1 ring deformation mode. [Bzn-H]- lacks a valence-localized excited state situated below the detachment threshold and does not exhibit thermionic emission following excitation of the temporary anion resonances. Thus, [Bzn-H]- is unlikely to be stable in many interstellar environments.

摘要

最近在金牛座分子云-1中发现了氰基取代的芳香族和双环多环芳烃分子,这引发了关于这些分子的电子结构和激发态动力学如何与其存在和丰度相关联的问题。在此,我们报告了对喷射冷却的对去质子化苯甲腈(p-[Bzn-H]-)的光剥离以及频率和角度分辨光电子能谱研究。绝热剥离能确定为1.70±0.01电子伏特,与CCSD(T)/aug-cc-pVTZ计算结果吻合良好。高于阈值的最初几个电子伏特范围内的光谱主要由与至少五个短寿命(几十飞秒)的临时阴离子形状共振激发相关的即时自剥离过程主导,因为激发截面比直接光剥离截面大几个数量级。光激发振动谱主要由约640厘米-1的环变形模式主导。[Bzn-H]-缺乏位于剥离阈值以下的价态局域激发态,并且在临时阴离子共振激发后不表现出热离子发射。因此,[Bzn-H]-在许多星际环境中不太可能稳定。

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