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探寻星际介质中缺失的CHO异构体:一项理论研究

In Quest of the Missing CHO Isomers in the Interstellar Medium: A Theoretical Search.

作者信息

Noriega Lisset, Gonzalez-Ortiz Luis Armando, Ortíz-Chi Filiberto, Ramírez Sandra I, Merino Gabriel

机构信息

Departamento de Física Aplicada, Centro de Investigación y de Estudios Avanzados, Unidad Mérida, km 6 Antigua Carretera a Progreso, Apdo. Postal 73, Cordemex, 97310 Mérida, Yucatán, México.

Conahcyt-Departamento de Física Aplicada, Centro de Investigación y de Estudios Avanzados del Instituto Politécnico Nacional, Mérida 97310, Yucatán, México.

出版信息

J Phys Chem A. 2024 Aug 15;128(32):6757-6762. doi: 10.1021/acs.jpca.4c04102. Epub 2024 Aug 1.

DOI:10.1021/acs.jpca.4c04102
PMID:39087830
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11331521/
Abstract

Ethylene glycol (CHO), the only diol detected in the interstellar medium (ISM), is a key component in the synthesis of prebiotic sugars. Its structural isomer, methoxymethanol, has also been found in the ISM. Our results show that neither ethylene glycol (ethane-1,2-diol) nor methoxymethanol is the most stable isomer. Using high-level computational methods, we identified five isomers: two diols, one hydroxy ether, and two peroxides. The geminal diol 1,1-ethanediol (ethane-1,1-diol) is the most stable isomer, although it has not been detected in the ISM, whereas the two peroxides are less stable than the geminal diol by 60 kcal/mol. This study also provides the rotational constants and dipole moment for each conformer of every CHO isomer.

摘要

乙二醇(CHO)是在星际介质(ISM)中检测到的唯一二醇,是合成益生元糖类的关键成分。其结构异构体甲氧基甲醇也已在星际介质中被发现。我们的结果表明,乙二醇(乙烷 - 1,2 - 二醇)和甲氧基甲醇都不是最稳定的异构体。使用高级计算方法,我们确定了五种异构体:两种二醇、一种羟基醚和两种过氧化物。偕二醇1,1 - 乙烷二醇(乙烷 - 1,1 - 二醇)是最稳定的异构体,尽管它尚未在星际介质中被检测到,而两种过氧化物的稳定性比偕二醇低60千卡/摩尔。这项研究还提供了每种CHO异构体的每个构象体的转动常数和偶极矩。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/db2f1fb09b6f/jp4c04102_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/4c5dc0ed5fc3/jp4c04102_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/72e6137ad7e4/jp4c04102_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/e1ce659ec42a/jp4c04102_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/fe3d7ce8357e/jp4c04102_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/db2f1fb09b6f/jp4c04102_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/4c5dc0ed5fc3/jp4c04102_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/72e6137ad7e4/jp4c04102_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/e1ce659ec42a/jp4c04102_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/fe3d7ce8357e/jp4c04102_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/5bce/11331521/db2f1fb09b6f/jp4c04102_0005.jpg

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