C -Catalyzed Reduction of Azo Derivatives
60
the same as that after NaBH +H O was added, and their
tween MO and C . It has been reported that Ag nanoparti-
4
2
60
UV spectra were identical as well (Figure 2, a versus b).
cles have the best catalytic performance among Ag, Au, and
Pt nanoparticles as MO is most easily adsorbed on its sur-
This suggested that C60 did not react with NaBH +H O
4
2
[9]
under UV irradiation to form C H species. We also consid-
face and activated. Thus, C -catalyzed MO reduction is
6
0
2
60
ered the possibility of C (OH) and C anion as reaction
most likely initiated by adsorption of MO on the C60 cluster
surface by using its vacant orbital to accept the electrons of
the bonding orbital in azo compounds under UV irradiation.
This possibly leads to the activation of MO.
6
0
n
60
intermediates. It has been reported that C (OH) dissolves
6
13]
0
n
[
in water to form a yellow aqueous solution and the forma-
[7]
tion of the C60 anion changes the solution color as well.
From samples b and c shown in Figure S6 (see the Support-
ing Information), it can be seen that the color of the toluene
layer (top) did not change and the water layer (bottom) was
colorless. Furthermore, the UV spectra of C , C -NaBH -
For a deeper understanding of MO activation by C
60
[16]
under UV irradiation, the unrestricted M062X method in
[17]
the Gaussian 09 program was adopted to investigate the
interaction between C and MO under UV irradiation since
6
0
60
4
60
[18]
H O-dark, and C -NaBH -H O-UV were identical (see the
a recent report recommends this functional for the fuller-
ene system. In our study, C60 does not dissolve in water and
acts as a heterogeneous catalyst to promote the reduction of
2
60
4
2
Supporting Information), thereby implying that C (OH)
n
6
0
and C60 anions did not form by the reaction of C60 with
[8]
[9]
NaBH +H O under UV irradiation. It has been reported
azo compounds, just like the Pd and Ag nanoparticle. To
simplify the calculation, one C60 molecule was chosen as
a model to investigate the interaction between C60 and MO.
Based on calculation results, C60 in the ground state (singlet
C ) has vacant bonding orbitals (orbitals with negative ener-
4
2
[13]
that the C (OH) species can dissolve in water. However,
60
n
the C (OH) species was not detected in the reaction solu-
60
n
tion by electrospray ionization, atmospheric pressure photo-
ionization, or atmospheric-pressure chemical ionization
mass spectrometries.
6
0
gies from 181 to 183, Figure 3), which indicate that it is
a electron acceptor. This is consistent with a previous
An inductively coupled plasma (ICP) emission spectrome-
ter was used to detect the metal contaminates in C . Trace
[19]
report and means that using the C60 molecule as a model
60
amounts (i.e., ppm) of Co, Cr,
Cu, Fe, and Ag were detected
(
see the Supporting Informa-
[6]
tion). These metal contami-
nants were removed by treating
C60 successively with HCl (12m)
and HNO (0.5m). ICP analysis
3
was carried out for the acid-
treated C60 and no residual
metal
contaminants
were
found. According to Figure S7
in the Supporting Information,
13
the C NMR spectrum of C60 is Figure 3. HOMO orbitals and the corresponding orbital energies of singlet (left) and triplet C60 (right). Bond-
ing orbitals have negative energy.
the same as that of acid-treated
C . This is also true for UV
60
spectra of C60 and acid-treated
C60 (see the Supporting Information). This means that C60
kept its structure after acid treatment. Then the treated C60
was used to reduce MO under UV irradiation in the pres-
can provide reliable information for the investigated system.
After C60 is irradiated by UV light, electrons are generally
excited into orbital 181 from orbital 180 and triplet C60 is
formed. An unrestricted M062X calculation was performed
for the triplet species to obtain orbital information. From
Figure 3, the energies of the half-occupied orbitals of triplet
C60 (orbital 180 and 181) are lower than those of the unoc-
cupied orbital of singlet C60 (orbital 181). Thus, C60 accepts
electrons more easily in the excited state than in the ground
state. The interaction energy between singlet C and MO is
ence of NaBH . From Figure S9 in the Supporting Informa-
4
tion, the treated C60 still effectively catalyzed MO reduction.
Thus, metal contaminants are not the driving force behind
fullerene catalytic activity.
It is well known that C60 is a better electron acceptor
[14,15]
under light irradiation than under dark conditions.
Also,
azo compounds contain N atoms and aromatic rings, which
are all electron-donor moieties. Therefore, C60 might cata-
lyze the reduction of azo compounds by using its vacant or-
bital to accept the electrons of the bonding orbital in azo
compounds. According to Figure S10 in the Supporting In-
formation, a small amount of MO molecules are adsorbed
on the C60 surface without UV irradiation. After UV irradia-
tion for 2h, the UV peak of MO clearly decreases, which
implies that UV irradiation can increase the interaction be-
6
0
À1
24.5 kcalmol , and smaller than that between triplet C
60
À1
and MO (54.0 kcalmol ). This accounts well as to why MO
is more easily adsorbed on the C60 surface under UV irradia-
tion than without UV irradiation (see the Supporting Infor-
mation). Singlet C60 interacts with MO to form a complex
(C SMO), whereas the complex from the interaction be-
60
tween triplet C60 and MO is named as C TMO. From
60
Figure 4, it can be seen that the length of the N=N bond is
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