Amplified spontaneous emission of a colloidal quantum dot film is electronically controlled in a practical device.
Abstract
Colloidal quantum dots (CQDs) are highly promising materials for light amplification thanks to their efficient photoluminescence, tunable emission wavelength and low-cost synthesis. Unfortunately, CQDs are suffering from band-edge state degeneracy which demands multiple excitons to achieve population inversion. As a result, non-radiative Auger recombination increases the lasing threshold and limits the gain lifetime. Here, benefiting from the negative charging, we demonstrate that the amplified spontaneous emission (ASE) threshold is controllable in a device where CQD film is exposed to an external electric field. Specifically, singly charged CQDs lower the threshold due to the preexisting electron in the conduction band, while strongly enhanced Auger recombination in doubly charged CQDs stymies the ASE. Experimental results and kinetic equation model show that ASE threshold reduces 10% even if our device only charges ~17% of the CQD population. Our results open new possibilities for controlling exciton recombination dynamics and achieving electrically pumped CQD lasers.
INTRODUCTION
Since colloidal quantum dots (CQDs) were first demonstrated as an optical gain medium for lasing applications, the search for CQDs with low gain threshold has been hindered by nonunity degeneracy of the band-edge states (1–6), which means that multiple-exciton gain is needed to achieve light amplification (7, 8). This condition requires that the average number of excitons per CQD is greater than one (〈N〉 > 1), signifying that a considerable percentage of CQDs should contain at least one biexciton. This results in the accelerated nonradiative Auger process (9–13), whereby electron-hole recombination energy is nonradiatively transferred to a third carrier. Auger recombination is almost two orders of magnitude faster than the radiative process in typical CQDs (4, 14–16), which has been the main obstacle to achieve sustainable and low-threshold CQD lasing.
Multiple strategies have been proposed to overcome this challenge and achieve low-threshold CQD lasers. Much work has pursued the idea of suppressing Auger recombination. This nonradiative Auger rate (inverse of Auger lifetime) can be reduced by engineering the wave function confinement of electrons and holes in CQDs including type II CQDs (17), alloyed core-shell interface CQDs (18), and “giant” or tailored CQDs (19). Another effort to reduce the optical gain threshold is to inject electrons into the conduction band, i.e., negatively charged CQDs. These extra electrons contribute to the carrier population in the excited state of the CQDs, substantially reducing the reabsorption (optical loss) or even creating optical transparency at the emission wavelength (20). Therefore, the population inversion or stimulated emission can be obtained at much lower pumping levels (6).
Very recently, Klimov’s group has demonstrated population inversion with the optical pumping threshold at 〈N〉 = 0.02 in charged CQDs via photochemical reduction (6). In addition, Guyot-Sionnest’s group had investigated the lowering amplified spontaneous emission (ASE) threshold in CQDs by electrochemical charging at low temperature (13). However, photochemical doping requires CQDs in an oxygen-free environment; otherwise, all these changes are reversed completely (20). In addition, the electrochemical method demands a solution (electrolyte) environment to charge CQDs. Given the final goal of achieving a practical CQD laser, a method to charge CQDs reliably in an optoelectronic device is preferred (16). The use of an electric field to modulate the spontaneous emission properties of nanoparticles in a capacitor had been explored by Delehanty’s group (12) and Woggon’s group (21) as a “device-ready” approach. To date, the investigation remaining in the spontaneous regime might be used for sensing applications. Here, we demonstrate the control of CQDs’ ASE in the device structure via electric field–induced charging. By adjusting the voltage bias on the device, we are able to regulate the average charging level in the CQD film, and a lower ASE threshold is achieved with optimum charging level where the advantages of low-population inversion threshold dominate the adverse effect of Auger recombination.
