2. Results and Discussion
Figure 1 shows the steady-state absorption and fluorescence spectra of
Al2O3:OHCCAfree and
Al2O3:OHCCAagg films. In the absorption spectrum of
Al2O3:OHCCAfree, the lowest energy transition band near 420 nm appears only when OHCCA is covalently adsorbed on Al
2O
3 film (see
Figure S1 for the non-binding case). This means that the chemisorption induces a strong electronic delocalization along the binding structure between the dye and metal oxide. The transition band shows a hypsochromic shift to 410 nm in
Al2O3:OHCCAagg as the number density of the dyes increases. The well-stacked geometry of the dyes on the film enhances the band’s blue shoulder which corresponds to the dipole-allowed transition for H-type aggregates. On the contrary, the higher energy absorption band at around 360 nm exhibits a bathochromic shift in the aggregates. Note that the direction of the transition dipoles for the S
1←S
0 absorption band is parallel to the long axis of the coumarin backbone, whereas it is rather perpendicular to the principal axis for the S
2←S
0 absorption band (see
Figure S2 for the quantum calculation). This may indicate that the origin of the absorption at 360 nm is the S
2←S
0 transition band and J-type interactions between the dyes are favorable in the film.
Figure 1b shows the steady-state fluorescence spectra of the films where the excitation wavelength at 400 nm could populate the lowest excited state exclusively (
vide infra). Compared to
Al2O3:OHCCAfree, the well-stacked OHCCA in
Al2O3:OHCCAagg exhibits further Stokes shift with a noticeable second vibronic band at 500 nm, indicating a hint of the excimer formation in the aggregates. It is well known that the π–π stacked geometry of dyes in a confined space can induce prominent vibronic features with a large displacement [
9,
10]. Hence, the well-stacked dyes with vertically oriented transition dipoles can cause an efficient excimer formation with the characteristic fluorescence spectrum.
The ambiguity in the assignment of the absorption at 360 nm led us to measure the steady-state two-dimensional (2D) fluorescence spectra. The OHCCA films showed unusual behaviors in radiative relaxations from their excited states. When the excitation wavelength (λ
ex) varied in the range of 350~400 nm, two emission bands appeared near 400 and 450 nm in both film samples (
Figure 2a). The higher energy band gradually grew as λ
ex became shorter, while the emission band at 450 nm, which corresponds to the lowest electronic transition (A→GS), was dominant at λ
ex > 400 nm. The emission band near 400 nm (B→GS) was not attributable to non-binding OHCCA dyes that do not interact with the Al
2O
3 surface because a solvent wash removed the non-binding dyes on the films in the sample preparation. The apparent absorption band at 420 nm also confirmed that the OHCCA dyes on the films interact with the Al
2O
3 surface (
Figure 1a). Therefore, the emission band abnormally observed near 400 nm may be related to the S
2→S
0 fluorescence, implying a breakdown of Kasha’s rule. It is well known that the azulene molecule has an exceptionally large energy gap of about 1.7 eV (~13,700 cm
−1), and so the internal conversion becomes slow because of the poor Franck–Condon factor [
11]. For
Al2O3:OHCCAfree, however, the estimated energy gap between the two electronic states was about 0.45 eV (3630 cm
−1) (see
Figure 2b, top), indicating that the gap was not large enough to induce the dual emission involving the S
2→S
0 fluorescence. In fact, the azulene derivative with an energy gap of about 4300 cm
−1 showed only the S
1→S
0 fluorescence at room temperature [
12]. Therefore, it is reasonable to conclude that Kasha’s rule is still valid in both
Al2O3:OHCCAfree and
Al2O3:OHCCAagg films.
The fluorescence excitation spectra monitored at λ
em = 400 nm revealed a well-separated B←GS transition band at 360 nm (
Figure 2b). As λ
em became longer, an additional band corresponding to the A←GS transition appeared near 420 nm in both film samples. Compared to
Al2O3:OHCCAfree, the excitation spectrum of
Al2O3:OHCCAagg monitored at λ
em = 460 nm exhibited a dramatically intensified and slightly blue-shifted A←GS transition band with the B←GS transition band being red-shifted (see vertical dashed lines in
Figure 2b). This is consistent with the absorption measurements shown in
Figure 1a. The enhanced A←GS transition is mainly due to the effective H-type interaction on the film, thereby increasing the oscillator strength for the dipole-allowed transition.
On the other hand, the shoulder of emission at 400 nm (B→GS) was not attributed to the S
2-S
0 transition but may be due to the excitonic splitting of the lowest excited state (S
1). Note that two excitation bands at 360 and 420 nm show the opposite shifting behaviors when OHCCA forms the aggregate on the surface of Al
2O
3 (see
Figure 2b). In the aggregates, one can attribute the H-type excitonic coupling to account for the hypsochromic shift of the lowest absorption band at 420 nm. However, the opposite behavior of the band at 360 nm is still counterintuitive. Instead, we assume the other possibilities on the origin of the B→GS transition: (1) the impurity of the OHCCA molecule and (2) structural heterogeneity via the various adsorption modes of a carboxylic acid group.
