Björn
Kriete
,
Carolien J.
Feenstra
and
Maxim S.
Pshenichnikov
*
Zernike Institute for Advanced Materials, University of Groningen, Nijenborgh 4, 9747AG Groningen, The Netherlands. E-mail: m.s.pchenitchnikov@rug.nl
First published on 21st April 2020
The bottom-up fabrication of functional nanosystems for light-harvesting applications and excitonic devices often relies on molecular self-assembly. Gaining access to the intermediate species involved in self-assembly would provide valuable insights into the pathways via which the final architecture has evolved, yet difficult to achieve due to their intrinsically short-lived nature. Here, we employ a lab-on-a-chip approach as a means to obtain in situ control of the structural complexity of an artificial light-harvesting complex: molecular double-walled nanotubes. Rapid and stable dissolution of the outer wall was realized via microfluidic mixing thereby rendering the thermodynamically unstable inner tubes accessible to spectroscopy. By measurement of the linear dichroism and time-resolved photoluminescence of both double-walled nanotubes and isolated inner tubes we show that the optical (excitonic) properties of the inner tube are remarkably robust to such drastic perturbation of the system's supramolecular structure as removal of the outer wall. The developed platform is readily extendable to a broad range of practical applications such as e.g. self-assembling systems and molecular photonics devices.
In this context, amphiphilically driven self-assembly is of special interest, as changing the relative strength and size of the hydrophobic/hydrophilic moieties allows fine-tuning the final supramolecular structure towards micelles, bilayer sheets or nanofibers.11–13 A notable example of one of such systems is a class of amphiphilic cyanine derivatives that are known to self-assemble in aqueous solution into highly homogenous, double-walled nanotubes with outer and inner diameters of ∼13 nm and ∼7 nm, respectively, and lengths on the order of several μm's.9 These systems comprise a large number of strongly coupled chromophores leading to the formation of delocalized excited stated (Frenkel excitons), which is considered promising for quasi-one-dimensional excitonic wires.14–16 The interest in such systems is further propelled by their structural resemblance of natural light-harvesting antenna complexes such as the chlorosomes of green sulfur bacteria.17–19
While the final, thermodynamically stable outcome of the self-assembly can be modified via molecular engineering of the initial building blocks and is readily accessible via a number of characterization techniques, the intermediate stages are much harder to target due to their short-lived nature as out-of-equilibrium species. Nevertheless, understanding these transient stages of the self-assembly process would not only provide great insight into how to steer the process into a certain (otherwise inaccessible) direction, but also shed light on the functional properties of intermediate species as simplified components of the more complex final assembly. One strategy that has successfully been used to gain access to out-of-equilibrium species of a self-assembly system relies on microfluidics.20,21 For instance, it has been used for real time monitoring22–24 and control25,26 of chemical reactions, following mixing reactions,27,28 steer molecular self-assembly29,30 and study (out-of-equilibrium) reactions in biological systems.31–33
In this paper, we use a lab-on-a-chip approach as a means to achieve out-of-equilibrium control over the structural hierarchy of an artificial light-harvesting complex: double-walled molecular nanotubes. Structural simplification of such nanotubes has previously been demonstrated in bulk solution by dissolving the outer tube via flash-dilution thereby exposing the bare inner tube for linear absorption spectroscopy.34,35 However, a rapid partial recovery of the original double-walled structure (within ∼60 s) leaves no time for more advanced and therefore informative spectroscopies. Here, we successfully transfer the flash-dilution technique to a microfluidic platform to achieve stable and continuous removal of the outer layer of the supramolecular assembly. Linear dichroism and time-resolved photoluminescence (PL) experiments demonstrated that the inner nanotube alone retains its excitonic functionality despite such drastic modifications of the supramolecular structure.
For spectroscopic measurements (linear dichroism and time-resolved PL) the (flash-diluted) sample solution was relayed to a second, thin-bottom flowcell (micronit, The Netherlands; borosilicate glass) with a channel thickness of 50 μm and a channel width of 500 μm connected by ∼15 cm of tubing (Teflon, channel diameter 250 μm). This flowcell allowed conducting spectroscopic experiments in transmission, as e.g. linear dichroism (vide infra) which was not possible in the micromixer because of the curved channel profile. Both the micromixer and the flowcell were used as received from the manufacturer without any additional surface treatment. Blockage of the channel or surface sticking of the sample were not observed, as these would have immediately been reflected in the gradual increase or decrease of the optical density of the sample.