RESULTS AND DISCUSSION
Spontaneous emission of CQDs in the device
We investigated CdSe/CdS/ZnS core-shell-shell CQDs, which were produced using a slightly modified synthesis recipe (1) reported by Bawendi’s group (see details in Materials and Methods). This quasi–type II structure, shown as an inset in Fig. 1A, has advantages of suppressed Auger rate, high quantum yield (QY), and enhanced absorption cross section, which are beneficial for laser applications. The high-bandgap ZnS shell with a thickness of ~1.5 nm passivates the potential surface traps and still maintains the quasi–type II structure. The absorbance and photoluminescence (PL) spectra of the diluted CQDs dispersed in toluene (1 mg/ml) at room temperature are presented in Fig. 1A. The PL spectrum [full width at half maximum (FWHM) of ~34 nm] is broader than that of typical CdSe/CdS CQDs, which is attributed to the ZnS outermost shell as widely discussed in the literature for this core-shell-shell structure (9, 18). Both the two well-resolved excitonic transitions and a clean emission spectrum with more than 70% QY suggest the high quality of CdSe/CdS/ZnS CQDs. High-concentration CQDs (>100 mg/ml) in toluene were prepared for subsequent spin-cast compact CQD films.
We used a capacitor structure to apply electric field on our CQD film. To avoid CQDs being directly adjacent to electrodes, which would quench the photon emission, the CQD film was sandwiched between two dielectric layers [SiO2 and poly(4-vinylphenol) (PVP); see the Device fabrication section in Materials and Methods]. Meanwhile, this multiple-layer capacitor structure limits the electrical current (see measured current in fig. S6) through the CQD film to a maximum extent. This is important as electric current through a photoconductive device can lead to heavy charging and result in totally quenched emission of CQDs (22). Figure 1B illustrates the schematic of the device’s layer structure and the excitation geometry for optical characterization. Accordingly, the spectroscopic modulation observed in our device is attributed to the applied electric field. A sinusoidal AC bias is applied to introduce the external electric field through two electrodes [indium tin oxide (ITO) and aluminum] attached to the top and bottom dielectric layers. The AC bias was chosen to avoid slow chemical processes happening reversibly with the DC bias (see more details in section S1). The thickness of each layer is determined by cross-sectional imaging of the capacitor structure by scanning electron microscopy, as shown in Fig. 1C, which is in good agreement with the measurement by a surface profiler (see thickness results in fig. S2). Given the three layers between the two electrodes, the device is equivalent to three capacitors in series; a reference capacitor is adopted to measure the voltage drop across the CQD film (the detail of the calculation is presented in fig. S1). Together with the measured thickness of the CQD film, the electric field can be obtained more accurately for the CQD layer.
The emission properties of the CQD film under the external electric field were investigated by using a subnanosecond pulse laser with a stripe excitation geometry (Fig. 1B). First, we checked the spontaneous emission behavior with increasing electric field. When pumping with a fluence of ~272 μJ/cm2, the CQD film exhibited a decrease in emission intensity (Fig. 1, D and E), accompanied by a redshifted emission peak and broadening of the emission profile (Fig. 1, D and F) with increasing electric field. Basically, these three observations match the expectation of quantum-confined stark effect (QCSE), which relies on the pulling effect in different directions on electron and hole wave functions in a spatially confined structure induced by the external electric field (23, 24). Because of the wave function adjustment, QCSE leads to a decrease in radiative recombination rate (PL quenching) (21, 25), a bandgap reduction (PL redshifting) (26), and enhanced phonon-exciton interaction (PL broadening) (23, 24, 26).
Because of the promising applications in nano-optoelectronics, intensive research had been focused on QCSE in nanoparticles. Bawendi’s group (23) demonstrated over 40-meV redshift and more than threefold spectral broadening in a single quantum dot at 10 K in an electric field of 350 kV/cm. In 2012, Weiss’s group (24) reported on a 36% loss in PL intensity, 41-meV redshift, and more than 30% spectrum broadening in a single, permittivity-engineered type II tailored nanoparticle at room temperature in an electric field of 400 kV/cm. Here, in our case, a PL decrease of ~18% in the maximum electric field of 264 kV/cm is roughly consistent with the previous results. In contrast to PL quenching, emission spectra do not exhibit any significant diffusion with increasing electric field: The redshift and broadening of PL spectrum are less than 2 nm (~6 meV) at the maximum electric field of 264 kV/cm. We should note that at room temperature, the local traps and excitons are much easier to fill and charge, causing confined potential fluctuation and resulting in weaker QCSE (24). Besides the weak QCSE, the charging effect of CQDs in our device could be another factor for the observed phenomena: The enhanced nonradiative Auger recombination rates in charged CQDs cause a remarkable PL quenching; the electrostatic interaction among multiple charges (negative trion) leads to a slight PL redshift; and the inhomogeneous charging of CQDs contributes to a small PL broadening. The PL broadening effect might also be attributed to sinusoidal sweeping of the applied electric field across the CQD layer.
