4
30
X.-y. Xu et al. / Spectrochimica Acta Part A: Molecular and Biomolecular Spectroscopy 95 (2012) 427–434
Table 1
[Cu(Phen-Np-Et)(POP)]BF
band centering at 550 nm as shown in Fig. 4. The emission band
shows no vibronic progressions with full-width-at-half-
maximum (FWHF) of 93 nm, which indicates that the emissive
state owns a charge-transfer (CT) character. The Stokes shift of
4
in solid state gives a broad emission
Selected bond lengths (Å) and angles (°) of [Cu(Phen-Np-Et)(POP)]BF
single crystal.
4
obtained from
a
Bond length
(Å)
Bond angle
(°)
Cu(1)–N(1)
Cu(1)–N(2)
Cu(1)–P(1)
Cu(1)–P(2)
Cuꢂ ꢂ ꢂO
2.074
2.035
2.226
2.255
3.063
N(1)–Cu–N(2)
N(1)–Cu–P(1)
N(2)–Cu–P(1)
N(1)–Cu–P(2)
N(2)–Cu–P(2)
P(1)–Cu–P(2)
80.46
109.14
122.59
104.44
113.11
118.06
4
[Cu(Phen-Np-Et)(POP)]BF between its absorption edge and emis-
sion maximum is calculated to be 90 nm, which is comparable
with literature values [8]. This large value suggests that there is
an intense structural relaxation that occurs in excited state. The
emissive energy of 550 nm is comparable with that of [Cu(Phen)
(
POP)]BF
4
[8], which means that the energy gap of [Cu(Phen-Np-
is similar with that of [Cu(Phen)(POP)]BF due to
performed on the Cu(I) complex, which has been demonstrated to
be an effective method to explore the electronic structure of transi-
tion metal complexes [8–10]. The percentage compositions of fron-
tier orbitals and the first five singlet excitation of [Cu(Phen-Np-
Et)(POP)]BF
4
4
naphthalene moiety’s inefficient conjugation with Phen ring.
The emission decay curves shown by the inset of Fig. 4 suggest
that the excited state of [Cu(Phen-Np-Et)(POP)]BF
lifetime of 287 s under pure N atmosphere, which identifies
the phosphorescence nature of the emission. Bearing above calcu-
lation results in mind, we conclude that the emission is generated
from MLCT excited state. A long-live excited state may give energy
acceptors enough time to attack and quench the excited state,
favoring sensitivity improvement and instant response [9].
Then, the potential surface crossing (PSC) from higher
state to lower MLCT state of [Cu(Phen-Np-Et)(POP)]BF
cussed as follows. As shown by the inset of Fig. 4, the emission un-
der pure N atmosphere follows a biexponential decay pattern
with = 380 s (A = 0.642) and = 80 s (A = 0.420), respec-
tively. It is reported that the observation of strong absorption in
p
p
+
4
has a long
Et)(POP)] are summarized in Table 2. The graphic presentation of
l
2
HOMO and LUMO shown in Fig. 2 suggests that HOMO of [Cu
+
(
Phen-Np-Et)(POP)] mainly localizes on Cu(I) center and P atoms,
⁄
while its LUMO is mainly composed of
p
orbital of Phen-Np-Et,
3
which is consistent with literature report [8–10]. The first electronic
transition is assigned as an electronic transition from HOMO to
LUMO, which confirms that the onset electronic transition of [Cu
⁄
p ? p
(
Phen-Np-Et)(POP)]BF
4
is a MLCT one. As shown in Table 2, LUMO
⁄
4
is dis-
is essentially
p
orbital of Phen-Np-Et ligand, and the excited state
electron localizing on LUMO may thus be attacked and quenched
by energy acceptors such as molecular oxygen, leading to a decrease
or even absence of emission intensity.
2
s
1
l
1
s
2
l
1
⁄
⁄
?
