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The Modeling of Grain Surface Chemistry
Long-fei Chen*1,2, Fang-fang Li1, Qiang Chang3
1.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, Urumqi 830011, China;2.School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, China;3.School of Physics and Optoelectronic Engineering, Shandong University of Technology, Zibo 255000, China
Abstract:
Astrochemistry has made great progress in recent years. Especially the grain surface chemistry played important roles in the explanation of the formation of the interstellar molecules. In this review, we will discuss the progress, including the different numerical methods to simulate the ice mantles in the astrochemical models. We will also introduce the laboratory astrochemical experimental results, and their contributions to the grain surface chemistry in the review.
Key words:  Astrochemistry, Molecules, Surface chemistry, Solid-state
FundProject:
尘埃表面化学理论模拟研究进展
陈龙飞*1,2, 李芳芳1, 常 强3
1.中国科学院新疆天文台,乌鲁木齐 830011;2.中国科学院大学天文与空间科学学院,北京 100049;3.山东理工大学物理与光电工程学院,淄博 255000
摘要:
近年来天体化学在解释星际分子的形成过程中起重要作用的尘埃表面化学取得了长足的发展,本文综述了在天体化学模拟中用到的各种数值计算方法,以及尘埃冰幔的化学模型. 同时也介绍在实验室天体化学方面获得的结果,及其对尘埃表面化学所起到的促进作用.
关键词:  天体化学,星际分子,表面化学,实验室天体化学
DOI:10.1063/1674-0068/cjcp1911205
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