Electric field–dependent ASE
With increasing optical pump fluence across our device under zero electric field, a remarkable reduction in the FWHM and a sudden increase in the integrated intensity of the edge emission show a clear transition from spontaneous emission to ASE (see section S2). The ASE peak has a redshift of ~3.4 nm compared with the spontaneous emission peak when the pump fluence increases from 270 to 1605 μJ/cm2 (fig. S7), as expected from biexcitonic gain in our CQDs. The ASE threshold is around 890 μJ/cm2, which is higher than the previously reported threshold (27) for CdSe/CdS/ZnS CQDs (~600 μJ/cm2, when pumped by a femtosecond pulse laser). Three effects here are possibly responsible for the increased ASE threshold: (i) The multiple layers can cause the pump fluence reduction because of the reflection and scattering at each layer and their interfaces; (ii) compared with the femtosecond laser, our 0.5-ns pulsed laser pump has to compete with very fast nonradiative Auger recombination to build up the population inversion; and (iii) the significant reduction of CQD absorption at our pumping wavelength (532 nm) when compared with that at the femtosecond pump wavelength (480 nm), as seen in Fig. 1A. Here, we explore the electric field–dependent ASE at a pump fluence of 1605 μJ/cm2, which can show the dominant stimulated emission and will not cause thermal degradation of the device. The stimulated emission spectra as a function of the electric field are presented in Fig. 2A. The increasing electric field leads to a continuous enhancement in the stimulated emission intensity (Fig. 2B), which is predicted for charged CQDs (see the charge injection mechanism in fig. S5) as it is easier for them to achieve population inversion. Meanwhile, the ASE peaks exhibit a blueshift of ~1.2 nm (see Fig. 2C) when the electric field increases from 0 to 264 kV/cm. The blueshift in the spectrum, together with the intensity enhancement of ASE, indicates contradicting behaviors associated with the QCSE, implying the dominant charging effect in our CQD device. The blueshift in ASE implies lower reabsorption along the stripe waveguide due to the occupied state in the conduction band by extra electrons. However, the increase in ASE intensity is only true when the electric field is low. As the applied electric field exceeds a certain value, the behavior of stimulated emission goes to an opposite direction.
It is shown in Fig. 2D that, at the turning point of ~20.13 kV/cm, we observe a reversed knee behavior in the integrated ASE intensity versus the applied electric field. It is akin to the ASE’s pumping threshold extracted from the light input–light output curve (28); here, we name it as the “E-field threshold.” Below the E-field threshold, the FWHM of the stimulated emission is narrower, and the intensity of the stimulated emission is enhanced as the electric field increases (shown in Fig. 2, B, D, and E). Beyond the E-field threshold, the ASE intensity decreases exponentially as the electric field increases, as shown by the fit to the experimental data in Fig. 2D. At the electric field of 264 kV/cm, the FWHM increases to ~33.3 nm, which is close to that of the spontaneous emission (~35 nm) of the CQD films.
As shown in Fig. 2F, we have achieved an ~10% reduction in the ASE threshold by applying an electric field, which is far from the theoretical calculation: ~40% threshold reduction is expected for singly charged CQDs, and the zero threshold is predicted for doubly charged CQDs (6). However, it should be noted that the theoretical calculation for the threshold is only for the population inversion or the optical transparency of the materials, while the ASE threshold can be only achieved with the net gain where the optical gain dominates all the optical loss. One can probe the optical transparency of the material with the transient absorption experiment but might not achieve ASE because of the low gain coefficient and large optical loss (29). Nevertheless, this behavior of first increasing and then decreasing threshold in our device with respect to the electric field implies multiple competing mechanisms. This leads us to delve into the electric field–induced spectroscopy in greater depth and figure out the dominant recombination processes with respect to different electric fields.
