天体化学的 Ab initio 计算

Francesca Tonolo, Silvia Alessandrini
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引用次数: 0

摘要

计算化学在许多天体化学研究领域都发挥着重要作用,或者是对实验测量的补充,或者是推导出实验室难以复制的参数。本章介绍了计算光谱学在协助太空新观测方面的作用,其核心内容是以作者在 2023 年 9 月于的里雅斯特举行的 "第二届意大利原(行星)天体化学全国大会 "上发表的论文为指导,研究星际介质气相条件下发生的碰撞辐射转移和双分子反应过程。特别要讨论的是,建立分子丰度模型需要精确的碰撞系数数据集。然后,将介绍量子化学在研究星际相关势能面中的作用,重点是估算速率系数的准确热力学量。
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Ab initio Calculations for Astrochemistry
Computational chemistry plays a relevant role in many astrochemical research fields, either by complementing experimental measurements or by deriving parameters difficult to be reproduced by laboratories. While the role of computational spectroscopy in assisting new observations in space is described, the core of the chapter is the investigation of the collisional radiative transfer and the bimolecular reactive processes occurring in the gas-phase conditions of the interstellar medium, using as a guide the contributions presented by the authors at the "Second Italian National Congress on Proto(-planetary) Astrochemistry", held in Trieste in September 2023. In particular, the need for accurate datasets of collisional coefficients to model molecular abundances will be discussed. Then, the role of quantum chemistry in the investigation of interstellar-relevant potential energy surfaces will be described, focusing on accurate thermodynamic quantities for the estimate of rate coefficients.
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