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