Nils
Lenngren
*a,
Mohamed A.
Abdellah
ab,
Kaibo
Zheng
ac,
Mohammed J.
Al-Marri
c,
Donatas
Zigmantas
a,
Karel
Žídek
ad and
Tõnu
Pullerits
a
aDepartment of Chemical Physics, Lund University, PO Box 124, 221 00 Lund, Sweden. E-mail: tonu.pullerits@chemphys.lu.se; Fax: +46 46 2224119; Tel: +46 46 2228131
bDepartment of Chemistry, Qena Faculty of Science, South Valley University, Qena 83523, Egypt
cGas Processing Center, College of Engineering, Qatar University, PO Box 2713, Doha, Qatar
dRegional Centre for Special Optics and Optoelectronic Systems (TOPTEC), Institute of Plasma Physics, Academy of Sciences of the Czech Republic, Za Slovankou 1782/3, 182 00 Prague 8, Czech Republic
First published on 25th August 2016
Colloidal quantum dots (QDs) have attracted interest as materials for opto-electronic applications, wherein their efficient energy use requires the understanding of carrier relaxation. In QDs capped by bifunctional thiols, used to attach the QDs to a surface, the relaxation is complicated by carrier traps. Using 2D spectroscopy at 77 K, we follow excitations in thiol-capped CdSe QDs with state specificity and high time resolution. We unambiguously identify the lowest state as an optically allowed hole trap, and identify an electron trap with excited-state absorption. The presence of traps changes the initial dynamics entirely by offering a different relaxation channel. 2D electronic spectroscopy enables us to pinpoint correlations between states and to easily separate relaxation from different starting states. We observe the direct rapid trapping of 1S3/2, 2S3/2, and 1S1/2 holes, and several competing electron relaxation processes from the 1Pe state.
Most earlier studies of the electronic decay pathways have focused on as-synthesized QDs capped by oleic acid with very few surface traps, showing stepwise relaxation to the nearest lower-lying state.18 For many applications, however, QDs need bifunctional capping agents such as thiols, enabling attachment of the QDs to the surfaces of other nanostructures.6,19 The new capping agent introduces surface traps for both electrons and holes, both due to the identity of the capping agent and the exchange process,20 which leads to the additional complexity of the level structure and carrier dynamics.21 While it is possible to synthesize CdSe QDs with bifunctional capping agents directly,22 this would not solve the problem completely and characterization of the traps is necessary. Trapping from the band-edge state in PbSe has been studied by multidimensional spectroscopy,23,24 but the character of the trap states is still a matter of active investigation.25
In this article, we address the question of energy relaxation in QDs with bifunctional capping agents by using 2D electronic spectroscopy. 2D electronic spectroscopy (2DES) has in recent years shown its utility when it comes to showing correlations and connectivity between different energy levels, as well as achieving high time and energy resolution in QDs and other systems.26–31 The correlations can be tracked by the ability of 2DES to create spectral maps (see Fig. 1 for example) resolving both excitation energy (x-axis) and detection energy (y-axis). The x-axis of a 2D spectrum is created by two-pulse time-domain interferometric excitation with Fourier transform over the delay (the coherence time) between the pulses, while the y-axis shows the spectral resolution of the signal after a probe pulse, detected by spectral interferometry. To a certain extent, the x-axis is analogous to the pump energy in pump–probe spectroscopy, while the y-axis corresponds to the detection energy. The delay between the first two pulses and the third one corresponds to the time delay in pump–probe, here called the population time.
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Fig. 1 2D spectra at early and late population times with energy levels and important features marked, laser and absorption spectra. Middle panel: Total real 2D spectrum of 7.1 nm CdSe QDs in methanol/ethanol glass at 77 K, at a population time of 5 fs. Even at this early time, the nonresonant response of the glass is minor (ESI†). The diagonal line marks where ℏω1 = ℏω3; the horizontal and vertical lines mark the energy levels (see Fig. 2). Bottom panel: The same, at 10 ps. The solid horizontal line marks where a cut was taken for state analysis. Note the rescaling by a factor 2. For letter labels, see the text. Side and top panels: Sample absorbance (red line) and spectrum of the laser employed in the 2D experiment (blue line) in arbitrary units. |
In conventional transient absorption spectroscopy, the Fourier transform forces a compromise between temporal and spectral resolution. 2D spectroscopy avoids this limitation due to the two excitation pulses, enabling simultaneous high time and energy resolution. In the 2D spectrum, inhomogeneous broadening only affects the diagonal direction, and cross-peaks (off-diagonal) show correlations between different states. Furthermore, the high resolution of our setup makes it possible to measure large QDs with closely spaced states, letting us cover more states than previous experiments.