Competing mechanism in CQDs under varied electric fields
Quantifying the bleaching of the absorbance features can shed light on the occupied states in the conduction band of CQDs and give us more information about the ongoing transition processes. Here, we calculate the absorbance spectra from measuring electric field–dependent reflectance spectra of our device under different electric fields (see related equations, measurement setup, and data in section S3; figs. S8 to S10). As illustrated in Fig. 3A, the increase in the applied electric field results in progressive reduction in the amplitude of the first and second excitonic absorbance peaks. We also notice that the absorbance at the pumping wavelength (532 nm) is enhanced slightly as the electric field increases because of the reduced energy required for trion formation. However, at ~21 kV/cm, this enhancement (<0.3%) is negligible compared with the achieved threshold modulation (>10%) (see more details in section S3). To be quantitative about the degree of charging (the average excess electrons per CQD, <ne>), the absorbance spectra are fitted to the sum of four Gaussian fittings (Fig. 3B and fig. S11) (20, 30, 31). According to the two lowest allowed interband transitions in CdSe/CdS/ZnS CQDs (inset of Fig. 3B) (31), we can assign the first Gaussian peak (A1) to 1S(e)-1S3/2(h) transition and the second Gaussian peak (A2) to 1S(e)-2S3/2(h) transition.
Thus, <ne> can be estimated from the reduction of the integrated area of each Gaussian fitting, providing that a 100% bleaching corresponds to two excess electrons occupying the 1S(e) state in the conduction band (20, 32). A plot of the integrated area of A1 and A2 as a function of the applied electric field (Fig. 3C) indicates that bleaching of the 1S(e)-1S3/2(h) and 1S(e)-2S3/2(h) almost changes at the same pace with the increase in electric field. Specifically, the decrease in the integrated area of A2 (−∆A2/A20) versus the decrease in the integrated area of A1(−∆A1/A10) can be well fitted by the line with a slope of ~1.05 (inset of Fig. 3C). The result suggests that the 1S(e)-1S3/2(h) and 1S(e)-2S3/2(h) transitions have the same absorption strength (30) and show the same degree of bleaching in the absorption spectra when applying the electric field because the single-state 1S(e) is involved in both transitions. However, when the E-field is high (>200 kV/cm), the −∆A2/A20 increases slower than −∆A1/A10, implying more absorption strength reduction for 1S(e)-1S3/2(h) than 1S(e)-2S3/2(h). Meanwhile, the integrated areas of the other two Gaussian curves, A3 and A4 (fig. S12), remain virtually unchanged with respect to the applied electric field, implying that no excess electrons can be induced in the states beyond 1S(e) with the electric field up to 264 kV/cm.
We adopt two ways to calculate <ne>. One method is based on extracting <ne> from the first Gaussian fitting of the absorbance spectra. Another way is to calculate <ne> by integrating the absorbance difference (inset of Fig. 3A). As shown in Fig. 3D, they are consistent with each other. Up to the electric field of 264 kV/cm, we find a maximum <ne> of ~0.35. According to the previous reports about photochemical charging (20), there is a linear correlation between <ne> and the amount of hole quenchers, while it is also true for electrochemical charging where <ne> varies linearly with the charges flowing into the CQDs (32). Here, the linear relationship between <ne> and applied electric field is still valid in our case. However, <ne> increases at different rates in the low and high regimes of electric field. A reasonable explanation for this observation is the different charging levels for a portion of CQDs in the thick film. Although <ne> is only 0.35, the charges are likely distributed to the CQDs at the interfaces with other dielectric materials (SiO2 and PVP), while the measured absorbance bleaching is the average effect of the ensemble CQDs. Hence, the turning point in the electric field of ~21 kV/cm is the indication that singly negatively charged CQDs are starting to become doubly negatively charged CQDs. Because of the Coulomb repulsion effect, it is more difficult for the electric field to induce one more electron to singly charged CQDs compared with the neutral ones. The electric field value of ~21 kV/cm matches the E-field threshold that we discussed in Fig. 2, signifying that singly charged and doubly charged CQDs should be responsible for the E-field threshold behavior of the “first increasing and then decreasing” ASE intensity.
To further verify the validity of the electric field–induced charging process in CQDs, we analyze the effect of the applied electric field on PL dynamics. Different processes associated with different physical properties of CQDs can be distinguished via the time-resolved PL (trPL) analysis if their decay rates are different. The radiative lifetime value inferred from the trPL measurement can elucidate the question in Fig. 1 about the dominant factor causing the reduction of spontaneous emission intensity: whether QCSE or charging effect dominates in CQDs. The two factors affect the spontaneous emission in different ways: QCSE weakens the radiative recombination (23), whereas trions can both accelerate nonradiative Auger recombination and enhance the radiative process compared with the neutral exciton (8).
