Theoretical investigation of photoabsorption in Cyanogen cluster

S. Parida, S. Sahu, Sagar B. Sharma
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Abstract

In this paper, photoabsorption spectrum of Cyanogen cluster has been investigated. The calculations of excitation energies, oscillator strengths and transition dipole moments are performed using the time-dependent density functional theory (TDDFT) approach. The first resonant peak for NCCN and NCNC isomer are found to occur at around 7.66, 6.94 eV, respectively. Furthermore, in case of NCCN, NCNC isomer the spectacular transitions of the spectra occurred in the far-UV (FUV) region of the electromagnetic spectrum. In addition, the absorption spectrum of NCNC isomer is red-shifted as compared to that of NCCN isomer. The natures of these excitations were investigated by analyzing the frontier molecular orbital's involved with these optical transitions. That means the LUMO of NCCN is combinations of s (85%) and p (15%) hybrid orbital's whereas in case of the NCNC, the LUMO corresponding to the first peak is contributed by both s (65%) and p (35%) orbits. However, the HOMO of both NCCN and CNCN are purely s-types.
氰簇光吸收的理论研究
本文研究了氰团簇的光吸收光谱。利用时变密度泛函理论(TDDFT)方法计算了激发态能、振子强度和跃迁偶极矩。NCCN和NCNC异构体的第一个共振峰分别出现在7.66和6.94 eV左右。此外,对于NCCN, NCNC异构体,在电磁波谱的远紫外(FUV)区域发生了显著的光谱跃迁。此外,与NCCN异构体相比,NCNC异构体的吸收光谱发生了红移。通过分析与这些光学跃迁有关的前沿分子轨道来研究这些激发的性质。这意味着NCCN的LUMO是s(85%)和p(15%)杂化轨道的组合,而NCNC的第一个峰对应的LUMO是s(65%)和p(35%)轨道的共同贡献。而NCCN和CNCN的HOMO都是纯s型。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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