Mikkel Baldtzer
Liisberg
,
Stefan
Krause
,
Cecilia
Cerretani
and
Tom
Vosch
*
Nanoscience Center, Department of Chemistry, University of Copenhagen, Universitetsparken 5, 2100 Copenhagen, Denmark. E-mail: tom@chem.ku.dk
First published on 21st April 2022
A method for measuring emission over a range of sub-nanosecond to millisecond timescales is presented and demonstrated for a DNA-stabilized silver nanocluster (DNA-AgNC) displaying dual emission. This approach allows one to disentangle the temporal evolution of the two spectrally overlapping signals and to determine both the nano- and microsecond decay times of the two emission components, together with the time they take to reach the steady-state equilibrium. Addition of a second near-infrared laser, synchronized with a fixed delay, enables simultaneous characterization of optically activated delayed fluorescence (OADF). For this particular DNA-AgNC, we demonstrate that the microsecond decay times of the luminescent state and the OADF-responsible state are similar, indicating that the OADF process starts from the luminescent state.
Since some DNA-AgNCs seem to emit photons over a large time domain, a single experiment covering this entire range will simplify characterization and provide the needed information to create a more complete picture of the excited state processes. The concept of simultaneously determining fluorescence and phosphorescence has previously been implemented for lifetime imaging (FLIM/PLIM) with a confocal microscope and a TCSPC counting module.21,22 In this application, a micro- to millisecond burst of high repetition rate excitation light (which enables to determine the nanosecond lived fluorescence) builds up a population of microsecond lived states that, after turning off the excitation source, allows any long-lived luminescence to fully decay without interfering fluorescence. This cycle is repeated until sufficient photons are collected for constructing both the nano- and microsecond decay curves. The burst approach is a convenient way to build up a population of species with a decay time that is longer than the pulse repetition time.23,24
We present here a similar and generally applicable method for studying systems exhibiting both nano- and microsecond decay times. As an exemplary system, we studied DNA-Ag16NC,25 which shows both nanosecond and microsecond emission at room-temperature (RT).13 The pulsed burst mode measurements were combined with secondary NIR excitation to elucidate the origin of the state responsible for OADF. By using time gating schemes, we were able to extract the decay time of the state responsible for OADF, which was similar to the decay time of the microsecond lived luminescent state.
The assignment of a micro- and macro-time to every photon brings many advantages. Histogramming the micro-times yields the nanosecond fluorescence decay curve, while long lived luminescence will appear as an increased background in the micro-time domain (Fig. 1c). To determine the luminescence decay (Fig. 1a), the high repetition rate of the 520 nm excitation source (fMicro = 11 MHz) is kept on for a certain period (Ton) to build up a population of the luminescent state, followed by a period where the excitation source is turned off until the next burst cycle starts (Toff). 11 MHz was chosen since it is a suitable time window to capture the ns decay curve. The sync signal of the high repetition rate laser allows for the determination of the macro-times of the luminescence photons during the Toff period and to construct a decay curve by histogramming these photons. While the Ton period will contain a combination of fluorescence and luminescence, the decay curve during Toff can be considered as luminescence only (if the photons in the nanosecond range after switching off the last pulse are ignored). Knowing both the micro- and macro-times, it is possible to gate the photons to extract specific temporal evolutions (see Fig. S2† for a representation of all gating schemes used). For instance, the temporal evolution of the luminescence during Ton and Toff in the macro-time domain can be constructed by only using the photons corresponding to the background level in Fig. 1c. A similar temporal evolution of the fluorescence can be constructed in the macro-time domain, allowing to investigate if the equilibrium times for the fluorescence and luminescence are alike. The latter was previously demonstrated by Petty et al. and must be the case when all states are connected in a classic three-level system.12
To verify whether the microsecond lived luminescent state of DNA-Ag16NC is capable of OADF, experiments were conducted by co-illuminating with a primary (520 nm) and a secondary (850 nm) excitation source able to regenerate the fluorescent state (Fig. 1b). Owing to their different optical path lengths, there is a temporal delay (tdelay) between the two pulses on the nanosecond timescale (Fig. 1c). The temporal evolution of OADF in the macro-time domain can be reconstructed by continuously illuminating with the secondary excitation source and micro-time gating the OADF-related photons (Fig. S2c†), as is done for all experiments. Note, however, that Fig. 1b shows the general realization of the experiment, where one can control independently the duration (Ton2) and the macro-time delay (Tdelay) of the secondary excitation source with regard to the primary.
