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星际多环芳烃的振动光谱:1-氰基萘和2-氰基萘。

Vibrational spectroscopy of interstellar PAHs: 1-cyanonaphthalene and 2-cyanonaphthalene.

作者信息

Rawat Vandana, Shastri Aparna, Das Asim K, Sharma Neha, Bhatt Himal, Rajasekhar B N

机构信息

Atomic & Molecular Physics Division, Bhabha Atomic Research Centre, Mumbai 400085, India; Homi Bhabha National Institute, Anushaktinagar, Mumbai 400094, India.

Atomic & Molecular Physics Division, Bhabha Atomic Research Centre, Mumbai 400085, India; Homi Bhabha National Institute, Anushaktinagar, Mumbai 400094, India.

出版信息

Spectrochim Acta A Mol Biomol Spectrosc. 2025 Jan 5;324:124971. doi: 10.1016/j.saa.2024.124971. Epub 2024 Aug 13.

Abstract

In this work, we present a comprehensive experimental and theoretical study of the vibrational spectra of PAH molecules recently detected in the interstellar medium: 1-cyanonaphthalene and 2-cyanonaphthalene. The room temperature IR spectra of 1- and 2-cyanonaphthalene in the region 100-3100 cm and their vibrational Raman spectra in the region 35-3100 cm are reported here for the first time. A detailed spectral analysis is carried out using quantum chemical calculations employing the DFT methodology. Anharmonic corrections using the VPT2 method yield excellent agreement with the experimental spectra. A re-investigation of the vibrational spectrum of the parent molecule: naphthalene validates the experimental and theoretical methods used. A consistent set of assignments is reported for the fundamental bands of 1- and 2-cyanonapththalene. The experimental and theoretical data presented here would be useful inputs for modelling the role of cyanonaphthalene in astrophysical processes.

摘要

在这项工作中,我们对最近在星际介质中检测到的多环芳烃分子(1-氰基萘和2-氰基萘)的振动光谱进行了全面的实验和理论研究。本文首次报道了1-氰基萘和2-氰基萘在100 - 3100厘米区域的室温红外光谱以及在35 - 3100厘米区域的振动拉曼光谱。使用采用密度泛函理论(DFT)方法的量子化学计算进行了详细的光谱分析。使用VPT2方法进行的非谐校正与实验光谱取得了极好的一致性。对母体分子萘的振动光谱进行的重新研究验证了所使用的实验和理论方法。报告了1-氰基萘和2-氰基萘基频带的一组一致的归属。这里给出的实验和理论数据将为模拟氰基萘在天体物理过程中的作用提供有用的输入。

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