D. V. Konarev et al.
FULL PAPER
The C60 complexes with Mn(Et2dtc)2 and Fe(Et2dtc)2 were also
obtained as powders by mixing C60 (25 mg, 0.0347 mmol) and a
twofold molar excess of M(Et2dtc)2 in C6H4Cl2 (20 mL) on heating
(60 °C, 2 h). The hot solution was filtered, cooled down to room
temperature, and stood overnight. The solution became colorless,
and a light brown polycrystalline precipitate was formed. However,
in contrast to crystals of 10, powdered samples did not show rea-
sonable elemental analyses probably because of the high air-sensi-
tivity of the complexes. Indeed, Mn(Et2dtc)2 and Fe(Et2dtc)2 are
extremely air-sensitive and oxidize in a few seconds in air.
(EtMedtc)2 and Cu(nPr2dtc)2 and complexes 11 and 13 (Tables S1
and S2, Figures S1–S7).
Acknowledgments
The work was supported by the RFBR grants N 03-03-32699-a and
03-03-20003 BNTS-a, the Russian Science Support Foundation,
Rosnauka grant 2006-RI-19.0/001/058, and partly by Grant-in-Aid
Scientific Research from the Ministry of Education, Culture,
Sports, Science and Technology, Japan (152005019, 21st Century
COE, and Elements Science 12CE2005). We thank Dr. E.I. Yud-
anova for help with the EPR investigations.
We tried to crystallize the C60 complexes with Co(Et2dtc)2 and
V(Et2dtc)2. C60 (25 mg, 0.0347 mmol) and a twofold molar excess
of M(Et2dtc)2 were dissolved in C6H4Cl2 (20 mL) on stirring at
60 °C for 4 h. The hot solution was filtered, cooled down to room
temperature, and filtered in a glass tube of 45 mL volume with a
ground glass plug. Slow diffusion of hexane (20 mL) was carried
out under anaerobic conditions. However, only black powder with-
out crystals formed after 2 months.
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General: UV/Visible-NIR spectra were measured with a Shimadzu-
3100 spectrometer in the 240–2600 nm range. FT-IR spectra were
measured in KBr pellets with a Perkin–Elmer 1000 Series spectrom-
eter (400–7800 cm–1). A Quantum Design MPMS-XL SQUID
magnetometer was used to measure static magnetic susceptibilities
of 1–4 and 10 from 1.9 up to 300 K. A sample holder contribution
and core temperature independent diamagnetic susceptibility (χ0)
were subtracted from the experimental values. The values of Θ, χ0
were calculated using the appropriate formula: χM = C/(T – Θ) +
χ0. EPR spectra were recorded for 1, 2, 11, and 13 at room temp.
and for 3, 4, and 10 from RT down to 4 K with a JEOL JES-TE
200 X-band ESR spectrometer equipped with a JEOL ES-CT470
cryostat. Photoconductivity of 1, 2, 7, and 8 was excited using a
white light halogen tube with 1012–1014 photons/cm2s intensity. To
record the spectra of photoconductivity the light beam of a xenon
lamp was transmitted through a high-aperture monochromator. A
static magnetic field with the induction up to 1 T was generated by
an electromagnet of a Radiopan SE/X 2547 ESR spectrometer.
X-ray Crystal Structure Determination: X-ray diffraction data for
1, 3, 4, 6, 7, 11, and 12 were collected with a Bruker SMART1000
CCD diffractometer installed at a rotating anode source (Mo-Kα
radiation, λ = 0.71073 Å), and equipped with an Oxford Cryosys-
tems nitrogen gas-flow apparatus. The data were collected by the
rotation method with 0.3° frame-width (ω scan) and 10 s exposure
time per frame. Four sets of data (600 frames in each set) were
collected, nominally covering half of the reciprocal space. The data
were integrated, scaled, sorted and averaged using the SMART
software package.[66] The structures were solved by the direct meth-
ods using SHELXTL NT Version 5.10.[67] The structure was re-
fined by full-matrix least-squares against F2. The details of the X-
ray crystal structure analysis for 1, 3, 4, 6, 7, 11, and 12 including
CCDC numbers for the structures are given in Table 4. Non-hydro-
gen atoms were refined in the anisotropic approximation. Positions
of hydrogen atoms were calculated geometrically. Subsequently, the
positions of H-atoms were refined by the “riding” model with Uiso
= 1.2Ueq of the connected non-hydrogen atom or as ideal CH3
groups with Uiso = 1.5Ueq. The supplementary crystallographic
data for this paper can be obtained free of charge from The Cam-
bridge Crystallographic Data Centre via www.ccdc.cam.ac.uk/
data_request/cif.
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Supporting Information (for details see the footnote on the first
page of this article): IR-data, UV/Vis-NIR spectra of pristine do-
nors and complexes 1–15, and EPR spectra of pristine Cu-
1894
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Eur. J. Inorg. Chem. 2006, 1881–1895