2-氰噻吩和3-氰噻吩的超精细结构:量子化学研究

Q2 Physics and Astronomy
René Simbizi , Godefroid Gahungu , Minh Tho Nguyen
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引用次数: 0

摘要

文献中没有足够的s取代杂环分子的光谱数据来充分研究星际硫消耗。本文对2CNT、3CNT及其部分同位素物的四极超精细结构进行了量子化学研究,以补充文献,并为ISM中新物种的检测提供有价值的新数据。2-氰噻吩(2CNT)、3-氰噻吩(3CNT)的核超细四极结构及其33S、2h同位素在预计发现这些化合物的温度范围内(T ~ 5K至T ~ 150)进行了分析。利用密度泛函理论(M06-2X/6-31G(d,p))计算几何参数,并对系统误差进行经验修正。计算了2CNT、3CNT、33S- 2c15nt、33S- 3c15nt、2C15NT-3D和2C15NT-2D的14N、33S和2H四极超精细常数和偶极矩,并分析了它们对应的超精细结构。讨论了最强过渡线和最优可探测区域。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Hyperfine structures of 2-cyanothiophene and 3-cyanothiophene: A quantum chemical study

Hyperfine structures of 2-cyanothiophene and 3-cyanothiophene: A quantum chemical study

A sufficient amount of spectroscopic data for S-substituted heterocyclic molecules are not available in the literature to adequately examine interstellar sulfur depletion. A quantum chemical investigation of quadrupole hyperfine structures of 2CNT, 3CNT, and some of their isotopologues is undertaken here in order to supplement the literature and supply new data that are valuable for the detection of new species in the ISM. The nuclear hyperfine quadrupole structures of 2-cyanothiophene (2CNT), 3-cyanothiophene (3CNT), and their 33S, 2H-isotopologues were analyzed at temperatures prevailing in regions where these compounds are expected to be found (T5K to T150). The geometrical parameters were calculated using density functional theory (M06-2X/6-31G(d,p)) with empirical corrections for systematic errors. The 14N, 33S, and 2H quadrupole hyperfine constants, and dipole moments for 2CNT, 3CNT, 33S-2C15NT, 33S-3C15NT, 2C15NT-3D, and 2C15NT-2D were calculated, and their corresponding hyperfine structures were analyzed. The strongest transition lines and optimal regions of detectability were also discussed.

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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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