M. Z. Shafikov et al. reported that the origin of the dual emission of a coumarin derivative (C-2) in the solution is the impurity that is one of the synthetic intermediates [
13]. The authors confirmed that C-2 has an energy gap (S
2-S
1) of about 4000 cm
−1, and the purified C-2 does not show any dual fluorescence. Although this is similar to the case of the OHCCA on film, the impurity of OHCCA should be negligible: only the
Al2O3:OHCCA films exhibited the dual emission while the drop-casted film (the non-binding dye) did not show any additional band at 450 nm as shown in
Figure S1. Y. Gao et al. reported that three anchoring modes of retinoic acid, which contain a carboxylic acid group adsorbed on TiO
2, reveal different absorption transitions [
14]. They showed that the distance between a dye and the surface of the metal oxide after the formation of the H–bond significantly affects the coupling between the dye’s excited state and the conduction band states of the semiconductor. Therefore, it is reasonable to assume that the electronic transitions of OHCCA anchored on the surface of the Al
2O
3 film are strongly dependent on the anchoring mode of the carboxylic acid group. Moreover, different anchoring modes of a carboxylic acid group on the surface of Al
2O
3 might be responsible for the dual emission and the opposite shifting behaviors of the corresponding absorption bands.
The electronic transition pathways in the film samples are summarized in
Figure 3. In
Al2O3:OHCCAfree, the bidentate binding mode (A) causes the strongest orbital mixing to give the lowest electronic transition at 420 nm. The monodentate binding mode (B) with/without an H–bond reveals the tilted binding geometry on the surface of Al
2O
3, which induces relatively weak orbital mixing to give a higher electronic transition at 360 nm [
14]. As a result, the dual emission can be ascribed to the mixture of OHCCA with different anchoring modes. In
Al2O3:OHCCAagg, the monodentate binding geometry is heterogeneous in terms of the intermolecular orientation, i.e., the co-facial stacking interaction is less probable in randomly oriented geometry. The van der Waals interactions between weakly coupled dyes are expected, and it can stabilize the excited state of OHCCA (B) to give the red-shifted absorption near 360 nm (see
Figure 1). Accordingly, only some portion of the aggregate with the bidentate binding one reveals the well-stacked assembly in the film. Influenced partly by the strong orbital coupling between the dye and Al
2O
3, the intermolecular interaction between the dyes in
Al2O3:OHCCAagg is effective enough to induce the excitonic splitting of the electronic transitions.
To elucidate the ultrafast reaction dynamics of the OHCCA aggregates without any perturbations from higher-lying excited states in the energy (B), we focused on the relaxation dynamics of the lowest excited state (A), employing time-resolved fluorescence (TRF) spectroscopy with 400 nm excitation.
Figure 4 displays the time-resolved emission spectra (TRES) of the film samples recorded by the time-correlated single photon counting (TCSPC) method with a time resolution of 50 ps (see
Figure S5 for the raw images). In
Al2O3:OHCCAfree, TRES slowly decay in intensity over 6 ns and show no dynamic Stokes shift with a large displacement. As shown in the inset of
Figure 4a, the first moment of TRES, which represents the center wavelength of the spectrum weighted by fluorescence intensity, does not change much for up to 6 ns. By contrast, the TRES of
Al2O3:OHCCAagg decays relatively fast during 1 ns with a gradual growth of the red shoulder at 500 nm (
Figure 4b).
The decay profiles of TRF at the maximum wavelength, 460 nm, clearly demonstrate faster decay components in
Al2O3:OHCCAagg (
Figure 5a). For a quantitative comparison, we used the maximum entropy method (MEM) to calculate the lifetime distributions from the fluorescence decay profiles of the film samples, as depicted in
Figure 5b. The MEM is commonly used to obtain the distribution of rates (or time constants) in the logarithm scale [
15]. In the lifetime distribution of
Al2O3:OHCCAfree, there are two bands in the time constants longer than 1 ns with a dominant one near 5 ns, indicating that isolated OHCCA on the film has a rigid structure and, thus, no fast relaxation processes via structural deformations such as the twisting motion are observed. However, in the lifetime distribution of
Al2O3:OHCCAagg, two prominent bands appear in the time constants shorter than 1 ns. Note that there are no ultrafast components shorter than 50 ps in the picosecond lifetime distribution. The excimer formation (or charge transfer exciton formation) is known to occur typically within a 1 ps time scale for the well-stacked perylene derivatives in a confined geometry [
5,
16]. In the aggregated sample, OHCCA dyes can effectively interact with each other in the 2D space to give the excitonic splitting in the absorption spectra, as shown in
Figure 1a. However, the time scale of about 100 ps observed in
Figure 5b is too long to represent the excimer formation of OHCCA dyes on the film. The femtosecond fluorescence up-conversion measurements could reveal an ultrafast decay with a time constant of 550 fs in the aggregated sample (
vide infra). That is, we can conclude that the ultrafast decay within 1 ps is drastically attenuated by the convolution-integral with the instrument response function (IRF) of about a 50 ps width, and the observed slow kinetics in the TCSPC experiment is rather related to any subsequent relaxation processes of a nascent excimer.
