This article reviews the current status of chemically doped fullerene superconductors and related compounds, with particular focus on Mott–Hubbard states and the role of molecular orbital degeneracy. Alkaline-earth metal fullerides produce superconductors of several kinds, all of which have states with higher valence than (C 60 ) 6− , where the second lowest unoccupied molecular orbital (the LUMO + 1 state) is filled. Alkali-metal-doped fullerides, on the other hand, afford superconductors only at the stoichiometry A 3 C 60 (A denotes alkali metal) and in basically fcc structures. The metallicity and superconductivity of A 3 C 60 compounds are destroyed either by reduction of the crystal symmetry or by change in the valence of C 60 . This difference is attributed to the narrower bandwidth in the A 3 C 60 system, causing electronic instability in Jahn–Teller insulators and Mott–Hubbard insulators. The latter metal–insulator transition is driven by intercalation of ammonia molecules into A 3 C 60 -type superconductors. Furthermore, the triple degeneracy of the LUMO state of C 60 plays a crucial role in the metal–insulator transition and in controlling the magnetic structures of insulating states, possibly providing novel properties of degenerate orbitals. The goal of this article is to establish a unifying picture of fullerene intercalation compounds, and to clarify the underlying physics: competing energy scales and orbital properties of molecule-based systems.
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Iwasa et al. (2003) studied this question.
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