Timothée Stoerkler‡
a,
Gilles Ulricha,
Adèle D. Laurentb,
Denis Jacquemin
*bc and
Julien Massue
*a
aInstitut de Chimie et Procédés pour l'Energie, l'Environnement et la Santé (ICPEES), UMR CNRS 7515, Equipe Chimie Organique pour la Biologie, les Matériaux et l'Optique (COMBO), 25 Rue Becquerel, 67087 Strasbourg Cedex 02, France. E-mail: massue@unistra.fr
bNantes Université, CNRS, CEISAM UMR CNRS 6230, F-44000 Nantes, France. E-mail: Denis.Jacquemin@univ-nantes.fr
cInstitut Universitaire de France (IUF), F-75005 Paris, France
First published on 21st July 2025
This article describes the synthesis, along with comprehensive photophysical and ab initio characterization, of a series of 2-(2′-hydroxyphenyl)benzoxazole (HBO) fluorophores, a family of compounds prone to undergoing an excited-state intramolecular proton transfer (ESIPT) process, functionalized with different positional isomers of quinoline or isoquinoline. We notably show that the position of the nitrogen atom at the azaheterocycle site has a key influence on both the emission profile and the photoluminescence quantum yield in solution. We also demonstrate the proton-sensitive nature of these dyes in solution, where not only does protonation trigger fluorescence enhancement, but it also acts as a transition switch between two excited states, with different emission profiles. HBO-isoquinoline displays very intense fluorescence not only in neutral and protonated dichloromethane solutions in the green-yellow region, but also in the solid state. Moreover, this dye exhibited a record Stokes shift of 11000 cm−1.
ESIPT implies a major reorganization of the electronic cloud in the molecular scaffold, eventually leading to a low-lying K* state, responsible for a redshifted K* fluorescence (Fig. 1a). ESIPT is indeed characterized by important Stokes’ shifts, in the 8000–10000 cm−1 range, a feature highly beneficial for applications where reabsorption processes and related inner-filter effects hamper the use of fluorescent organic scaffolds presenting a significant overlap between the absorption and emission spectra.3 Moreover, ESIPT can compete with other processes in the excited state such as proton abstraction, leading, in basic or dissociative media, to highly emissive anionic species (D* state).4 All these excited-state dynamical processes have nonetheless detrimental effects on the overall performance of fluorescent dyes, as efficient non-radiative pathways tend to decrease the fluorescence intensity of ESIPT dyes in solution; the photoluminescence quantum yields (QYs) of unsubstituted HBX dyes are typically in the 0.01–0.03 range, due to an accessible conical intersection (CI), corresponding to the twisting of the molecule after proton transfer.5 The access to this CI can be significantly hampered in the solid state, making ESIPT fluorophores attractive solid-state emitters, contrasting with the majority of molecular dyes where aggregative processes open non-radiative channels.6 ESIPT dyes have therefore been largely used for their solid-state luminescence properties7 and applied in optoelectronic devices,8 as laser dyes9 or embedded in various luminescent displays.10
Dual solution–solid emission (DSSE) corresponds to a highly sought-after property of some fluorophores which display intense luminescence both in solution and in the solid state.11 DSSE has emerged as an attractive area of research, due to the large array of applications targeted by these dyes, in the fields of materials science and biology.12 ESIPT dyes that already exhibit strong emission in the solid state are naturally attractive candidates for DSSE engineering, provided a reduction of non-radiative deactivation processes in solution is obtained.13 Some solution-emissive ESIPT compounds are known, involving limited access to the CI owing to molecular rigidity enhancement14 or the insertion of electron-withdrawing substituents onto the molecular scaffold.15 We16 and others17 have detailed another strategy to promote fluorescence intensity in solution, based on the concept of resonance-enhanced emission.18 A recent example involves a pyridine-substituted 2-(2′-hydroxyphenylbenzoxazole) (HBO) fluorophore. In neutral media, this dye undergoes deprotonation in lieu of ESIPT, thanks to the electron-withdrawing nature of the pyridine ring. An excited anion is formed with a QY of 0.12 (Fig. 1b). When protons are present, a pyridinium is formed, impeding deprotonation and leading to K*, formed by ESIPT, and presenting enhanced electronic delocalization. This merocyanine-type excited species is highly emissive (QY = 0.55) in solution and its excited-state energy level can be fine-tuned by chemical substitution.19
One drawback of this pyridine substitution on HBO lies in the emission wavelength observed, in either neutral or protonated media, below 500 nm, which impedes the use of these highly emissive compounds for biological applications, which require emission within the so-called biological window, where the absorption by biological tissues is minimal. One way to redshift the emission wavelength of the resonance-stabilized ESIPT emission would be to substitute pyridine for quinoline or isoquinoline analogs (Fig. 1c). Indeed, increasing the length of the excited merocyanine through longer π-delocalization is expected to stabilize the LUMO, leading to a significant bathochromic shift of the fluorescence wavelength.20 Notably, a recent example emphasizes that the replacement of a pyridine with a quinoline analog on an imidazole core leads to red shifts of both the absorption and emission wavelengths by up to 150 nm.21
In this contribution, we report synthetic efforts to introduce a quinoline ring onto the HBO scaffold, along with a full investigation of the photophysical properties in solution and in the solid state. Moreover, the nature of the observed transitions is rationalized and discussed using first-principles calculations.