For the measurements on the double-walled nanotubes, the diluting agent was replaced by Milli-Q water, operated at the same flow rate as in flash-dilution experiments. Under these conditions the maximum optical density of the sample solution was between 0.1 and 0.2 to avoid PL reabsorption.
The same peak assignment also holds for the PL spectrum (Fig. 1, short dashed line), where the reversed peak ratio (i.e., Iinner > Iouter) is a consequence of the equilibration of the exciton populations between both tubes on a sub-ps timescale prior to PL.39–41 The higher-frequency transitions are not observed in PL as they quickly (within ∼100 fs) relax to the two lowest-energy states.
Dissolution of the outer tube of double-walled nanotubes is achieved in a tear-drop micromixer (Fig. 2a) via mixing of the two parent reactants, i.e., a H2O/MeOH diluting agent (1:1 by volume), and nanotube sample solution. Efficient intermixing of the two reactants in the mixing zone of the micromixer is evident from the wide-field PL images superimposed with bright-field microscope images of the microfluidic channel. Here the laminar flow regime (Fig. 2b, top) and mixed phase (Fig. 2b, bottom) can clearly be distinguished. This rapid mixing induces flash-dilution during which the outer layer is dissolved from the double-walled nanotubes.34,35 Note that the PL signal after flash-dilution does not contain any contribution from dissolved C8S3 monomers, because their absorption is not in resonance with the excitation wavelength (λexc = 561 nm); see ESI,† Section S3 for results using a different excitation wavelength.
Fig. 2 Overview of microfluidic setup. (a) Schematic of the micromixer and flowcell used in this study. The flow direction of the sample is indicated by the white arrows. (b) Microscope images of two sections of the micromixer marked in panel (a). The upper and lower panels show the Y-junction before and the microfluidic channel behind the mixing zone, respectively. The bright-field microscope images (in black and white) are superimposed with wide-field excitation PL images following excitation at λexc = 561 nm; ESI,† Section S6. The wide-field excitation area is indicated by green circles in both panels. The bottom panel corresponds to a mixing time of ∼12 s. (c)–(e) Steady-state PL spectra (black dots) of double-walled nanotubes (top) and isolated inner tubes (center and bottom) following tightly focused excitation at λexc = 561 nm at the spots indicated in panel (b). The PL spectrum in panel (e) was obtained from streak camera measurements (spectral resolution 85 cm−1). The shaded peaks (red: inner tube; gray: outer tube) are obtained by fitting the PL spectra to a sum of two (black line) and a single Lorentzian lineshape(s) in the case of double-walled nanotubes and isolated inner tubes, respectively. Insets: Schematics of double and single-walled nanotubes, which illustrate the origin of the observed peaks in the PL spectra. |
After flash-dilution, the isolated inner tubes are in a thermodynamically unfavourable configuration, since the hydrophobic side-group are now directly exposed to the H2O/MeOH environment. This out-of-equilibrium configuration leads to a quick partial recovery of the outer tube on a timescale of tens of seconds via re-attachment of the dissolved monomers to the exterior of the isolated inner tubes. This process continues until a new equilibrium between monomers and nanotubes is established that is dictated by the solvent composition after flash-dilution (ESI,† Section S4). The longer-time (tens of minutes later) consequences of this process can be monitored using absorption spectroscopy (ESI,† Section S4) or cryo-TEM imaging (ESI,† Section S5). To the best of our knowledge, this re-assembly of the outer layer can neither be restricted nor halted. However, by using the microfluidics platform, it is possible to spatially separate the regions where the isolated inner tubes are continuously being produced, from the region where the outer layer starts to recover. This approach, thus, enables spectroscopy on the clean isolated inner tubes for which the attainable experimental time (i.e., supply time of isolated inner tubes) is only limited by the amount of sample solutions (up to ∼30 hours in practice). This way, microfluidic flash-dilution can also be interfaced with other, more advanced and often time-consuming types of spectroscopy, e.g., 2D spectroscopy.28,42
In order to verify the successful dissolution of the outer tube upon microfluidic flash-dilution we use the spectral band assignment in the steady-state nanotube PL spectra (Fig. 2c–e). These PL spectra prove that the high energy band (∼590 nm, 16950 cm−1) corresponding to the outer tube is almost completely eliminated after microfluidic mixing, while the spectral signature of the inner tubes (∼600 nm, 16670 cm−1) is preserved. The similarity of the PL spectra at the exit of the micromixer and in the thin-bottom flowcell (given lower spectral resolution in the latter case) proves negligible recovery of the outer layer in the relaying tubing. The weak shoulder on the blue flank (around ∼590 nm) of the inner tube PL spectrum (Fig. 2d and e) is due to a small number of residual undissolved parts of the outer nanotube layer.
