Melosso Mattia, Stoppa Paolo, Alvarado-Jiménez Daniela, Tamassia Filippo, Sapienza Carlotta, Bizzocchi Luca, Dore Luca, Puzzarini Cristina, Pietropolli Charmet Andrea, Tasinato Nicola
Dipartimento di Chimica "Giacomo Ciamician", Università di Bologna, Via F. Selmi 2, 40126 Bologna, Italy.
Dipartimento di Scienze Molecolari e Nanosistemi, Università Ca' Foscari Venezia, Via Torino 155, 30172 Venezia Mestre, Italy.
Molecules. 2025 Apr 3;30(7):1604. doi: 10.3390/molecules30071604.
Chloromethane (CHCl) is a key chlorinated organic compound not only in atmospheric chemistry, but also in the field of molecular astrophysics and a possible biosignature in exoplanetary atmospheres. While the spectroscopic characterization of the main isotopic species has been addressed in great detail, that of its isotopologues remains incomplete. This work aims at filling this gap by focusing on the bideuterated species, CHDCl, and exploiting both rotational and vibrational spectroscopy in combination with state-of-the-art quantum-chemical (QC) calculations. First, the rotational spectrum of CHDCl has been measured in the millimeter-wave domain, allowing the accurate determination of several spectroscopic constants for four isotopologues, namely CHDCl, CHDCl, CHDCl, and CHDCl. The newly determined rotational constants have been used to refine the semi-experimental equilibrium structure of chloromethane. Secondly, the vibrational analysis, supported by high-level QC predictions of vibrational energies, has been conducted in the 500-6200 cm infrared (IR) region, enabling the identification of more than 30 bands including fundamental, overtone, and combination transitions. Finally, chloromethane's radiative efficiency has been simulated using the QC IR absorption cross-sections, and the effects of isotopologue distribution on the predicted radiative properties have been investigated. All these findings greatly improve the comprehension of the spectroscopic properties of bideuterated chloromethane isotopologues, and of chloromethane in general, and facilitate future terrestrial and extraterrestrial studies.
氯甲烷(CHCl)不仅是大气化学中的一种关键氯化有机化合物,也是分子天体物理学领域的关键化合物,并且可能是系外行星大气中的生物特征。虽然主要同位素物种的光谱表征已得到详细研究,但其同位素变体的光谱表征仍不完整。这项工作旨在通过聚焦双氘代物种CHDCl,并结合旋转光谱和振动光谱以及最先进的量子化学(QC)计算来填补这一空白。首先,在毫米波域测量了CHDCl的旋转光谱,从而能够准确确定四种同位素变体(即CHDCl、CHDCl、CHDCl和CHDCl)的几个光谱常数。新确定的旋转常数已用于完善氯甲烷的半实验平衡结构。其次,在500 - 6200 cm的红外(IR)区域进行了振动分析,并得到了振动能量的高水平QC预测的支持,从而能够识别30多个谱带,包括基频、泛音和组合跃迁。最后,使用QC红外吸收截面模拟了氯甲烷的辐射效率,并研究了同位素变体分布对预测辐射特性的影响。所有这些发现极大地提高了对双氘代氯甲烷同位素变体以及一般氯甲烷光谱特性的理解,并促进了未来的地球和外星研究。