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超热氧与甲烷笼形冰碰撞中甲醇的形成

Methanol Formation in Hyperthermal Oxygen Collisions with Methane Clathrate Ice.

作者信息

Grayson Robert W, Giapis Konstantinos P, Goddard William A

机构信息

Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, California 91125, United States.

Materials and Process Simulation Center, California Institute of Technology, Pasadena, California 91125, United States.

出版信息

J Phys Chem A. 2024 Nov 28;128(47):10250-10258. doi: 10.1021/acs.jpca.4c06078. Epub 2024 Nov 18.

DOI:10.1021/acs.jpca.4c06078
PMID:39556664
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11613570/
Abstract

The presence of small organic molecules at airless icy bodies may be significant for prebiotic chemistry, yet uncertainties remain about their origin. Here, we consider the role of hyperthermal reactive ions in modifying the organic inventory of ice. We employ molecular dynamics using the ReaxFF formalism to simulate bombardment of carbon-bearing ice by hyperthermal water group molecules (HO, = 0-2) with kinetic energy between 2 and 58 eV. Methanol is the dominant closed-shell organic product for a CH clathrate irradiated at low dose by atomic oxygen. It is produced at yields as high as 10%, primarily by a novel hot-atom reaction mechanism, while radiolysis makes a secondary contribution. At high irradiation doses (≳1.4 × 10 cm), the composition is driven toward greater carbon oxidation states with formaldehyde being favored over methanol production. Other water group impactors are less efficient at inducing chemistry in the ice, and alternate clathrate guest species (CO, CO) are very robust against hydrogenation.

摘要

在无气冰质天体上存在的小分子有机物可能对生命起源前的化学过程具有重要意义,但其起源仍存在不确定性。在此,我们考虑超热反应离子在改变冰的有机成分方面所起的作用。我们采用基于ReaxFF形式的分子动力学方法,模拟超热水基团分子(HO,= 0 - 2)以2至58电子伏特的动能轰击含碳冰的过程。对于由原子氧低剂量辐照的CH笼形水合物,甲醇是主要的闭壳有机产物。它的产率高达10%,主要通过一种新型的热原子反应机制产生,而辐射分解起次要作用。在高辐照剂量(≳1.4×10厘米)下,成分趋向于更高的碳氧化态,此时甲醛的生成比甲醇更受青睐。其他水基团撞击体在引发冰中的化学反应方面效率较低,而替代的笼形水合物客体物种(CO、CO)对氢化作用非常稳定。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/8fe0c0e5751c/jp4c06078_0007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/d20e3c6073e1/jp4c06078_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/b13e81071f06/jp4c06078_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/607aa423e116/jp4c06078_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/8a018b3767bb/jp4c06078_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/9b62ff282e43/jp4c06078_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/bbe28d0a412a/jp4c06078_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/8fe0c0e5751c/jp4c06078_0007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/d20e3c6073e1/jp4c06078_0001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/b13e81071f06/jp4c06078_0002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/607aa423e116/jp4c06078_0003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/8a018b3767bb/jp4c06078_0004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/9b62ff282e43/jp4c06078_0005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/bbe28d0a412a/jp4c06078_0006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/7897/11613570/8fe0c0e5751c/jp4c06078_0007.jpg

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