28 research outputs found
Detection of a Family of Gadolinium-Containing Endohedral Fullerenes and the Isolation and Crystallographic Characterization of One Member as a Metal−Carbide Encapsulated inside a Large Fullerene Cage
A series of di-gadolinium endohedrals that extends from Gd2C90 to Gd2C124 has been detected by mass spectrometry of the o-dichlorobenzene extract of the carbon soot produced by direct current arcing of graphite rods filled with a mixture of Gd2O3 and graphite powder. Chromatographic separation has led to the isolation of pure samples of two isomers of Gd2C94 and the complete series from Gd2C96 to Gd2C106. Endohedral fullerenes of the type M2C2n can exist as the conventional endohedral, M2@C2n, or as the carbide-containing endohedral, M2C2@C2n−2. Crystallographic characterization of the more rapidly eluting isomer of Gd2C94 reveals that it possesses the carbide structure, Gd2C2@D3(85)-C92. Computational studies suggest that the more slowly eluting isomer of Gd2C94 may be a conventional endohedral, Gd2@C2(121)-C94
Detection of a Family of Gadolinium-Containing Endohedral Fullerenes and the Isolation and Crystallographic Characterization of One Member as a Metal−Carbide Encapsulated inside a Large Fullerene Cage
A series of di-gadolinium endohedrals that extends from Gd2C90 to Gd2C124 has been detected by mass spectrometry of the o-dichlorobenzene extract of the carbon soot produced by direct current arcing of graphite rods filled with a mixture of Gd2O3 and graphite powder. Chromatographic separation has led to the isolation of pure samples of two isomers of Gd2C94 and the complete series from Gd2C96 to Gd2C106. Endohedral fullerenes of the type M2C2n can exist as the conventional endohedral, M2@C2n, or as the carbide-containing endohedral, M2C2@C2n−2. Crystallographic characterization of the more rapidly eluting isomer of Gd2C94 reveals that it possesses the carbide structure, Gd2C2@D3(85)-C92. Computational studies suggest that the more slowly eluting isomer of Gd2C94 may be a conventional endohedral, Gd2@C2(121)-C94
Single Samarium Atoms in Large Fullerene Cages. Characterization of Two Isomers of Sm@C<sub>92</sub> and Four Isomers of Sm@C<sub>94</sub> with the X-ray Crystallographic Identification of Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub>, Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub>, and Sm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>
Two isomers of Sm@C<sub>92</sub> and four isomers of
Sm@C<sub>94</sub> were isolated from carbon soot obtained by electric
arc vaporization
of carbon rods doped with Sm<sub>2</sub>O<sub>3</sub>. Analysis of
the structures by single-crystal X-ray diffraction on cocrystals formed
with Ni<sup>II</sup>(octaethylporphyrin) reveals the identities of
two of the Sm@C<sub>92</sub> isomers: Sm@C<sub>92</sub>(I), which
is the more abundant isomer, is Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub>, and Sm@C<sub>92</sub>(II) is Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub>. The structure of the
most abundant form of the four isomers of Sm@C<sub>94</sub>, Sm@C<sub>94</sub>(I), is Sm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>, which utilizes the same cage isomer as the
previously known Ca@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub> and Tm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>. All of the structurally characterized
isomers obey the isolated pentagon rule. While the four Sm@C<sub>90</sub> and five isomers of Sm@C<sub>84</sub> belong to common isomerization
maps that allow these isomers to be interconverted through Stone–Wales
transformations, Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub> and Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub> are not related to each other by any set of Stone–Wales
transformations. UV–vis–NIR spectroscopy and computational
studies indicate that Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub> is more stable than Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub> but possesses a smaller HOMO–LUMO
gap. While the electronic structures of these endohedrals can be formally
described as Sm<sup>2+</sup>@C<sub>2<i>n</i></sub><sup>2–</sup>, the net charge transferred to the cage is less than two due to
some back-donation of electrons from π orbitals of the cage
to the metal ion
Fabrication of Mesoporous Co<sub>3</sub>O<sub>4</sub> from LP-FDU-12 via Nanocasting Route and Effect of Wall/Pore Size on Their Magnetic Properties