Upon flash-dilution the PL peak of isolated inner tubes undergoes a small spectral blue-shift of about 50 cm−1 relative to the case of double-walled nanotubes. Such behaviour has also previously been reported for conventional ‘bulk’ flash-dilution experiments.34,35,42 We hypothesize that the sudden dissolution of the outer tube may lead to slight decrease of the inner tube radius and, consequently shift its absorption/PL spectrum. Substantial shortening of the nanotubes (down to sub-100 nm length, where the nanoconfinment effects are expected to occur43) can be excluded as the reason for this blue-shift, because no short fragments were found in PL microscopy images recorded directly after flash-dilution (ESI,† Section S6).
The exciton transition dipole moments associated with different peaks in the nanotubes’ absorption spectrum (Fig. 1d) have different alignment along the nanotube.10,34,37 This leads to linear dichroism in absorption (providing the nanotubes are aligned along a certain direction) which can be used as an indication for retaining the exciton properties upon flash-dilution. The nanotubes tend to flow-align in a microfluidics channel owing to their large aspect ratio (μm length versus ∼13 nm diameter); similar alignment effects have previously been observed for other systems.44–47 The reduced linear dichroism (LDr) spectra (Fig. 3) were obtained by recording the absorption spectra with light polarized parallel and perpendicular to the flow direction in the microfluidic channel; a detailed description of the experimental apparatus and data processing protocol is given in the ESI,† Section S1. The alignment of double-walled nanotubes along the flow is evident from the pronounced positive amplitude peaks in the LDr spectrum at the spectral positions of the outer (at ∼590 nm, 16950 cm−1) and inner tube (at ∼600 nm, 16670 cm−1) absorption peaks (Fig. 3a). This proves that the nanotubes efficiently flow-align despite the lower flow speeds reached in microfluidics as compared to conventional flow cuvettes.37 These data also reveal the mixed polarization character (i.e., both parallel and perpendicular) of the absorption peaks towards shorter wavelengths between 550 nm and 580 nm; both shape and amplitude of the measured LDr spectra agree remarkably well with previous findings.37
After flash-dilution the maximal LDr amplitude (of ∼2.1 ± 0.2; mean ± standard error) of the inner tube transition is retained (Fig. 3b), which shows that the excitonic character of the main absorption peak is preserved even upon complete removal of the outer tube. Strong alignment of the flash-diluted nanotubes along the flow direction also indicates that the nanotubes are not substantially shortened during flash-dilution. Unlike for double-walled nanotubes, any low amplitude LDr peaks occurring at shorter wavelengths cannot be distinguished given the signal-to-noise ratio of the data, which is limited by the low molar concentration of nanotubes after flash-dilution and the channel thickness of only 50 μm.
Next, we study the exciton dynamics of double-walled nanotubes and isolated inner tubes. Hereby, we utilize the fact that under intense laser excitation excitons start to mutually interact leading to exciton–exciton annihilation (EEA).48,49 The probability that two excitons are able to meet and consequently annihilate depends on the exciton density (i.e., the number of excitons per number of molecules; ESI,† Section S7) as well as the excitonic properties of the system, such as exciton delocalization and exciton diffusion. EEA then opens a new non-radiative (and intensity dependent) decay channel for excitons,50–52 which leads to acceleration of the observed PL dynamics. In multi-chromophoric systems excitons are collectively shared by many molecules so that it can be experimentally challenging to reach sufficiently low exciton densities to isolate the true response of single excitons, while avoiding EEA. In this regard, time-resolved PL offers unprecedented sensitivity down to extremely low exciton densities (as low as 1 exciton per ∼106 chromophores).
