Binding energies: New values and impact on the efficiency of chemical desorption

Q2 Physics and Astronomy
V. Wakelam , J.-C. Loison , R. Mereau , M. Ruaud
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引用次数: 117

Abstract

Recent laboratory measurements have confirmed that chemical desorption (desorption of products due to exothermic surface reactions) can be an efficient process. The impact of including this process into gas-grain chemical models entirely depends on the formalism used and the associated parameters. Among these parameters, binding energies are probably the most uncertain ones for the moment. We propose a new model to compute binding energy of species to water ice surfaces. We have also compared the model results using either the new chemical desorption model proposed by Minissale et al. (2016) or the one of Garrod et al. (2007). The new binding energies have a strong impact on the formation of complex organic molecules. In addition, the new chemical desorption model from Minissale produces a much smaller desorption of these species and also of methanol. Combining the two effects, the abundances of CH3OH and COMs observed in cold cores cannot be reproduced by astrochemical models anymore.

结合能:新的数值及其对化学解吸效率的影响
最近的实验室测量证实,化学解吸(由于放热表面反应的产物的解吸)可以是一个有效的过程。将这一过程纳入气粒化学模型的影响完全取决于所使用的形式和相关参数。在这些参数中,结合能可能是目前最不确定的参数。我们提出了一种计算物质与水冰表面结合能的新模型。我们还使用Minissale等人(2016)提出的新化学解吸模型或Garrod等人(2007)提出的模型结果进行了比较。新的结合能对复杂有机分子的形成有很大的影响。此外,来自Minissale的新化学解吸模型产生了更小的这些物种和甲醇的解吸。结合这两种效应,在冷核中观测到的CH3OH和COMs的丰度不能再用天体化学模型再现。
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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.
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