Highly ordered mesoporous Co<sub>3</sub>O<sub>4</sub> nanostructures
were prepared using LP-FDU-12 as hard templates. By changing the hydrothermal
temperature or by the acid treatment of the LP-FDU-12 template, Co<sub>3</sub>O<sub>4</sub> replicas with different cell parameters and
wall thicknesses have been obtained. The structure and textural characteristics
of both LP-FDU-12 and Co<sub>3</sub>O<sub>4</sub> replicas were investigated
by X-ray diffraction, transmission electron microscopy, and N<sub>2</sub> adsorption–desorption isotherm analysis. The cell
parameter and wall thickness of a mesoporous Co<sub>3</sub>O<sub>4</sub> have been varied systematically within the ranges 30.4–33.9
and 24.8–18.2 nm, respectively, and the materials exhibit surface
areas in the 29.6–52.9 m<sup>2</sup> g<sup>–1</sup> range,
while preserving a highly ordered 3D pore structure and highly crystalline
walls. Most importantly, magnetic studies show that the factors which
affect the magnetic behavior in the Co<sub>3</sub>O<sub>4</sub> nanosphere
system are not only the sphere size but also the space-filled parameter
at the nanoscale
Single Samarium Atoms in Large Fullerene Cages. Characterization of Two Isomers of Sm@C<sub>92</sub> and Four Isomers of Sm@C<sub>94</sub> with the X-ray Crystallographic Identification of Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub>, Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub>, and Sm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>
Two isomers of Sm@C<sub>92</sub> and four isomers of
Sm@C<sub>94</sub> were isolated from carbon soot obtained by electric
arc vaporization
of carbon rods doped with Sm<sub>2</sub>O<sub>3</sub>. Analysis of
the structures by single-crystal X-ray diffraction on cocrystals formed
with Ni<sup>II</sup>(octaethylporphyrin) reveals the identities of
two of the Sm@C<sub>92</sub> isomers: Sm@C<sub>92</sub>(I), which
is the more abundant isomer, is Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub>, and Sm@C<sub>92</sub>(II) is Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub>. The structure of the
most abundant form of the four isomers of Sm@C<sub>94</sub>, Sm@C<sub>94</sub>(I), is Sm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>, which utilizes the same cage isomer as the
previously known Ca@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub> and Tm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>. All of the structurally characterized
isomers obey the isolated pentagon rule. While the four Sm@C<sub>90</sub> and five isomers of Sm@C<sub>84</sub> belong to common isomerization
maps that allow these isomers to be interconverted through Stone–Wales
transformations, Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub> and Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub> are not related to each other by any set of Stone–Wales
transformations. UV–vis–NIR spectroscopy and computational
studies indicate that Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub> is more stable than Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub> but possesses a smaller HOMO–LUMO
gap. While the electronic structures of these endohedrals can be formally
described as Sm<sup>2+</sup>@C<sub>2<i>n</i></sub><sup>2–</sup>, the net charge transferred to the cage is less than two due to
some back-donation of electrons from π orbitals of the cage
to the metal ion
Single Samarium Atoms in Large Fullerene Cages. Characterization of Two Isomers of Sm@C<sub>92</sub> and Four Isomers of Sm@C<sub>94</sub> with the X-ray Crystallographic Identification of Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub>, Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub>, and Sm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>
Two isomers of Sm@C<sub>92</sub> and four isomers of
Sm@C<sub>94</sub> were isolated from carbon soot obtained by electric
arc vaporization
of carbon rods doped with Sm<sub>2</sub>O<sub>3</sub>. Analysis of
the structures by single-crystal X-ray diffraction on cocrystals formed
with Ni<sup>II</sup>(octaethylporphyrin) reveals the identities of
two of the Sm@C<sub>92</sub> isomers: Sm@C<sub>92</sub>(I), which
is the more abundant isomer, is Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub>, and Sm@C<sub>92</sub>(II) is Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub>. The structure of the
most abundant form of the four isomers of Sm@C<sub>94</sub>, Sm@C<sub>94</sub>(I), is Sm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>, which utilizes the same cage isomer as the