The ability of 2D spectroscopy to reveal correlations between states is to a great extent limited by the homogeneous linewidth of the states. If the sample is cooled, spectral bands are narrower due to reduced phonon-related broadening.32 In this article, we carry out low-temperature (77 K) measurements, enabling us to observe a structure in the 2D spectra that would be smeared out at room temperature.
By combining 2D spectroscopy with cooling the QD sample, we were able to identify states present in the QDs, as well as signals originating from trapping processes. This enables us to reveal the interplay between carrier trapping and relaxation in the QDs.
The measurements were performed with the QDs in a solvent glass. The QDs were redispersed in a 1:
1 mixture of methanol and ethanol,36 and cooled to 77 K in a cryostat (Optistat DN2, Oxford Instruments). Some cracking of the solvent glass occurred, but it was possible to position the beam path away from the cracks. The absorbance was below 0.4 at the first absorption peak (635 nm) in a 0.5 mm cuvette measured at room temperature, and the average number of excitations per QD was 0.12 (ESI†).
We used a previously described 2D spectroscopy setup.37 1030 nm pulses are generated in a Yb:KGW laser at 10 kHz, and feed a nonlinear optical parametric amplifier (Light Conversion), the output of which is then compressed to 9.2 fs long pulses (FWHM) centered at 600 nm. Pulses are delayed using a delay stage (for population time) and glass wedges (for coherence time) and sent through the sample, with the signal beam being detected via heterodyning with a low-intensity pulse in a phase-matching direction. The energy per pulse at the sample is 1 nJ and the diameter of the spot is 100 μm. The interferogram is recorded using a CCD coupled to a spectrometer. 2D spectra were obtained using a broad range of coherence times (−141 fs to 360 fs with 1.5 fs steps) for 85 population times up to 20 ps, with increasing timesteps at longer times (ESI†).
Other prominent features are the diagonal peak B of the second exciton state and the cross-peaks C between the first and second exciton states, showing a strong correlation of these transitions. One can also identify negative peaks D that are a result of the excited-state absorption which is stronger than the bleach in this region. Such spectral features are the result of complex multibody interactions giving rise to biexcitonic shifts.
Finally, for ℏω3 energies below 16000 cm−1, a broad positive feature E arises for later population times. Above 17
000 cm−1 but below the diagonal, a broad negative feature F appears. We will later show that these features can be ascribed to QDs with trapped holes and electrons, respectively.
In order to identify all states in the studied energy range, we have carried out an analysis of the long-lived 2D signal. After a population time of 10 ps, all excited QDs will be in the lowest excited state,18 and by cutting through the total amplitude 2D spectrum at the ℏω3 of the lowest state (16200 cm−1), we can identify the energies of the states which were initially excited (see Fig. 2). This is done by fitting the cut to a sum of Gaussians. Before the fitting, the raw cut is divided by the laser spectrum, as the signal scales with laser intensity along the ω1 axis.38 The main peak (at 16
200 cm−1) is fitted to a sum of two Gaussians. The fit is consistent with absorption spectra at 77 K and room temperature (the details are given in the ESI†).
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Fig. 2 To identify the electronic states of the QDs, we fit a slice of the 2D spectrum along with absorption spectra. All panels show fits of data (black squares) as a sum (gray line) of Gaussians (colored lines, average energies marked by vertical dashed lines) corresponding to specific states. Values were normalized to the maximum. Top panel: 2D total signal amplitude along a cut at ℏω3 = 16![]() |
Apart from a low-energy weakly absorbing state, which can be assigned to the trap-related signal as we will show later, all peaks are in good agreement with the energies given by Norris and Bawendi (ESI†)39 after taking the temperature shift from 10 K to 77 K into account.40,41 We can therefore identify the peaks using their description. In order, they are 1S3/2–1Se, 2S3/2–1Se, 1S1/2–1Se, 1P3/2–1Pe and 2S1/2–1Se. For convenience, we label them as |X1〉, |X2〉, |X3〉, |X4〉, and |X5〉. |X5〉 is at the edge of the 2D spectra and will not be considered further. We point out that all exciton states but one contain the 1Se electron state.