Figure 4A shows the PL decay of a CQD film measured under different electric fields. All the data are measured with the same collection time and then normalized by the maximum intensity of the CQD film without electric field. Hence, the results allow us to extract not only the decay rates but also the relative intensity among different electric fields at any decay time. Without the electric field, the single-exponential decay process for the CQD film (lifetime: ~20.1 ns) in the device structure is slightly faster than that for a bare CQD film on glass (lifetime: ~25 ns) because of the different dielectric environments (6, 8). We notice that the PL signal at early time increases relative to that in neutral CQDs. This phenomenon results from the enhanced radiative process in charged CQDs and supports the argument that charging effect, instead of QCSE, is responsible for the spectroscopy changes. However, time-integrated PL still shows the intensity reduction with the increasing electric field due to the Auger process caused by the extra electron. As the electric field increases, both enhanced radiative recombination and the Auger process are responsible for trPL becoming continuously faster.
To develop more insight, we fit each decay curve to extract the dynamics with different electric fields (solid lines in Fig. 4A). With increasing electric fields, two new fast decay components appear. As illustrated in Fig. 4B, these two fast decay components (4.1 and 0.75 ns) are well correlated with the singly charged exciton lifetime (5 ns) and doubly charged exciton lifetime (2 ns) measured in single quasi–type II CQD for blinking study (33). Slightly faster decay in our sample compared with (33) is understandable as a single CQD normally has a longer lifetime than a CQD ensemble, and our CQD film experiences different dielectric environments. To eliminate other possibilities (Auger process or carrier trapping), we have conducted fluence-dependent trPL to justify the lifetime assignment (details are presented in section S4; fig. S13). Hence, we can safely assign the lifetimes of 20.1, 4.1, and 0.75 ns to neutral exciton, singly charged exciton, and doubly charged exciton, respectively. It is important to note that these three lifetimes remain almost constant with increasing electric field, implying that electric field changes only the population of X0, X1−, and X2− and further confirming that a change of the integrated wave function overlap caused by the electric field (QCSE) is very small in our case.
From the fitting parameters of trPL, we can derive populations of X0, X1−, and X2− (inset of Fig. 4B) with different electric fields. With low electric field, only neutral-state and singly charged excitons contribute to the PL intensity dynamics. However, as electric field goes beyond a certain level (~21 kV/cm), the amount of X2− soars up, while the population of neutral CQDs remains unchanged. This trend largely agrees with the conclusion drawn from the steady-state absorbance analysis: Electric field can only charge a portion of the CQD populations. At the optimal electric field (~21 kV/cm), our device charges 17% of the CQD population to lower the threshold by ~10%.
We can perform a simple calculation to extract <ne> (<ne> = 0 × X0 + 1 × X1− + 2 × X2−) based on the derived populations. As shown in Fig. 4C, <ne> extracted from the PL decay exhibits a good agreement with that obtained from the optical bleaching. The maximum deviation of less than 0.04 electron per CQD is acceptable, considering the Gaussian deconvolution and exponential fitting process. From the standpoint of optical gain applications, we are concerned more about the radiative recombination and the Auger process under different conditions. We assume that neutral exciton lifetime (20.1 ns) is purely radiative based on the fact that the PL of CQDs without electric field is a single exponential decay (almost a straight line in our semilog plotting). Hence, we can deduce the radiative lifetime of X1−, X2−, and the neutral biexciton, XX, using the relationship τradiative = 20.1/α (α is the radiative enhancement factor). Statistically, α is 4 for biexcitons, while α is 2 for singly and doubly charged exciton. However, recent reports (33) show that the electron repulsion effect occurring in charged CQDs will result in a factor less than 2. Here, we use α = 1.5 according to the fitting results of PL dynamics using a Poisson distribution model (see details in section S4; fig. S14) (6). Thus, we can calculate the Auger lifetime using the following equation: 1/τtotal = 1/τradiative + 1/τAuger. As shown in Fig. 4D, the Auger lifetime of X1− is about 5.9 ns, which is much lower than the Auger process (~730 ± 47 ps; see fig. S13) in the biexciton (34). However, the Auger lifetime of the doubly charged exciton (~790 ps) is quite close to the value in the neutral biexciton. The stimulated emission rate of X2− is twofold less than the stimulated emission rate (section S5) in the biexciton.