previously known Ca@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub> and Tm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>. All of the structurally characterized
isomers obey the isolated pentagon rule. While the four Sm@C<sub>90</sub> and five isomers of Sm@C<sub>84</sub> belong to common isomerization
maps that allow these isomers to be interconverted through Stone–Wales
transformations, Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub> and Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub> are not related to each other by any set of Stone–Wales
transformations. UV–vis–NIR spectroscopy and computational
studies indicate that Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub> is more stable than Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub> but possesses a smaller HOMO–LUMO
gap. While the electronic structures of these endohedrals can be formally
described as Sm<sup>2+</sup>@C<sub>2<i>n</i></sub><sup>2–</sup>, the net charge transferred to the cage is less than two due to
some back-donation of electrons from π orbitals of the cage
to the metal ion
Single Samarium Atoms in Large Fullerene Cages. Characterization of Two Isomers of Sm@C<sub>92</sub> and Four Isomers of Sm@C<sub>94</sub> with the X-ray Crystallographic Identification of Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub>, Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub>, and Sm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>
Two isomers of Sm@C<sub>92</sub> and four isomers of
Sm@C<sub>94</sub> were isolated from carbon soot obtained by electric
arc vaporization
of carbon rods doped with Sm<sub>2</sub>O<sub>3</sub>. Analysis of
the structures by single-crystal X-ray diffraction on cocrystals formed
with Ni<sup>II</sup>(octaethylporphyrin) reveals the identities of
two of the Sm@C<sub>92</sub> isomers: Sm@C<sub>92</sub>(I), which
is the more abundant isomer, is Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub>, and Sm@C<sub>92</sub>(II) is Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub>. The structure of the
most abundant form of the four isomers of Sm@C<sub>94</sub>, Sm@C<sub>94</sub>(I), is Sm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>, which utilizes the same cage isomer as the
previously known Ca@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub> and Tm@<i>C</i><sub>3<i>v</i></sub>(134)-C<sub>94</sub>. All of the structurally characterized
isomers obey the isolated pentagon rule. While the four Sm@C<sub>90</sub> and five isomers of Sm@C<sub>84</sub> belong to common isomerization
maps that allow these isomers to be interconverted through Stone–Wales
transformations, Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub> and Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub> are not related to each other by any set of Stone–Wales
transformations. UV–vis–NIR spectroscopy and computational
studies indicate that Sm@<i>C</i><sub>1</sub>(42)-C<sub>92</sub> is more stable than Sm@<i>C</i><sub><i>s</i></sub>(24)-C<sub>92</sub> but possesses a smaller HOMO–LUMO
gap. While the electronic structures of these endohedrals can be formally
described as Sm<sup>2+</sup>@C<sub>2<i>n</i></sub><sup>2–</sup>, the net charge transferred to the cage is less than two due to
some back-donation of electrons from π orbitals of the cage
to the metal ion
Isolation of Three Isomers of Sm@C<sub>84</sub> and X-ray Crystallographic Characterization of Sm@<i>D</i><sub>3<i>d</i></sub>(19)-C<sub>84</sub> and Sm@<i>C</i><sub>2</sub>(13)-C<sub>84</sub>
Three isomers with the composition Sm@C<sub>84</sub> were
isolated
from carbon soot obtained by electric arc vaporization of carbon rods
doped with Sm<sub>2</sub>O<sub>3</sub>. These isomers were labeled
Sm@C<sub>84</sub>(I), Sm@C<sub>84</sub>(II), and Sm@C<sub>84</sub>(III) in order of their elution times during chromatography on a
Buckyprep column with toluene as the eluent. Analysis of the structures
by single-crystal X-ray diffraction on cocrystals formed with Ni<sup>II</sup>(octaethylporphyrin) reveals the identities of two of the
isomers: Sm@C<sub>84</sub>(I) is Sm@<i>C</i><sub>2</sub>(13)-C<sub>84</sub>, and Sm@C<sub>84</sub>(III) is Sm@ <i>D</i><sub>3<i>d</i></sub>(19)-C<sub>84</sub>. Sm@C<sub>84</sub>(II) can be identified as Sm@<i>C</i><sub>2</sub>(11)-C<sub>84</sub> on the basis of the similarity of its UV/vis/NIR spectrum
with that of Yb@<i>C</i><sub>2</sub>(11)-C<sub>84</sub>,
whose carbon cage has been characterized by <sup>13</sup>C NMR spectroscopy.