?
p
p
absorption region and a short-lived decay component from
state than those from MLCT state suggests an efficient PSC
Photophysical properties of [Cu(Phen-Np-Et)(POP)]BF
4
⁄
from the higher
p
?
p
state to MLCT state. The absorption spec-
The UV–Vis absorption spectrum of [Cu(Phen-Np-Et)(POP)]BF
4
trum of [Cu(Phen-Np-Et)(POP)]BF
4
shown in Fig. 3 exhibits a strong
is as-
ꢀ4
⁄
in CH
2
Cl
2
solution with a concentration of 1 ꢃ 10 mol/L is shown
absorption at
signed to
Under pure O
to 0.2 s, which is over 1000 times shorter than that under pure N
atmosphere. The largely decreased lifetime suggests that [Cu
(Phen-Np-Et)(POP)]BF excited state can be easily quenched by
p
?
p
absorption region. Consequently,
is assigned to MLCT decay.
atmosphere, the excited state lifetime decreases
s
2
⁄
in Fig. 3, along with those of free Phen-Np-Et ligand and POP ligand
for comparison purpose. The absorption spectrum of [Cu(Phen-
p ? p decay, and s
2
2
Np-Et)(POP)]BF
4
is mainly composed of two regions, ending at
l
2
ꢁ
460 nm. After the absorption spectrum comparison between free
ligands and [Cu(Phen-Np-Et)(POP)]BF
ing from 220 nm to 325 nm is assigned to ligand
4
, the strong absorption rang-
4
⁄
p
?
p
transitions,
molecular oxygen through a dynamic mechanism described as fol-
lows [7]:
while the weak absorption ranging from 350 nm to 450 nm is tenta-
tively attributed to MLCT transitions. After a comparison between
ꢅ
þOꢅ
½
CuðPhen-Np-EtÞðPOPÞꢄBF þO
2
!½CuðPhen-Np-EtÞðPOPÞꢄBF
4
4
2
absorption spectra of [Cu(Phen)(POP)]BF
throline) and [Cu(Phen-Np-Et)(POP)]BF , the MLCT absorption of
Cu(Phen-Np-Et)(POP)]BF
red shifts by ꢁ10 nm, owing to the large
4
(Phen = 1,10-phenan-
ð1Þ
4
[
4
⁄
where ‘‘ ’’ denotes excited state.
coplanar conjugation system in Phen-Np-Et ligand [8]. However, the
redshift tendency is limited, which may be caused by the conjuga-
tion break between naphthalene moiety and Phen ring, owing to
the free rotation of naphthalene moiety as mentioned above.
4
Characterization of [Cu(Phen-Np-Et)(POP)]BF /PS and [Cu(Phen-Np-
4
Et)(POP)]BF /MCM-41
Since its has been above confirmed that [Cu(Phen-Np-Et)
POP)]BF emission is quenchable by molecular oxygen, we decide
Table 2
(
4
Orbital percentage composition of [Cu(Phen-Np-Et)(POP)]+ calculated at RB3LYP/
SBKJC level.
to further explore its oxygen-sensing performance. For practical
sensing systems, optical probes should be embedded into support-
ing matrix to eliminate self-quenching of optical probes and to
allow analyte transportation from surrounding. There are also
some stringent criteria for supporting matrix to achieve suitable
performances [7]. Here, we select PS and MCM-41, which have
been proved to be excellent supporting materials for optical sen-
sors, as the supporting matrixes for our primitive research [7,15].
At first, three dopant concentrations of 3.0 wt.%, 3.5 wt.% and
Orbitals/
transition
Composition (%)
Energy
(eV)
LUMO + 1(174)
LUMO(173)
HOMO(172)
HOMO ꢀ 1(171)
Phen-Np-Et(93.5)
ꢀ3.935
ꢀ4.291
ꢀ7.701
ꢀ8.003
Phen-Np-Et(84.7) and POP(11.7)
Cu(28.6) and POP(65.4)
Cu(26.6) and Phen-Np(58.2) and
POP(15.3)
HOMO ꢀ 2(170)
HOMO ꢀ 3(169)
Cu(22.3) and Phen-Np(65.2) and
POP(12.3)
Cu(34.6) and Phen-Np(21.2) and
POP(44.2)
ꢀ8.038
ꢀ8.226
4
.0 wt.% are tried to achieve optimal performance. A typical SEM
image of the 3.5 wt.% doped sample is shown in Fig. 5a. [Cu
Phen-Np-Et)(POP)]BF /PS sample shows smooth and uniform
(
4
S
0
S
0
S
0
S
0
S
0
? S
? S
? S
? S
? S
1
2
3
4
5
171 ? 173(60.4) and 170 ? 173(34.5)
172 ? 173(96.3)
169 ? 173(94.7)
172 ? 174(96.8)
171 ? 174(63.2) and 170 ? 174(34.3)
2.7401
2.8074
3.0747
3.1468
3.2716
morphology with average diameter of ꢁ500 nm. The fibers are ran-
domly distributed on the substrate without any branch structures,
and this unique morphology has been reported to own a large sur-
face-area-to-volume ratio that is two orders of magnitude larger