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C60(2+) 和 C60(3+) 在氖基质中的红外、近红外和紫外吸收光谱

IR, NIR, and UV Absorption Spectroscopy of C60(2+) and C60(3+) in Neon Matrixes.

作者信息

Kern Bastian, Strelnikov Dmitry, Weis Patrick, Böttcher Artur, Kappes Manfred M

机构信息

Institute of Physical Chemistry II, KIT, Fritz-Haber-Weg 2, 76131 Karlsruhe, Germany.

出版信息

J Phys Chem Lett. 2014 Feb 6;5(3):457-60. doi: 10.1021/jz402630z. Epub 2014 Jan 17.

Abstract

C60(2+) and C60(3+) were produced by electron-impact ionization of sublimed C60 and charge-state-selectively codeposited onto a gold mirror substrate held at 5 K together with neon matrix gas containing a few percent of the electron scavengers CO2 or CCl4. This procedure limits charge-changing of the incident fullerene projectiles during matrix isolation. IR, NIR, and UV-vis spectra were then measured. Ten IR absorptions of C60(2+) were identified. C60(3+) was observed to absorb in the NIR region close to the known vibronic bands of C60(+). UV spectra of C60, C60(+), and C60(2+) were almost indistinguishable, consistent with a plasmon-like nature of their UV absorptions. The measurements were supported by DFT and TDDFT calculations, revealing that C60(2+) has a singlet D5d ground state whereas C60(3+) forms a doublet of Ci symmetry. The new results may be of interest regarding the presence of C60(2+) and C60(3+) in space.

摘要

通过对升华的C60进行电子碰撞电离产生C60(2+)和C60(3+),并与含有百分之几电子清除剂CO2或CCl4的氖基质气体一起电荷态选择性地共沉积到保持在5 K的金镜基底上。该过程限制了基质隔离期间入射富勒烯射弹的电荷变化。然后测量了红外、近红外和紫外可见光谱。确定了C60(2+)的10个红外吸收峰。观察到C60(3+)在近红外区域吸收,靠近C60(+)的已知振动带。C60、C60(+)和C60(2+)的紫外光谱几乎无法区分,这与其紫外吸收的类等离子体性质一致。这些测量得到了密度泛函理论(DFT)和含时密度泛函理论(TDDFT)计算的支持,结果表明C60(2+)具有单重态D5d基态,而C60(3+)形成具有Ci对称性的双重态。这些新结果可能对于太空中C60(2+)和C60(3+)的存在具有重要意义。

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