Binning all the macro-times directly, yields an ungated intensity trace that represents the combination of both fluorescence and luminescence contributions (see also Fig. S5;† note that Fig. S5† is an example at 77 K, while the data in Fig. 2 is recorded at RT). Since each photon has a micro- and macro-time assigned, it is possible to gate photons based on whether they are in or out of the fluorescence window (approximately from 12 to 35 ns, see Fig. 2a). Furthermore, the fraction of luminescence in the fluorescence window can be calculated (see ESI and Fig. S6† for further details on the disentanglement of both signals). Thus, the macro-time evolution of fluorescence and luminescence can be determined and represented separately (Fig. 2b). Fig. 2b shows that the fluorescence intensity drops with time until the steady-state equilibrium is reached. Similarly, the luminescence intensity increases until it also reaches a steady-state equilibrium (see Fig. S7† for the IRF profile of the burst period). After the last 520 nm laser pulse (at 0.5 ms), a steep drop can be observed, as would be expected for the ns-lived fluorescence. The decay of the luminescence is slower, spanning from tens to hundreds of microseconds at RT and 77 K, respectively. The constant intensity level from ca. 1 to 1.5 ms in the luminescence trace (Fig. 2b) is due to detector dark counts. This contribution could be subtracted, but it was neglected here given the low number of counts.
With the fluorescence and luminescence disentangled, it is possible to extract four parameters from the data in Fig. 2: the decay time of the nanosecond fluorescence (τFl), the equilibrium time of fluorescence (τFl,E), the equilibrium time of luminescence (τLu,E), and the decay time of luminescence (τLu,D). Fitting τFl, τFl,E and τLu,E bi-exponentially (intensity averaged decay times are represented, see Fig. S8†), and τLu,D mono-exponentially yields values of: τFl = 2.17 ns, τFl,E = 53.7 μs, τLu,E = 54.1 μs, and τLu,D = 75.7 μs for the data in Fig. 2.
So far, the phenomenological electronic structures of DNA-AgNCs have been described by either a three-12 or a four-level model.19 The values τFl and τLu,D represent post-laser pulse and post-burst processes on the micro- and macro-timescale, respectively, and hence should be excitation intensity-independent. Indeed, in the entire investigated excitation intensity range, τFl is constant and centered around 2.17 ns. τLu,D is fairly constant, however, a minor drop from 76 μs to 73 μs can be observed upon going from 1084 W cm−2 to 23 W cm−2. We believe that this drop is the result of an environmental change, rather than an intensity-dependent phenomenon. During the approximately four hours of measuring, the amount of dissolved molecular oxygen could change, and the concentration of H2O would steadily increase by dynamic exchange of D2O with atmospheric H2O. We have recently demonstrated that an increase in oxygen and H2O content lead to a shortening of τLu,D and this is the most plausible explanation for the change of τLu,D.13 Note that the experiment was performed from high to low excitation intensity.
Unlike τFl and τLu,D, the equilibrium times of the fluorescence (τFl,E) and the luminescence (τLu,E) should be excitation intensity-dependent. For a classic three-level system, τFl,E would be expected to be equal to τLu,E, as was recently shown for a green-emitting DNA-AgNC, where the excitation intensities were kept below 50 W cm−2.12τFl,E and τLu,E are indeed similar and approach the value of τLu,D at low excitation intensities.11 Shorter equilibrium times are obtained for increasing excitation intensities (Fig. 3). It is worth noticing that both equilibrium times could have been satisfactorily fitted with a mono-exponential function at low excitation intensities, given the limited number of counts. However, at higher excitation intensities, especially above 400 W cm−2, τFl,E was significantly better fitted with a bi-exponential model (see Fig. S8†), thus we chose to fit also τLu,E bi-exponentially. It is unclear why the equilibrium time τFl,E is bi-exponential, but a possible explanation could be that there are subsets of populations with different sets of photophysical rates. This suggestion is not unreasonable, since we previously demonstrated for a red-emitting DNA-AgNC that a small fraction of the population had a significantly higher dark state formation yield in poly vinyl alcohol (PVA).26 However, this explanation should be considered suggestive at this point and further studies are needed to unravel the origin of the bi-exponential nature of τFl,E, but this is beyond the scope of this paper.
