2 research outputs found

    Popular C<sub>82</sub> Fullerene Cage Encapsulating a Divalent Metal Ion Sm<sup>2+</sup>: Structure and Electrochemistry

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    Two Sm@C<sub>82</sub> isomers have been well characterized for the first time by means of <sup>13</sup>C NMR spectroscopy, and their structures were unambiguously determined as Sm@<i>C</i><sub><i>2v</i></sub><i>(9)</i>-C<sub>82</sub> and Sm@<i>C</i><sub><i>3v</i></sub><i>(7)</i>-C<sub>82</sub>, respectively. A combined study of single crystal X-ray diffraction and theoretical calculations suggest that in Sm@<i>C</i><sub><i>2v</i></sub><i>(9)</i>-C<sub>82</sub> the preferred Sm<sup>2+</sup> ion position shall be located in a region slightly off the <i>C</i><sub>2</sub> axis of <i>C</i><sub><i>2v</i></sub><i>(9)</i>-C<sub>82</sub>. Moreover, the electrochemical surveys on these Sm@C<sub>82</sub> isomers reveal that their redox activities are mainly determined by the properties of their carbon cages

    Sm@<i>C</i><sub>2<i>v</i></sub>(19138)‑C<sub>76</sub>: A Non-IPR Cage Stabilized by a Divalent Metal Ion

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    Although a non-IPR fullerene cage is common for endohedral cluster fullerenes, it is very rare for conventional endofullerenes M@C<sub>2<i>n</i></sub>, probably because of the minimum geometry fit effect of the endohedral single metal ion. In this work, we report on a new non-IPR endofullerene Sm@<i>C</i><sub>2<i>v</i></sub>(19138)-C<sub>76</sub>, including its structural and electrochemical features. A combined study of single-crystal X-ray diffraction and DFT calculations not only elucidates the non-IPR cage structure of <i>C</i><sub>2<i>v</i></sub>(19138)-C<sub>76</sub> but also suggests that the endohedral Sm<sup>2+</sup> ion prefers to reside along the C<sub>2</sub> cage axis and close to the fused pentagon unit in the cage framework, indicative of a significant metal–cage interaction, which alone can stabilize the non-IPR cage. Furthermore, electrochemical studies reveal the fully reversible redox behaviors and small electrochemical gap of Sm@<i>C</i><sub>2<i>v</i></sub>(19138)-C<sub>76</sub>, which are comparable to those of IPR species Sm@<i>D</i><sub>3<i>h</i></sub>-C<sub>74</sub>
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