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were observed (Figure S7). The energy-dispersive X-ray
Therefore, the Ace-COF-Ni was examined in the visible-
(EDX) mapping images of the Ace-COF-Ni give clear
evidence for the presence of C, N, Cl, and Ni which are
homogeneously distributed in the COF matrix (Figures S7
and S8). Bright contrast features in the Z-contrast HAADF-
STEM image correspond to single atoms spread within the
Ace-COF supporting material (Figure 1g), some examples
are marked by the white arrows). Ni as the heaviest element
in the Ace-COF-Ni, the bright contrast features highlighted
by the white arrows in the Z-contrast HAADF-STEM images
can be safely attributed to single sites of Ni sitting within the
Ace-COF network. The Ni content, determined by induc-
tively coupled plasma mass spectrometry (ICP-MS) is
1.03 mmolgÀ1.
The surface area of the Ace-COF and Ace-COF-Ni
compound was determined by measuring the Argon adsorp-
tion isotherm at 87 K of the activated samples. As shown in
Figure S9a, a sharp increase in the gas uptake is observed at
low relative pressures (P/P0 < 0.1) indicating the presence of
micropores. The Brunauer–Emmett–Teller (BET) surface
area and total pore volume (at P/P0 = 0.97) decreased from
1238 m2 gÀ1 and 0.85 cm3 gÀ1 for Ace-COF to 825 m2 gÀ1 and
0.61 cm3 gÀ1 for Ace-COF-Ni, respectively. The pore sizes of
both the Ace-COF and Ace-COF-Ni were calculated to be
0.97 nm in diameter using Ar at 87 K quenched solid density
functional theory (QSDFT) carbon model (Figure S9b). From
these observations, it is clear that, although the interior
cavities of the Ace-COF-Ni are partially occupied by Ni ions,
the Ace-COF-Ni structure exhibits a permanent open struc-
ture, ensuring a good diffusion of the reactants to the Ni
active sites. Besides a permanent porosity, thermal stability is
also very important for its practical application as a hetero-
geneous catalyst. As indicated in Figure S10, the thermo-
gravimetric analysis (TGA) shows that both Ace-COF and
Ace-COF-Ni possess excellent thermal stability, up to 4508C
under a nitrogen atmosphere.
light-driven S–C cross-coupling reaction to evaluate its
potential as a dual catalyst. First, iodobenzene (1a) and
thiophenol (2a) were used as model substrates for the
optimization of the reaction conditions (Table 1). More
specifically, under an Ar atmosphere, a reaction mixture of
iodobenzene (0.5 mmol) (1a), thiophenol (0.75 mmol) (2a),
2 mol% Ace-COF-Ni, and pyridine (1 mmol) in anhydrous
acetonitrile (5 mL) was irradiated with 34W blue LEDs (420–
430 nm). After 24 hours, an excellent yield (> 95%) towards
the corresponding S–C cross-coupled product phenyl sulfide
(3a) was obtained at room temperature (Table 1, entry 1).
From the blank tests, it was noted that no reaction occurred in
the absence of light, the absence of pyridine, or the absence of
Ace-COF-Ni (Table 1, entries 2–4). When the model com-
pound MC-Ni instead of the Ace-COF-Ni was added into the
reaction mixture, no detectable product of phenyl sulfide was
observed, which suggests that the photosensitive triazine-
based Ace-COF scaffold is essential (Table 1, entry 5). When
using Ace-COF instead of Ace-COF-Ni, no product was
detected, implying that Ni also plays a crucial role in this
cross-coupling reaction (Table 1, entry 6). Interestingly, when
using a physical mixture of either Ace-COF and NiCl2·6H2O
or Ace-COF and the model compound MC-Ni as the catalyst
(Table 1, entries 7 and 8), also significant amounts of the
product was observed (58%, 26%), albeit much lower than
with the Ace-COF-Ni. This might be due to the in situ
formation of Ace-COF-Ni by Ace-COF scaffold and
NiCl2·6H2O. In the case of the mixture of MC-Ni and Ace-
COF, the COF will act as the required photosensitizer to
allow the reaction to proceed, which has been reported
previously.[17] Based on these results, it is clear that both
photosensitive triazine-based Ace-COF scaffold and Ni are
Table 1: Ace-COF-Ni dual-catalyzed S–C cross-coupling: influence of
reaction parameters.
The optical properties of Ace-COF-Ni and Ace-COF
were assessed to verify the feasibility of using Ace-COF-Ni to
catalyze reactions under visible light irradiation solely.
UV/Vis absorption experiments are carried out at room
temperature, the UV-vis spectra indicate that the Ace-COF
and the Ace-COF-Ni can absorb light in the UV and visible
regions (Figure S11). However, the Ace-COF-Ni model
compound (abbreviated as MC-Ni, Scheme 2a) only absorbs
UV light. The optical band gaps of Ace-COF, Ace-COF-Ni,
and MC-Ni were analyzed to be 1.74 eV, 1.83 eV, and 2.85 eV,
respectively. Ace-COF and Ace-COF-Ni have a much smaller
band gap than the model compound, this can be explained by
the introduction of the electron-accepting triazine unit, the
extended imine conjugation in the x and y direction of the
COF structure, and enhanced p-conjugation between the
COF layers. In comparison with the previously reported
photocatalytic COFs, such as LZU-190, LZU-191, and
LZU-192 (optical band gaps are 2.02 eV, 2.38 eV, and
2.10 eV, respectively).[13b] Ace-COF-Ni and Ace-COF show
enhanced absorption in the visible light range. This implies
that the Ace-COF-Ni is a promising platform for visible-light-
driven organic transformation reactions.
Entry
Variation from the standard conditions
Yield [%][b]
1
2
3
4
5
6
7
Standard conditions[a]
No light (dark)
>95
No Product
No Product
No Product
No Product
No Product
58
No pyridine
No Ace-COF-Ni
MC-Ni instead of Ace-COF-Ni
Ace-COF instead of Ace-COF-Ni
Ace-COF mixed NiCl2·6H2O
instead of Ace-COF-Ni
Ace-COF mixed MC-Ni
instead of Ace-COF-Ni
0.5 mol% Ace-COF-Ni
1 mol% Ace-COF-Ni
2 mol% Ace-COF-Ni
8
26
9
10
11
35
73
>95
[a] Standard conditions: Under an Ar atmosphere, 1a (0.50 mmol), 2a
(0.75 mmol), 2 mol% Ace-COF-Ni, pyridine (1 mmol), and 5 mL of
99.8% anhydrous acetonitrile, then 34 W blue LED irradiation for 24 h at
R.T. [b] yield was determined by 1H NMR spectroscopy with CH3NO2 as
an internal standard.
Angew. Chem. Int. Ed. 2021, 60, 10820 –10827
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