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非能量、低温形成 C-糖基自由基,一种潜在的星际天然氨基酸前体。

Non-energetic, Low-Temperature Formation of C-Glycyl Radical, a Potential Interstellar Precursor of Natural Amino Acids.

机构信息

MTA-ELTE Lendület Laboratory Astrochemistry Research Group, Institute of Chemistry, ELTE Eötvös Loránd University, H-1518 Budapest, Hungary.

Laboratory of Molecular Spectroscopy, Institute of Chemistry, ELTE Eötvös Loránd University, H-1518 Budapest, Hungary.

出版信息

J Phys Chem Lett. 2021 Jul 22;12(28):6744-6751. doi: 10.1021/acs.jpclett.1c01306. Epub 2021 Jul 15.

Abstract

The reaction of H atoms with glycine was investigated at 3.1 K in -H, a quantum-solid host. The reaction was followed by IR spectroscopy, with the spectral analysis aided by quantum chemical computations. Comparison of the experimental IR spectrum with computed anharmonic frequencies and intensities proved that, regardless of the reactant glycine conformation, C-glycyl radical is formed in an H-atom-abstraction process with great selectivity. The product of the second H-atom abstraction, iminoacetic acid, was also observed in a smaller amount. The C-glycyl radical is sensitive to UV light and decomposes to iminoacetic acid and H atom upon 280 nm radiation. Since the reactive radical center is located on the C-atom, it is suggested that natural α-amino acids can be formed from glycine via the C-glycyl radical by non-energetic mechanisms in the solid phase of the interstellar medium.

摘要

在 -H 量子固体基质中,于 3.1 K 下研究了 H 原子与甘氨酸的反应。通过红外光谱法进行了反应跟踪,通过量子化学计算辅助光谱分析。实验红外光谱与计算非谐频率和强度的比较证明,无论反应物甘氨酸构象如何,在 H 原子的夺取过程中,C-甘氨酰基自由基都具有很大的选择性。第二个 H 原子夺取的产物亚氨基乙酸也以较小的量被观察到。C-甘氨酰基自由基对紫外线敏感,在 280nm 辐射下分解为亚氨基乙酸和 H 原子。由于反应性自由基中心位于 C 原子上,因此有人认为,在星际介质固相中,通过 C-甘氨酰基自由基,天然的α-氨基酸可以从甘氨酸非能量机制形成。

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