Comparison of the three Sm@C<sub>84</sub> isomers identified in this
project with two prior reports of the preparation and isolation of
isomers of Sm@C<sub>84</sub> indicate that five different Sm@C<sub>84</sub> isomers have been found and that the source of samarium
used for the generation of fullerene soot is important in determining
which of these isomers form
Isolation of Three Isomers of Sm@C<sub>84</sub> and X-ray Crystallographic Characterization of Sm@<i>D</i><sub>3<i>d</i></sub>(19)-C<sub>84</sub> and Sm@<i>C</i><sub>2</sub>(13)-C<sub>84</sub>
Three isomers with the composition Sm@C<sub>84</sub> were
isolated
from carbon soot obtained by electric arc vaporization of carbon rods
doped with Sm<sub>2</sub>O<sub>3</sub>. These isomers were labeled
Sm@C<sub>84</sub>(I), Sm@C<sub>84</sub>(II), and Sm@C<sub>84</sub>(III) in order of their elution times during chromatography on a
Buckyprep column with toluene as the eluent. Analysis of the structures
by single-crystal X-ray diffraction on cocrystals formed with Ni<sup>II</sup>(octaethylporphyrin) reveals the identities of two of the
isomers: Sm@C<sub>84</sub>(I) is Sm@<i>C</i><sub>2</sub>(13)-C<sub>84</sub>, and Sm@C<sub>84</sub>(III) is Sm@ <i>D</i><sub>3<i>d</i></sub>(19)-C<sub>84</sub>. Sm@C<sub>84</sub>(II) can be identified as Sm@<i>C</i><sub>2</sub>(11)-C<sub>84</sub> on the basis of the similarity of its UV/vis/NIR spectrum
with that of Yb@<i>C</i><sub>2</sub>(11)-C<sub>84</sub>,
whose carbon cage has been characterized by <sup>13</sup>C NMR spectroscopy.
Comparison of the three Sm@C<sub>84</sub> isomers identified in this
project with two prior reports of the preparation and isolation of
isomers of Sm@C<sub>84</sub> indicate that five different Sm@C<sub>84</sub> isomers have been found and that the source of samarium
used for the generation of fullerene soot is important in determining
which of these isomers form
Isolation of Three Isomers of Sm@C<sub>84</sub> and X-ray Crystallographic Characterization of Sm@<i>D</i><sub>3<i>d</i></sub>(19)-C<sub>84</sub> and Sm@<i>C</i><sub>2</sub>(13)-C<sub>84</sub>
Three isomers with the composition Sm@C<sub>84</sub> were
isolated
from carbon soot obtained by electric arc vaporization of carbon rods
doped with Sm<sub>2</sub>O<sub>3</sub>. These isomers were labeled
Sm@C<sub>84</sub>(I), Sm@C<sub>84</sub>(II), and Sm@C<sub>84</sub>(III) in order of their elution times during chromatography on a
Buckyprep column with toluene as the eluent. Analysis of the structures
by single-crystal X-ray diffraction on cocrystals formed with Ni<sup>II</sup>(octaethylporphyrin) reveals the identities of two of the
isomers: Sm@C<sub>84</sub>(I) is Sm@<i>C</i><sub>2</sub>(13)-C<sub>84</sub>, and Sm@C<sub>84</sub>(III) is Sm@ <i>D</i><sub>3<i>d</i></sub>(19)-C<sub>84</sub>. Sm@C<sub>84</sub>(II) can be identified as Sm@<i>C</i><sub>2</sub>(11)-C<sub>84</sub> on the basis of the similarity of its UV/vis/NIR spectrum
with that of Yb@<i>C</i><sub>2</sub>(11)-C<sub>84</sub>,
whose carbon cage has been characterized by <sup>13</sup>C NMR spectroscopy.
Comparison of the three Sm@C<sub>84</sub> isomers identified in this
project with two prior reports of the preparation and isolation of
isomers of Sm@C<sub>84</sub> indicate that five different Sm@C<sub>84</sub> isomers have been found and that the source of samarium
used for the generation of fullerene soot is important in determining
which of these isomers form