![]() | ||
Scheme 2 Synthesis of HBO quinolines and isoquinoline via Pd-catalyzed cross-coupling between HBO-Br and Bpin derivatives 1–4. |
While HBO-5-quino was obtained with a good yield of 68%, other quinoline or isoquinoline isomers HBO-4-quino and HBO-6-isoquino were obtained in only 16 and 17% yields. Moreover, the formation of HBO-6-quino was not observed under these coupling conditions. These low yields can be tentatively explained by the poor reactivity of (iso)quinolines 1–4, whose carbon adjacent to boron features a weak electron density due to the electron-withdrawing nature of the (iso)quinoline group.
Reversing the nature of the coupling partners in the Suzuki cross-coupling, i.e., using commercial brominated (iso)quinolines with reported HBO-Bpin, under modified coupling conditions (Pd(dppf)Cl2 with potassium phosphate in a toluene/H2O mixture) led to the access of all desired (iso)quinoline targets in 53 to 78% yields (Scheme 3). The molecular structures of all these compounds were confirmed by 1H and 13C NMR spectroscopy and HR-MS (Fig. S1–S16†).
![]() | ||
Scheme 3 Synthesis of HBO quinolines and isoquinoline via Pd-catalyzed cross-coupling between HBO-Bpin and Br-quinolines or isoquinoline. |
HBO | Solvent/solid | λabs![]() |
ε (M−1 cm−1) | λem![]() |
Φf![]() |
Δss![]() |
σ (ns) | Kr![]() |
Knr![]() |
---|---|---|---|---|---|---|---|---|---|
a Maximum absorption wavelength (C = 10−5 M).b Maximum emission wavelength recorded at 25 °C (C = 10−6 M for solution measurements).c Quantum yield in solution, using rhodamine 6G as a reference (λexc = 488 nm and Φ = 0.88 in ethanol); quantum yield in the solid state, as absolute (calculated with an integration sphere).d Stokes shift.e kr (108 s−1) and knr (108 s−1) were calculated using kr = ΦF/τ and knr = (1 − ΦF)/τ, where τ is the lifetime.f Excitation wavelength. | |||||||||
HBO-Pyr | CH2Cl2 | 332 | 14![]() |
497 | 0.12 | 10![]() |
3.4 | 0.4 | 0.26 |
CH2Cl2/H+ | 330 | 29![]() |
490 | 0.55 | 9900 | 3.5 | 0.16 | 0.13 | |
Solid | 330f | — | 496 | 0.38 | 10![]() |
— | — | — | |
HBO-4-quino | CH2Cl2 | 326 | 18![]() |
504 | 0.12 | 10![]() |
1.5 | 0.08 | 0.59 |
CH2Cl2/H+ | 360 | 15![]() |
560 | 0.08 | 9900 | 1.7 | 0.05 | 0.53 | |
Solid | 364f | — | 517 | 0.39 | 8100 | — | — | — | |
HBO-5-quino | CH2Cl2 | 328 | 16![]() |
513 | 0.04 | 11![]() |
0.9 | 0.05 | 1.10 |
CH2Cl2/H+ | 333/379 | 17![]() |
500/671 | 0.01 | 6400 | 7.7 | 0.01 | 0.13 | |
Solid | 367f | — | 510 | 0.44 | 7600 | — | — | — | |
HBO-6-quino | CH2Cl2 | 335 | 21![]() |
523 | 0.12 | 10![]() |
1.4 | 0.09 | 0.63 |
CH2Cl2/H+ | 341/377 | 20![]() |
510/624 | 0.07 | 6900 | 0.9 | 0.08 | 1.03 | |
Solid | 371f | — | 531 | 0.50 | 8100 | — | — | — | |
HBO-6-isoquino | CH2Cl2 | 340 | 12![]() |
544 | 0.21 | 11![]() |
2.1 | 0.10 | 0.38 |
CH2Cl2/H+ | 344 | 23![]() |
548 | 0.79 | 10![]() |
3.5 | 0.22 | 0.06 | |
Solid | 374f | — | 525 | 0.40 | 7700 | — | — | — |
In neutral dichloromethane, all HBO (iso)quinoline dyes exhibit a low-lying S0–S1 absorption band located between 326 and 340 nm with absorption coefficient ε values between 12800 and 21