Modeling the electric field–dependent threshold
We have now quantified the lifetimes of X, XX, X1−, and X2− by fitting the PL dynamics. Meanwhile, we know the population of each state as a function of the applied electric field obtained by analyzing the trPL and absorbance bleaching data. Therefore, we can apply the rate equations to evaluate the ASE threshold with different electric fields. The model we use here is based on the recent calculations for optical gain, which considers both the Auger process and optical cavity losses (35–37). We adopt the rate equations for neutral and singly/doubly charged CQDs and plug in the electric field–dependent population distribution and all the recombination rates to complete our model [see the detailed parameters, transition processes (fig. S15), rate equations, and simulated dynamics (figs. S19 and S20) in section S5]. Figure 5A shows a cartoon of the stimulated emission process in neutral, singly, and doubly charged CQDs, respectively. In neutral CQDs, a biexciton is required for population inversion, which is harder to achieve but provides better gain coefficient. Singly charged CQDs lower the requirement for population inversion due to the preexisting electron in the conduction band. For X2−, the doubly charged CQDs are transparent and achieve population inversion with any excitation level. However, the enhanced Auger recombination (compared with singly charged CQDs) and less efficient radiative recombination (compared with biexcitons) deplete the exciton very fast. This affects the optical gain in two ways: fewer emission photons to trigger stimulated emission and fewer excitons to contribute to stimulated emission. One can experimentally show negative absorption (population inversion) in transient absorption measurement at very low pumping level, but the demonstration of ASE where the gain has to overcome various losses is very challenging (29). In addition, obtaining the net gain out of the doubly charged CQDs is more difficult with our subnanosecond pumping source because of the very short gain lifetime, governed by dominant nonradiative Auger recombination.
Here, we simulate the dynamics of emitted photon density as a function of the applied electric field under different pump fluence. As presented in section S5, we only consider the photons coupling to the waveguide and participating in the ASE process. Noncoupling photons (~95.5%; see the COMSOL simulation in fig. S16) are spontaneously emitted out of the CQD film. At the pump fluence of 800 μJ/cm2 (Fig. 5B and fig. S18A), the abrupt acceleration of photon emission, which is the evidence of the onset of ASE, can only be achieved with the electric field around 21 kV/cm. When the electric field is too low or too high, there is only spontaneous emission. It is consistent with the E-field threshold of ~20 kV/cm extracted from the electric field–dependent ASE characterization (Fig. 2), implying that singly charged CQDs help build up the net gain in our device. In the case of high pump fluence, 1000 μJ/cm2 (Fig. 5C and fig. S18B), the ASE can happen with the electric field up to ~149 kV/cm. This behavior illustrates the stimulated emission process presented in Fig. 5A: Optimum electric field creates enough singly charged CQDs and enables ASE at lower threshold, while higher electric field increases the population of doubly charged CQDs and results in higher threshold for optical net gain (ASE). Our model also suggests that if a device can charge the entire CQD population with a single electron, then we would be able to lower the ASE threshold down to ~35% compared with neutral CQDs, which is slightly less than the theoretical improvement (~40%) for the population inversion threshold (6) due to finite loss in ASE.
The time integration of the emitted photon density (log scale) as a function of the applied electric field (linear scale) and pump fluence (log scale) is shown in Fig. 5D. The threshold with different electric fields (dashed blue line in Fig. 5D and fig. S17) is extracted as the transition point from spontaneous emission to stimulated emission. In Fig. 5E, we compare the simulated ASE threshold trend with the experimental results. With low electric field, the simulated result is in very good agreement with the “up and down” threshold behavior (Fig. 2) up to the electric field of ~200 kV/cm. At higher electric field, the simulation shows lower threshold than the experiment data. This is understandable as our model considered only up to doubly charged CQDs, which would only be valid at low electric field. The Auger recombination rate will increase faster with more electrons in CQDs, and therefore, achieving the optical net gain is harder in the experiment.