The luminescence of DNA-Ag16NC was collected during co-illumination in D2O at RT, and the ungated micro-times of all photons were binned as shown in Fig. 4a. A fluorescence response is observed when excited by the primary 520 nm laser at 12 ns, and a second smaller response arises at 57 ns due to the secondary 850 nm laser. Similar as for the disentanglement of fluorescence from luminescence, it is possible to separate the additional OADF contribution by micro-time gating (Fig. S2c†). Thus, the primary fluorescence, OADF, and luminescence signals are individually resolved in the macro-time domain (Fig. 4b).
From these measurements, three additional parameters can be extracted: the nanosecond decay of the OADF signal (τOADF), the equilibrium time of the OADF state (τOADF,E), and the microsecond decay of the OADF state (τOADF,D). Fitting every OADF contribution and τLu,D mono-exponentially and the rest bi-exponentially yields values of: τFl = 2.17 ns, τOADF = 2.20 ns, τFl,E = 66.2 μs, τLu,E = 66.0 μs, τLu,D = 74.8 μs, τOADF,E = 49.8 μs, and τOADF,D = 65.8 μs for the data in Fig. 4. In agreement with a previous report,19 roughly the same nanosecond decay time is observed under primary (τFl) and secondary (τOADF) excitation, alluding to the repopulation of the fluorescent state upon 850 nm excitation. The equilibrium time of the state responsible for OADF (τOADF,E = 49.8 μs) is similar but slightly lower than the equilibrium time of the luminescent state (τLu,E = 66.0 μs), while the macro-domain decay times under additional 850 nm excitation are also similar (τOADF,D = 65.8 μs, τLu,D = 74.8 μs). Note that a previous report showed that τOADF,D can be multi-exponential, however, the amount of OADF counts in our case is rather low to justify going beyond a mono-exponential fit.19 The slight differences between the OADF and luminescence equilibrium and post-burst decay times could be due to the limited numbers of counts for the OADF signal. Despite these minor discrepancies, we feel confident to conclude that the state responsible for OADF is the luminescent state.
Embedment of DNA-AgNCs in a PVA film has previously shown to enhance the overall OADF contribution (area under OADF decay divided by area under primary fluorescence decay like in Fig. 4a).19 Also for DNA-Ag16NC, the OADF contribution increases from 0.7% in a 10 mM NH4OAc D2O solution to 2.4% in PVA (Fig. S10†). Furthermore, the ns fluorescence decay lengthens to an intensity-averaged decay time, τFl, of 3.73 ns; τOADF,D also increases to 107 μs. While other DNA-AgNCs have shown upconversion fluorescence (UCF) during sole secondary illumination when embedded in PVA,18 DNA-Ag16NCs within PVA exhibit negligible UCF at 6.3 kW cm−2 (Fig. S10†).
Interestingly, while our results show a seemingly 0.7% OADF efficiency for DNA-Ag16NCs in a 10 mM NH4OAc D2O solution (Fig. 4a), it should be noted that this contains both steady-state and non-steady state contributions (Fig. 4b), and that during Ton a significant population of luminescent states is built up. One should also realize that the 0.7% is not a single 850 nm pulse efficiency as the OADF-responsible state is subjected to thousands of 850 nm pulses during its lifetime. In fact the value of τLu,D with the secondary light on (74.8 μs) is basically identical to the value of τLu,D reported in Fig. 3 (ranging from 76 to 73 μs), where no secondary light was present. These findings are in line with previous work showing that significantly higher secondary excitation intensities are needed to really observe a shortening of τOADF,D (preferably kW cm−2 to MW cm−2).18,19 Another reason for the absence of any significant shortening of τOADF,D is that we did not investigate the wavelength dependency of the OADF process for DNA-Ag16NCs and perhaps 850 nm is not the most ideal wavelength.16
Footnote |
† Electronic supplementary information (ESI) available: Materials and methods section, HPLC purification details and additional spectral and time-resolved information. See https://doi.org/10.1039/d2sc01137a |
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