Abstract

Vibrationally resolved electronic absorption spectrum of 1,2-dihydrogenated[60]fullerene has been recorded in a 6 K neon matrix after mass-selected deposition of m/z = 722 cations produced from reaction of protonated methane and C60 in an ion source. One system has the origin band at 688.5 ± 0.1 nm and another commencing at 404.8 ± 0.1 nm. Theoretical computations were used to calculate the relative energies of three isomers of dihydrogenated[60]fullerene and time-dependent density functional theory predicted the vertical excitations to 50 electronic states.

Highlights

  • Fullerenes are spherical or ellipsoidal structures of pure carbon, such as C60, C70, and C84

  • Computational.—Equilibrium structures for different isomers of C60H2 were calculated with density functional theory (DFT) using B3LYP functional18.19 and cc-pVDZ basis set.[20]

  • The electronic spectrum of 1,2- dihydrogenated[60]fullerene (1,2C60H2) in a 6 K neon matrix is illustrated in Figures 1 and 2

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Summary

Introduction

Fullerenes are spherical or ellipsoidal structures of pure carbon, such as C60, C70, and C84. ISM would be ionized, being predicted first by Kroto.[11] Recently, it has been shown that C6+0 is the carrier of five astronomical absorption features, known as diffuse interstellar bands (DIBs).[12,13,14,15] It has been suggested that C6+0 may atomic hydrogen,[2] making C60Hn undergo ion-neutral reactions with + (n > 1) cations possible species in the ISM. These types of protonated species could be candidate molecules for the DIBs observed towards reddened stars. Mass-selective deposition of C60 H2+ was undertaken; electron recombination occurred with cations in the crystalline neon and only neutral C60H2 was observed

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