CONCLUSION
In summary, we have demonstrated controllable and tunable ASE in a colloidal semiconductor device via electric field–induced charging. The contribution of neutral, singly, and doubly charged CQDs to the ASE are quantitatively determined by analyzing the competing mechanisms happening in the CQD population. Neutral CQDs need high optical pump to create biexcitons, compete with fast nonradiative Auger recombination, and achieve high optical gain. Singly charged CQDs can lower the optical gain threshold because of the partially filled conduction band and low Auger recombination rate. Doubly charged CQDs can, in principle, achieve population inversion with any pumping level, but achieving the net gain still requires a significantly high pumping level due to enhanced nonradiative Auger recombination and low gain coefficient. Our kinetics model to simulate the ASE behavior shows very good consistence with the experimental results, highlighting the dominant role of singly charged CQDs to achieve low ASE threshold. Our work demonstrates the feasibility of controlling not only exciton recombination dynamics but also the CQD charging level to lower the threshold of CQD lasing in a device structure. Our results suggest that good control of the charging process for the entire CQD film will significantly improve the CQD lasers and lower the threshold to possibly enable continuous wave or electrically driven devices.
MATERIALS AND METHODS
Synthesis of CdSe/CdS/ZnS CQDs
Here, the recipe is a slightly modified facile one-pot method (1, 27, 38). Amounts of 1 mmol of cadmium oxide (CdO; >99.99%), 18.85 mmol of oleic acid (OA; 90%), and 2 mmol of zinc acetate [Zn(AC)2; 99.99%] were mixed with 25 ml of 1-octadecene (1-ODE; 90%) in a three-neck flask. The mixture was evacuated for 15 min and heated to 300°C under nitrogen condition. After that, selenium precursor made by dissolving 0.2 mmol of selenium power (Se; >99.99%) in 0.2 mmol of trioctylphosphine (TOP; 90%) was quickly added into the reaction flask at 300°C. Three minutes later, 0.3 ml of dodecanethiol (DT; >98%) was injected slowly into the mixture. The reaction lasts for 20 min to get CdSe/CdS QDs. Subsequently, sulfur precursor made by dissolving 2 mmol of sulfur powder (S; >99.5%) in 1 mmol of TOP was added to react with the excess Cd ions and passivate the surface with ZnS shell. CdSe/CdS/ZnS (core-shell-shell) CQDs were purified with ethanol several times and dispersed in toluene for film fabrication.
Characterization of CdSe/CdS/ZnS CQDs
Absorption spectra of CQDs in toluene (1 mg/ml) were measured using an ultraviolet-visible spectrophotometer (Shimadzu, UV-1800). PL spectra of CQDs in toluene (1 mg/ml) were recorded using a spectrofluorophotometer (Shimadzu, RF-5301PC; excitation wavelength, 532 nm). QY of CQDs in toluene (100 mg/ml) was measured with an integrating sphere and calculated as the ratio of absolute emission photons and absorption photons. The accuracy of the QY measurement was verified using Rhodamine 6G, and the measured QY of 94.3% in our setup was in good agreement with the standard value of 95%.
Device fabrication
First, the glass substrate with ITO was patterned to yield three devices per substrate; the top 2 devices were with CQD film, which provided redundancy in the fabrication process for testing reproducibility, while the bottom one was exactly the same structure but without CQD film, which was used as a reference for steady-state absorption measurement (see details in section S3). After that, glass substrates were carefully cleaned and ultrasonicated. Then, an SiO2 layer with a thickness of ~160 nm was deposited via sputtering (UNIVEX 350; radio frequency, 150 W). The CQD film was deposited by the spin-casting technique (spin duration, 3 min; spin velocity, 500 rpm/s). Another dielectric layer was a PVP film deposited on top of the CQD film also by spin casting [PVP dissolved in ethanol (20 mg/ml); spin duration, 45 s; spin velocity, 2000 rpm/s]. All the spin-casting processes were made inside the glove box, and each spin-casting step was followed by baking the device at 60°C in a nitrogen environment for 20 min. Last, the sample was loaded into a thermal evaporator to deposit the aluminum layer as the top electrode.
Capacitance of the dielectric layers
The capacitance of each dielectric layer was determined using the equation of parallel plate capacitor: C = A × ε/d, where A is the area of the capacitor (8 mm × 2 mm), d is the thickness of each layer determined by the scanning electron microscopy measurement and surface profiler measurement (DektakXT surface profiler), and ε is the permittivity of each dielectric film. Here, low-frequency permittivity was approximated as that at optical frequency and measured using an ellipsometer (VASE, J.A. Woollam; spectral range from 193 to 3200 nm). The measurement data and fitting process of the permittivity can be found in section S1 (fig. S3). The voltage drop across the CQD layer was calibrated via the calculation of the charge stored in insulator layers (see details in fig. S4).