To elucidate the origin of the slow relaxation dynamics of
Al2O3:OHCCAagg, the picosecond TRES were further analyzed by the time-resolved area normalized emission spectra (TRANES). The TRANES is commonly used to identify the characteristic excited state dynamics of a dye without concerning any population decay in the excited state [
17].
Figure 6a displays the TRANES of
Al2O3:OHCCAagg, which has an iso-emissive point near 470 nm. This indicates that two independent emissive states are involved in the relaxation processes [
14]. Since an ultrafast decay component shorter than 1 ps cannot be resolved in the picosecond TRES, its contribution to the TRES is negligible. The intermolecular energy transfer occurring in the π-stacked OHCCA on the film may be related to the spectral shift, but we ruled out this possibility because a localization of coherent excitons might be ultrafast in the stacked aggregates [
18]. Moreover, the internal conversion from the S
2 state and the intramolecular vibrational relaxations (IVR) from the vibrationally hot band of the S
1 state are not responsible here because the excitation at 400 nm can populate the S
1 state exclusively (see
Figure 2), and the IVR process is ultrafast in a condensed phase [
19]. Therefore, it is reasonable to conclude that two independent emissive states in TRANES likely correspond to the nascent excimer in the lowest excited state and its subsequently relaxed form, which are observed beyond 100 ps and unrelated to the nascent excimer formation.
The time scale for the subsequent relaxation pathway can be determined by the evolution-associated spectra (EAS) analysis of the TRES image, as shown in
Figure 6b. Here, we implemented the first-order serial reaction scheme, E→E’→ground state (GS), in the global target analysis where E and E’ denote the nascent excimer and subsequently relaxed excimer, respectively. The best fit with a simple two-step model results in the time constants of 280 ps and 1.91 ns (see
Figure S6 for the detailed results). The shorter time constant (280 ps) represents the time scale of structural relaxation. Note that the MEM only gives a lifetime distribution for the decay profile recorded at a single wavelength so that the redundant lifetime band near 500 ps in
Figure 5b can be ascribed to the associated evolutions of two closely lying emissive states, not the actual population change.
For further investigations on ultrafast relaxation processes in the excited state, we measured the fluorescence up-conversion with a time resolution of about 100 fs (
Figure 7). It should be noted that the up-conversion signal of
Al2O3:OHCCAfree is very weak, as shown in
Figure 7a, due to the extremely low OHCCA concentration on the film. Nonetheless, no fast relaxation shorter than 20 ps was observed in the
Al2O3:OHCCAfree sample, which is consistent with the MEM analysis of the picosecond TRF shown in
Figure 5b. This strongly supports the fact that isolated OHCCA on the film undergoes no fast structural relaxations in the excited state and, therefore, shows no discernible dynamic Stokes shift in the picosecond TRES. On the other hand, an ultrafast decay shorter than 1 ps emerges in the up-conversion signal at 450 nm when the OHCCA dyes form H-type aggregates on the film. That is, the origin of the fast decay should be related to population relaxation dynamics occurring in the aggregates. Note that this component is dominant even at 525 nm in the emission band’s red shoulder (see
Figure S7). Since the TRES of the excimer is not fully separated in the energy from the TRES of the Franck–Condon state, the decay profiles recorded at a single wavelength can be complicated by the considerable spectral overlap, as depicted in
Figure 6b. Again, to quantitatively determine the rate of excimer formation, we employed the first-order reaction scheme, A→E→E’, where the A term denotes the Franck–Condon state of the OHCCA aggregate. As shown in
Figure 7b, the single decay profile is well described by the sum of A and E terms. The A term is dominant at both 450 and 525 nm, indicating that the excimer formation causes a sudden change in oscillator strength and reduces the emission intensity over the whole spectral range.
The overall reaction pathways for the excited state dynamics of
Al2O3:OHCCAagg are summarized in
Figure 8. Upon excitation to the Franck–Condon state at 400 nm, OHCCA in aggregate can immediately undergo excimer formation with a time constant of about 550 fs, as demonstrated by the fluorescence up-conversion experiments. After the nascent excimer formation, subsequent structural relaxations proceed with a time constant of 280 ps. Skeletal motions changing the intermolecular orientation and separation distance may be responsible for this structural reorganization.