Zasimov Pavel V, Volosatova Anastasia D, Góbi Sándor, Keresztes Barbara, Tyurin Daniil A, Feldman Vladimir I, Tarczay György
MTA-ELTE Lendület Laboratory Astrochemistry Research Group, Institute of Chemistry, ELTE Eötvös Loránd University, P.O. Box 32, H-1518 Budapest, Hungary.
Department of Chemistry, Lomonosov Moscow State University, 119991 Moscow, Russia.
J Chem Phys. 2024 Jan 14;160(2). doi: 10.1063/5.0177189.
The α-hydroxyethyl radical (CH3·CHOH, 2A) is a key intermediate in ethanol biochemistry, combustion, atmospheric chemistry, radiation chemistry, and astrochemistry. Experimental data on the vibrational spectrum of this radical are crucially important for reliable detection and understanding of the chemical dynamics of this species. This study represents the first detailed experimental report on the infrared absorption bands of the α-hydroxyethyl radical complemented by ab initio computations. The radical was generated in solid para-H2 and Xe matrices via the reactions of hydrogen atoms with matrix-isolated ethanol molecules and radiolysis of isolated ethanol molecules with x rays. The absorption bands with maxima at 3654.6, 3052.1, 1425.7, 1247.9, 1195.6 (1177.4), and 1048.4 cm-1, observed in para-H2 matrices appearing upon the H· atom reaction, were attributed to the OHstr, α-CHstr, CCstr, COstr + CCObend, COstr, and CCstr + CCObend vibrational modes of the CH3·CHOH radical, respectively. The absorption bands with the positions slightly red-shifted from those observed in para-H2 were detected in both the irradiated and post-irradiation annealed Xe matrices containing C2H5OH. The results of the experiments with the isotopically substituted ethanol molecules (CH3CD2OH and CD3CD2OH) and the quantum-chemical computations at the UCCSD(T)/L2a_3 level support the assignment. The photolysis with ultraviolet light (240-300 nm) results in the decay of the α-hydroxyethyl radical, yielding acetaldehyde and its isomer, vinyl alcohol. A comparison of the experimental and theoretical results suggests that the radical adopts the thermodynamically more stable anti-conformation in both matrices.
α-羟乙基自由基(CH3·CHOH,2A)是乙醇生物化学、燃烧、大气化学、辐射化学和天体化学中的关键中间体。该自由基振动光谱的实验数据对于可靠检测和理解该物种的化学动力学至关重要。本研究首次详细报道了α-羟乙基自由基的红外吸收带,并辅以从头算计算。该自由基通过氢原子与基质隔离的乙醇分子反应以及用X射线对隔离的乙醇分子进行辐射分解,在固态对-氢和氙基质中产生。在对-氢基质中,氢原子反应后出现的最大吸收带出现在3654.6、3052.1、1425.7、1247.9、1195.6(1177.4)和1048.4 cm-1处,分别归因于CH3·CHOH自由基的OH伸缩振动、α-CH伸缩振动、C-C伸缩振动、C=O伸缩振动+C-C弯曲振动、C=O伸缩振动以及C-C伸缩振动+C-C弯曲振动模式。在含有C2H5OH的辐照和辐照后退火的氙基质中,检测到吸收带的位置相对于在对-氢中观察到的位置略有红移。用同位素取代的乙醇分子(CH3CD2OH和CD3CD2OH)进行的实验结果以及在UCCSD(T)/L2a_3水平上的量子化学计算支持了这种归属。用紫外光(240 - 300 nm)进行光解会导致α-羟乙基自由基衰变,生成乙醛及其异构体乙烯醇。实验和理论结果的比较表明,该自由基在两种基质中均采用热力学上更稳定的反式构象。