500 M−1 cm−1 (Fig. 2a and b). Interestingly, HBO-6-isoquino is the most redshifted in the series (λabs = 340 nm) with the lowest ε value (ε = 12
800 M−1 cm−1). Protonation of the dichloromethane solutions by bubbling HClg leads to the formation of the quinolinium analogs of all dyes, which triggers the appearance of a new bathochromically shifted absorption band (λabs = 344 to 377 nm; ε = 15 to 23
000 M−1 cm−1). In a neutral medium, the absorption spectra of all (iso)quinoline dyes are in the same range as that of HBO-Pyr, but after protonation, they all show a redshifted absorption band as compared to the pyridine analogue (Fig. 2c and d).
Photoexcitation in the S0–S1 band yields a single intense emission band in neutral dichloromethane solution, observed between 500 and 560 nm with QY values in the 0.04–0.21 range. These emission wavelengths are all redshifted compared to the reference HBO-Pyr (λem = 497 nm and QY = 0.12). HBO-6-isoquino is the most redshifted fluorophore of the series, along with the highest QY value (0.21).
It was previously reported that the emission of HBO-Pyr in neutral dichloromethane likely arose from an anionic excited species D*, although it was not entirely possible to rule out the possibility of emission from the K* state, as it was uneasy to distinguish between these two transitions.16,19 This analysis was based on significant changes in its optical profile after protonation and was consistent with the results of ab initio calculations. Compared to HBO-Pyr, the quinoline analogs show significant changes in their emission profiles in the presence of protons. Notably, upon protonation, the maximum emission wavelengths of HBO-4-quino and HBO-6-isoquino undergo bathochromic shifts to different extents (λem = 560 vs. 504 nm for HBO-4-quino and 548 vs. 544 nm for HBO-6-isoquino in the protonated vs. the neutral state, respectively), underlining the significant influence of the nature of (iso)quinoline positional isomers. Moreover, in their protonated state, while HBO-4-quino does not exhibit a drastic change in its fluorescence intensity (QY = 0.08 vs. 0.12), HBO-6-isoquino displays intense emission (QY = 0.79). In the latter case, the fluorescence band observed can be tentatively attributed to the decay of K*, stabilized by electronic delocalization (vide infra). In both cases, these two dyes display very large Stokes shifts, up to 11000 cm−1 (204 nm), which rank them among the organic fluorophores with the largest Stokes shifts, highlighting a major structural reorganization of the excited state.3a Upon protonation, HBO-5-quino and HBO-6-quino show different emission profiles with two distinct bands at 500/671 nm and 510/624 nm, respectively. Their QY values are, however, modest (0.01 and 0.07 for HBO-5-quino and HBO-6-quino, respectively). In protonated media, the formation of the quinolinium moiety impedes the emission of the anionic excited species D*, suggesting that the emission bands observed could be associated with the decay of E* and its tautomeric counterpart, K*, formed after ESIPT.