Fig. 4 shows the PL transients obtained by spectrally integrating the PL decay maps between 588–603 nm for double-walled nanotubes and 598–603 nm for isolated inner tubes (a schematic of the experimental setup and a few representative PL decay maps are shown in the ESI,† Sections S2 and S8, respectively). In the case of double-walled nanotubes, the PL transients of the inner and outer layer are identical, except for their different amplitudes, which is why only one set of PL transients is shown for both inner and outer tube. This observation is further corroborated by the fact that no spectral relaxation of the PL mean frequency is observed (ESI,† Section S8) at any excitation intensity. Had spectral relaxation on the timescale of PL been the case (due to e.g. ‘slow’ exciton transfer between the two tubes), the mean frequency would have dynamically shifted.53–55
At low exciton densities the PL of double-walled nanotubes (Fig. 4a) and isolated inner tubes (Fig. 4b) decays mono-exponentially with time constants of 43 ± 1 ps and 58 ± 1 ps, respectively. These time constants are independent of the excitation intensity, because the large average distance between the excitons – 1 exciton per ∼10 μm of nanotube length (containing 106 molecules) at the lowest intensity – prevents EEA. The observed increase of the lifetime of isolated inner tubes agrees well with previous spectro-chemical studies on nanotubes embedded in a sugar matrix,38 where the spectral response of the outer layer was quenched via oxidation with silver nitrate. We hypothesize that the presence of the outer layer may open an additional non-radiative decay channel for excitons and, thus, lead to a reduced PL lifetime in the case of double-walled nanotubes.
At high exciton densities, the PL transients of double-walled nanotubes and isolated inner tubes become increasingly multi-exponential, which is a typical fingerprint of EEA.48,52 After a rapid initial decay of the PL signal due to prominent EEA, the dynamics slow down as the surviving excitons become sparser and hence less likely to meet and annihilate. We will use these two time intervals to quantify the PL dynamics separately. In the first interval (up to 30 ps), we extract the PL lifetimes of double-walled nanotubes as well as isolated inner tubes by fitting the transients to a convolution of an exponential decay and a Gaussian apparatus function (as an approximation of the IRF; Fig. 4). In the second interval (30–150 ps), the tails of the PL transients are fitted to an exponential decay F(t) = Aexp(−t/τ). In both cases, the PL decay rate is determined as the inverse lifetime τ−1, normalized to the intrinsic (non-)radiative decay rate and plotted as a function of exciton density (Fig. 5a and b).
Fig. 5 Acceleration of PL dynamics. (a) and (b) experimental PL decay rates of double-walled nanotubes (black dots), isolated inner tube (red dots) and dissolved monomers (gray dots; ESI,† Section S9) as a function of exciton density in the first interval (−30 → 30 ps) and in the second interval (30 → 150 ps), respectively. The decay rates are normalized to the intrinsic (non-)radiative decay rate. The vertical error bars refer to the standard deviation of the respective fit. The horizontal error bars for the exciton density are obtained from propagation of uncertainty of all input parameters (ESI,† Section S7). Solid and dashed lines in panels (a) and (b) are derived from Monte-Carlo simulations. The solid black lines originate from the Monte-Carlo simulated transients (solid lines in Fig. 4). The dashed gray lines refer to the lower and upper limits of the acceleration of the PL decay (see main text for explanation); the region between these limits is shaded in gray for illustration. (c) Schematic representation of diffusion-assisted EEA on double-walled nanotubes (left) and isolated inner tubes (right). Excitons are depicted as yellow ellipses. Exciton diffusion (dotted paths) allows excitons to meet and annihilate (white symbols) or encounter a non-radiative trap state (blue symbols), both immediately quench the exciton. |
In the first time interval, PL of both double-walled nanotubes and isolated inner tubes feature a steep increase of the PL decay rate for exciton densities exceeding 1 exciton per ∼104 molecules (Fig. 5a), which corresponds to 1 exciton per ∼100 nm of the nanotube length. This value marks the onset of EEA, which refers to the critical exciton density at which excitons are able to undergo diffusion-assisted EEA. Below that threshold excitons are statistically spaced too far apart so that they hardly meet during their lifetime.
A similar behaviour is observed in the second interval, but with a shallower acceleration of the PL dynamics (Fig. 5b). Conceptually, this agrees with the previous assignment that the initial interval is dominated by EEA, while the second interval is less affected due to an already depleted exciton population. Note that the occurrence of EEA faster than the temporal resolution of the streak camera (∼7 ps) is manifested in a sub-linear scaling behaviour of the initial PL amplitude (ESI,† Section S8).
Comparison of the intensity-dependent acceleration of PL of double-walled nanotubes and isolated inner tubes reveals that independently of the chosen spectroscopic observable (PL decay rate and amplitude) the response of both systems is virtually identical at all exciton densities. This implies that the excitonic properties of the inner tube are robust towards stripping the outer layer and, hence, long-range exciton transport as a crucial factor for the occurrence of EEA, is not compromised (Fig. 5c). If the exciton transport had been compromised by complete dissolution of the nanotubes into diluted non-interacting molecules, no exciton density dependence would have been observed (Fig. 5a, gray dots).