AC bias and stripe excitation
The sinusoidal AC bias was generalized by the function generator (FG500A, WAVETEK) with a frequency of 128 Hz, and the pump laser at 532 nm used for stripe excitation was a frequency-doubling Nd:YAG laser with a pulse width of 0.5 ns and a repetition rate of 100 Hz. The laser beam was focused onto a stripe along the device structure using a cylindrical lens and incidents from the glass substrate. The width of the stripe, which contains (1 − 1/e) of the power in the laser beam, was 50 μm, determined using the knife-edge method. In the experiment, the stripe length was 4 mm. An automatically rotated λ/4 wave plate (WPQ05M-532, Thorlabs) and polarizer (CCM1-WPBS254, Thorlabs) were used to adjust the pump fluence on device. Then, the emission was collected via a fiber-coupled Andor spectrometer (monochromator: Andor Shamrock 303i; charge-coupled device: Andor iDus 401). The collection geometry was perpendicular to the laser pump. All measurements were performed at room temperature in air.
Steady-state absorption measurement
The white light generated by the light source (ELS-250, Asahi Spectra) was filtered by a monochromator (7ISWS; spectral selection range, 330 to 1000 nm) and then focused onto the device through the glass substrate at an angle of 45°; a silicon detector (Newport 2031; 400 to 1070 nm) was used to collect the reflection light off the device. Light transmitted through the CQD layer twice when reflecting off the device. The silicon detector was connected to a lock-in amplifier (SR830, Stanford Research System). The measurement setup and calculation details are shown in section S3.
PL dynamics measurement
The trPL spectroscopy was performed in a confocal system with Micro Photon Devices single-photon avalanche photodiode and a time-correlated single-photon counting acquisition module (Edinburgh Instruments, TCC900). For the excitation, we used a pulsed diode laser at 355 nm with a repetition rate of 10 MHz, while we filtered the emission at 640 ± 20 nm. For all the trPL measurements using the diode laser, the temporal resolution was 200 ps. For the femtosecond laser PL lifetime measurements, the output from a 1-kHz, 50-fs Coherent Libra Regenerative Amplifier (800 nm) that was frequency doubled using a beta-barium borate crystal (to 400 nm) was used as the pump source. The emission from the samples was detected by an Optronis Optoscope streak camera system, which has an ultimate temporal resolution of 10 ps.
Supplementary Material
Acknowledgments
Funding: We would like to acknowledge the financial support from the Singapore Ministry of Education AcRF Tier-1 grant (MOE-2017-T1-002-142). We are also grateful to acknowledge the financial support from the Singapore National Research Foundation under the program NRF-NRFI2016-08; the Competitive Research Program NRF-CRP14-2014-03; and the Singapore Agency for Science, Technology and Research (A*STAR) SERC Pharos Program under grant no. 152 73 00025. Author contributions: C.D. initiated the idea and led, supervised, and contributed to all aspects of the research. H.V.D. initiated and supervised the CQD synthesis and capacitor device fabrication. J.Y., H.V.D., and C.D. wrote the manuscript. J.Y., S.S., and B.L. fabricated the device. J.Y. performed the ASE measurements and the steady-state absorbance measurement. J.Y., S.H., and M.D.B. performed the PL dynamics measurement. M.L. conducted the fluence-dependent lifetime measurement. J.Y. and C.D. conducted the kinetic model simulation. S.S. and S.D. synthesized the CdSe/CdS/ZnS CQDs. P.H.-M. conducted the COMSOL simulation. C.H., W.-k.K., and J.Y. performed the SEM and TEM measurements. T.C.S. and H.W. discussed the results and provided the technical advice. All authors discussed the results, commented on the manuscript, and participated in the manuscript revision. Competing interests: The authors declare that they have no competing interests. Data and materials availability: All data needed to evaluate the conclusions in the paper are present in the paper and/or the Supplementary Materials. Additional data related to this paper may be requested from the authors.
SUPPLEMENTARY MATERIALS
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