One can easily and visually notice in Fig. 2c that only the emission intensity of HBO-6-isoquino drastically increases upon protonation of the dichloromethane solution, going from 0.21 to 0.79. We cautiously interpret this significant enhancement of the fluorescence as arising from the resonance stabilization of the excited keto species, formed after ESIPT (Fig. 2f). The π-delocalization in the K* form enables the formation of a quinoidal species, which is likely less prone to the out-of-plane motions leading to a CI structure. For all other positional isomers, it is possible to rationalize the weak fluorescence intensity observed for HBO-4-quino and HBO-5-quino by the presence of detrimental steric interactions, leading to a rotation or a twist of the quinoline ring, hampering planarity and electronic delocalization and ultimately enhancing non-radiative deactivation (Fig. 2e). In the case of HBO-6-quino, the radiative deactivation constant Kr is much lower than that of its HBO-Pyr counterpart and vice versa for the nonradiative deexcitation constant Knr. This reflects a less stabilized, excited state mesomeric form. This could simply be due to the position of the nitrogen in the azaheterocycle, at the “pseudo para” position unfavorable for delocalization.
The optical properties of all (iso)quinoline HBOs were also measured in the solid state as powders (Fig. 3). They all display an intense single emission band ranging from 510 to 531 nm, redshifted with respect to HBO-Pyr. The QY values (0.39 to 0.50) are in line with those observed for the pyridine-substituted HBO series.19
It is noteworthy that HBO-6-isoquino displays very attractive features: intense fluorescence both in dichloromethane solution (λem = 544 nm and QY = 0.21) and in the solid state as powder (λem = 525 nm and QY = 0.40) with a very large Stokes shift in both media (11000 cm−1). Moreover, HBO-6-isoquino is very sensitive to protonation stimuli, triggering a transition switch in the presence of protons. The formation of the isoquinolinium moiety indeed translates into a very important enhancement of fluorescence intensity (0.21 to 0.79), with a similarly large Stokes shift.
To further characterize these systems, we used ab initio calculations, using the same protocol as the one we recently applied for pyridine-substituted HBO derivatives.19 This protocol combines TD-DFT for the structures and a post-HF approach (CC2) for the energies. The electron density difference (EDD) plots are presented in section S3.2,† for the absorption of both neutral and protonated dyes. For the neutral compound, these plots show a classical topology for ESIPT dyes, i.e., a hydroxyl group losing density upon excitation, indicating an increase of acidity in the excited state, a configuration obviously favorable for proton transfer. The topology changes drastically after protonation, since the lowest excited state becomes a clear charge transfer state, with the pyridinium/isoquinolinium acting as an electron acceptor and the phenol as an electron donor. Such trends are consistent with our previous works.16,19 The topologies of the EDDs are not much affected by the nature of the substituent in the investigated series.
Table 2 lists the key results of the theoretical simulations. It should be recalled that vertical transition values are not equivalent to observed λmax (or λem), which is why we mainly focus on the trends and orders of magnitude in the following discussion. For absorption, one can note that we compute vertical transition energies that are similar within the series for the neutral forms, whereas protonation induces bathochromic shifts that are significantly larger for the (iso)quinolinium than the pyridinium dyes. All these trends are consistent with experimental findings (vide supra).
HBO | Form | λvert-abs (E) (nm) | λvert-fl (E*) (nm) | λvert-fl (K*) (nm) | λvert-fl (D*) (nm) | ΔSS (E*) (cm−1) | ΔSS (K*) (cm−1) | ΔSS (D*) (cm−1) | ΔG (K*–E*) (eV) |
---|---|---|---|---|---|---|---|---|---|
HBO-Pyr | Neutral | 309 | 360 | 467 | 450 | 4584 | 10![]() |
10![]() |
−0.24 |
Protonated | 353 | 414 | 500 | — | 4174 | 8328 | −0.20 | ||
HBO-4-quino | Neutral | 309 | 360 | 466 | 529 | 4584 | 10![]() |
13![]() |
−0.23 |
Protonated | 393 | 480 | 637 | — | 4611 | 9746 | −0.11 | ||
HBO-5-quino | Neutral | 312 | 367 | 473 | 600 | 4803 | 10![]() |
15![]() |
−0.21 |
Protonated | 390 | 588 | 859 | — | 8634 | 14![]() |
−0.01 | ||
HBO-6-quino | Neutral | 316 | 373 | 487 | 532 | 4835 | 11![]() |
12![]() |
−0.24 |
Protonated | 391 | 514 | 663 | − | 6120 | 10![]() |
−0.07 | ||
HBO-6-isoquino | Neutral | 316 | 375 | 486 | 507 | 4978 | 11![]() |
11![]() |
−0.23 |
Protonated | 368 | 496 | 701 | — | 7013 | 12![]() |
−0.04 |
Let us now turn towards fluorescence in neutral dichloromethane. For HBO-Pyr, theory provides a large driving force of −0.24 eV for the ESIPT process together with an emission wavelength of 360 nm for the E* form, clearly not compatible with experimental outcomes (emission at 497 nm with a very large Stokes shift). Therefore, consistent with previous studies,16,19 the observed emission would likely arise from the D* transition, although K* cannot be ruled out. Note that these spectral variations are accompanied by significant structural changes. In HBO-Pyr, the dihedral angle between the pyridinium and the phenol is 36° in the ground electronic E state, and it decreases to 27°, indicating stronger conjugation in the excited state (K*). Protonation decreases these values to 31° (E ground state) and 19° (K* excited state), which is consistent with the topology of the EDD, indicating a strong interaction between the two rings when the pyridinium is formed.