To model the observed PL dynamics, we use Monte-Carlo (MC) simulations of the exciton populations; an elaborate description of the MC simulations including a complete overview of the model and parameters has been published elsewhere.42 In essence, at time zero (marked by the arrival of the laser pulse at the sample) excitons are planted on a molecular grid representing the inner and (in the case of double-walled nanotubes) outer tube. The number of planted excitons is set in accordance with the experimental exciton density. Thereafter, excitons perform a random walk on the molecular grid during which they can hop between the inner and outer tube at a given transfer rate, decay (non-)radiatively according to their lifetime or undergo EEA once two excitons approach closer than a critical distance (the annihilation radius). The PL intensity at a given time in the simulation is evaluated as the number of remaining excitons. For comparison with experiment the PL transients are convoluted with a Gaussian apparatus function (FWHM ≈ 7 ps). The PL decay rates are obtained by applying the same fitting protocol as for the experimental data to the thus obtained transients.
Under these settings, MC simulations satisfactorily reproduce the initial (fast) PL dynamics (Fig. 5a, lower dashed line), but totally fail to capture the PL tails at high excitation densities (Fig. 5b, lower dashed line; and ESI,† Section S10). The reason for this is that towards the end of the first time interval (i.e., around ∼30 ps) the exciton density is already too depleted for further EEA, as most of the excitons have either decayed naturally or annihilated. Therefore, we are forced to conclude that the acceleration of the PL tail is unlikely caused by EEA. We also eliminated experimentally two other foreseeable reasons for such acceleration: accumulated photobleaching (ESI,† Section S11) and temperature dependence of the non-radiative decay (ESI,† Section S12).
As a possible scenario to explain the intensity dependent acceleration of the PL tails, we explore the formation of light-induced non-radiative trap states (or simply traps). Traps such as chemical impurities or morphological dislocations are known to act as quenching sites for excitons (as schematically depicted in Fig. 5c) and, thus, have profound impact on the exciton lifetime.56–60 For instance, it has been shown in a recent study61 that light exposure of the double-walled nanotubes embedded in a sugar matrix leads to reversible changes of their optical properties. Here, we include such possibility by allowing molecular grid sites to be converted into traps with probability P upon the decay (either naturally or due to EEA) of an exciton on that site, which thereafter is labelled as a trap until the end of the simulation run. Diffusion of another exciton onto a trap then causes the immediate death of that exciton. In the MC simulations, the probability P evolves according to:
(1) |
At low trap density, ntrap(t) ≪ nsat so that the probability to convert the site into the trap is unity, P(t) = 1. At high trap density (ntrap(t) ≫ nsat) the probability reduces to naught. Therefore, the saturation trap density implies a finite number of the molecular sites which can be converted into traps (‘weak links’). The trap formation is reversible in the sense that they fully recover before arrival of the next excitation laser pulse (after ∼12 ns), as otherwise accumulation effects would have been observed, which is not the case (ESI,† Sections S11 and S12). The photochemical mechanism behind the light-induced trap formation might be, for instance, photo-isomerization of the chromophore via a conical intersection.62–64
In our simulations nsat was the only fitting parameter; all other parameters (hopping rate, annihilation radius, etc.) were fixed according to ref. 42. The resulting transients from MC simulations are shown in Fig. 4 superimposed with the experimental data. Setting nsat = 10−4 yielded the most satisfactory global fit of all PL transients (Fig. 4) and PL decay rates (Fig. 5a and b) of both isolated inner tubes and double-walled nanotubes despite the simplicity of the model. This value of nsat implies that conversion of only one C8S3 molecule out of 10000 into a trap leads to substantial PL quenching, which is consistent with high exciton mobilities.14,15,42 Note that neglecting the saturation of the trap density does not lead to a satisfactory description of the experimental data (upper dashed lines in Fig. 5a and b, and ESI,† Section S10). Nevertheless, the origin of the saturation behaviour of the number of available light-induced traps still remains debatable.
Our findings underpin the versatility of the microfluidic approach to manipulate a nanoscale system via controlled reduction of the complexity of its hierarchical supramolecular structure. Working in tandem with ultrafast spectroscopy, this approach opens up unprecedented opportunities to study exciton dynamics in complex self-assembling molecular systems.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/d0cp01734e |
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