Hydrogenation reactions and adsorption : From CO to methanol on a graphene surface

Q2 Physics and Astronomy Molecular Astrophysics Pub Date : 2019-03-01 DOI:10.1016/j.molap.2019.02.001
Sabine Morisset, Nathalie Rougeau, Dominique Teillet-Billy
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引用次数: 5

Abstract

Successive hydrogenation reactions of isolated CO molecules adsorbed on a bare graphene surface have been studied by density functional theory using a van der Waals functional. Three hydrogenation scenarios, leading to the formation of methanol via the intermediate species: HCO, H2CO, HCOH, H3CO and H2COH, have been considered. Hydrogenation and adsorption energies on the surface have been calculated for all the species. The fractions of molecules released in the gas phase after formation on the surface have been calculated with two different chemical desorption models. Our results show that the fraction of methanol molecules released in the gas phase is low ( < 6%) whatever the scenario. Conversely, the highest fractions of molecules released in the gas phase have been obtained for formaldehyde, H2CO, and the hydroxymethyl radical, H2COH. The methoxy radical, H3CO, is characterized by a high adsorption energy on the substrate (−0.337 eV).

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氢化反应和吸附:从一氧化碳到甲醇在石墨烯表面
利用范德华泛函的密度泛函理论研究了吸附在裸露石墨烯表面的CO分子的连续加氢反应。研究了通过中间物质HCO、H2CO、HCOH、H3CO和H2COH生成甲醇的三种加氢情形。计算了所有物质的表面加氢能和吸附能。用两种不同的化学解吸模型计算了分子在表面形成后在气相中释放的分数。我们的结果表明,无论在何种情况下,在气相中释放的甲醇分子的比例都很低( < 6%)。相反,甲醛、H2CO和羟甲基自由基H2COH在气相中释放的分子分数最高。甲氧基自由基H3CO在底物上具有较高的吸附能(−0.337 eV)。
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来源期刊
Molecular Astrophysics
Molecular Astrophysics ASTRONOMY & ASTROPHYSICS-
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期刊介绍: Molecular Astrophysics is a peer-reviewed journal containing full research articles, selected review articles, and thematic issues. Molecular Astrophysics is a new journal where researchers working in planetary and exoplanetary science, astrochemistry, astrobiology, spectroscopy, physical chemistry and chemical physics can meet and exchange their ideas. Understanding the origin and evolution of interstellar and circumstellar molecules is key to understanding the Universe around us and our place in it and has become a fundamental goal of modern astrophysics. Molecular Astrophysics aims to provide a platform for scientists studying the chemical processes that form and dissociate molecules, and control chemical abundances in the universe, particularly in Solar System objects including planets, moons, and comets, in the atmospheres of exoplanets, as well as in regions of star and planet formation in the interstellar medium of galaxies. Observational studies of the molecular universe are driven by a range of new space missions and large-scale scale observatories opening up. With the Spitzer Space Telescope, the Herschel Space Observatory, the Atacama Large Millimeter/submillimeter Array (ALMA), NASA''s Kepler mission, the Rosetta mission, and more major future facilities such as NASA''s James Webb Space Telescope and various missions to Mars, the journal taps into the expected new insights and the need to bring the various communities together on one platform. The journal aims to cover observational, laboratory as well as computational results in the galactic, extragalactic and intergalactic areas of our universe.
期刊最新文献
Chemistry on Interstellar Grain Surfaces Molecular Emission and Absorption Gas Phase Chemical Processes Diffuse Clouds Molecular Spectroscopy
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