For all the other dyes, theory also predicts similarly large free energy differences between the enol and keto forms, allowing the exclusion of the presence of E* emission in all cases. Interestingly, theory predicts the anionic (D*) emission to be redshifted as compared to its K* counterpart in all (iso)quinoline derivatives, whereas the reverse was found in HBO-Pyr. For HBO-5-quino, the D* fluorescence is predicted at 600 nm, redshifted by more than 125 nm compared to HBO-Pyr, a trend that is not seen experimentally (Fig. 2b). Therefore, we can conclude that the fluorescence of HBO-5-quino is a pure K* one. The same holds for both HBO-4-quino and HBO-6-quino, which exhibit fluorescence, respectively, blueshifted and redshifted by ca. 10 nm as compared to HBO-5-quino experimentally (Table 1). This trend nicely fits the computed K* fluorescence wavelengths, but would be rather incompatible with D* fluorescence. Finally, we cannot definitively attribute the observed emission of HBO-6-isoquino (at 544 nm) to the D* or K* forms, although relative comparisons with the other compounds tend to hint at D* fluorescence.
Of course, the structure of the dye influences its geometry. For instance, in the ground E state (K* form) HBO-5-quino shows a dihedral angle of 53° (43°) between the quinoline and the phenol, due to the obvious steric clash appearing between the two cycles in that compound. In contrast, in HBO-6-isoquino, this angle amounts to 38° (21°), since the configuration allows for improved coplanarity.
In the presence of protons, the D* fluorescence cannot be observed. In this context, for HBO-Pyr, it is clear that the experimental fluorescence corresponds to the K* form since the computed ESIPT driving force remains large (−0.20 eV), and only the computed K* emission produces a Stokes shift comparable with the measurements. In both HBO-5-quino and HBO-6-quino, two bands are observed experimentally corresponding to a dual E*/K* emission. We note that in these two compounds, the ESIPT driving force is strongly reduced after protonation, leading to small negative ΔG of −0.01 and −0.07 eV, indicating that the K* form is only slightly more stable than its E* counterpart, which fits the presence of dual emission.22 Obviously for the former compound, theory strongly overestimates the emission wavelengths of the two forms, yet errors of ca. 0.4 eV remain, which are large but not impossible at the selected level of theory. The observed emission in CH2Cl2/H+ HBO-4-quino is in between the two bands observed for both HBO-5-quino and HBO-6-quino, which clearly points at K* emission. We note that the driving force for ESIPT in (protonated) HBO-4-quino is also larger than those in the other two compounds, consistent with this assignment. Finally, for protonated HBO-6-isoquino, the experimental emission wavelength remains mostly unchanged as compared to the neutral form and, according to calculations, this would better fit a computed E* emission, with a large Stokes shift explained by a strong CT character. However, a K* transition, characterized by a resonant quinoidal structure, would be closer to what was evidenced for the pyridine analog, HBO-pyr, and cannot be ruled out in our opinion.
Footnotes |
† Electronic supplementary information (ESI) available: 1H and 13C NMR spectra, details of the computational procedures and methods, and EDD plots for all compounds. See DOI: https://doi.org/10.1039/d5qo00639b |
‡ Present address: University of Ottawa, Department of Chemistry, D'Iorio Hall, 10 Marie Curie, Ottawa ON Canada, K1N 6N5 |
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