The weak absorption band, 600 cm−1 below the first main peak (on the ω1 axis), is not part of the effective mass model. We consider it to arise from a trap, justified by how relaxation appears in the measured 2D spectra (see Fig. 1): the lowest band (on the ω3 axis) forms a horizontal feature (labeled E in Fig. 1), i.e. the resulting energy of the carriers after relaxation (along the ℏω3 axis) is independent of the excitation energy (ℏω1) which is characteristic of traps. This is quite unlike the exciton–exciton cross-peaks (e.g. the C peaks) in the 2D spectra, where the ℏω3 and ℏω1 energies are clearly correlated (due to inhomogeneous broadening and the size–energy relationships of the energy levels39). The slope of the laser spectrum shifts the E band upwards compared to the position expected from the analysis of the cut and absorption spectra. The absence of correlation between the lowest state and the energies of the excitonic states also rules out an assignment to trions, as it has been reported previously that the trion energy is correlated with the exciton state energies.42 As thiol groups are known to cause hole traps,43,44 we assign this band to a trapped hole combined with the 1Se core electron, and label it as |R1〉. We summarize the initial states in Fig. 3.
With the energy state picture established, we turn to the dynamics. If one disregards signals arising due to coherent dynamics, which show up as oscillatory signals in this system, the total real 2D signal for a chosen ℏω1 and ℏω3 value can be seen as analogous to the pump–probe signal with ℏω1 excitation energy and ℏω3 probe energy, with population time representing the pump–probe delay. Vertical slices through the 2D spectra therefore correspond to excitation wavelength-resolved transient absorption.‡ The signals are a sum of several different contributions, such as bleach, excited-state absorption and stimulated emission. The bleach is due to electrons or holes already residing in the final state, thus blocking a transition. The 1Se state is only twofold degenerate and thus causes strong bleach, but the 1Pe state and the hole states have higher degeneracy and therefore the corresponding bleach is much weaker. The bleach contribution from the hole states is also diminished because they are so close together that they overlap partially.
By knowing the energy of each electronic state, we can track the population dynamics at the particular ℏω1 energies and observe carrier relaxation or trapping with state resolution. If the set of 2D spectra is viewed along the population time axis, the population dynamics can be followed as excitons relax from state to state. We select a number of ℏω1 values where one initial exciton state should be dominant and slice the 2D spectra at these values, following the development of the ℏω3 spectrum as a function of population time (see Fig. 4). We choose the excitation energies ℏω3 in such a way that they correspond to the peak positions in Fig. 2, except for the |R1〉 and |X3〉 states where we pick a lower energy to avoid the otherwise overwhelming signal from the |X1〉 or |X4〉 state, respectively. The large width of the |X3〉 and |X4〉 bands means that the corresponding excitation energies will necessarily lead to contributions from both initial populations. Still, the decay from |X3〉 dominates in panel 4 and the decay from |X4〉 in panel 5.
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Fig. 4 In order to study the population dynamics of specific electronic states, we follow the development of the total real 2D signal as a function of population time and ℏω3, at a number of fixed excitation energies ℏω1 where one electronic state should be dominant (not necessarily the state energy). Each panel can be thought of as a slice along a vertical (constant ℏω1) line through a stack of 2D spectra spaced along a logarithmic time axis. Note that the color schemes of the panels are normalized differently. The gray horizontal lines mark the actual energies of the states according to the fit described in Fig. 2, with the exception of the e–h trap state, the energy of which is unknown (see the text). The blue horizontal lines mark the diagonals in the 2D spectra. The letters are the peak labels from Fig. 1. At right, a summary of the kinetic scheme derived from the slices (see the text) and the identity of the states (according to Norris and Bawendi). Dark blue: hole trapping; dark red: electron and hole trapping; light red: electron and hole (Auger) relaxation. Not all intermediate steps are shown for electron and hole decays, indicated by the dashed line. |
A detailed description of each panel is given in the ESI.† In brief, panels 1–4 show decay directly from the initial (diagonal) states (e.g. the A and B peaks in Fig. 1) to the trap state (the E peak), remarkably without passing through the intermediate states as can be seen from the constant cross-peaks (the C peaks). Trapping occurs on a 50–100 fs timescale, outcompeting hole relaxation which has been shown to have time constants on the order of ∼10 ps.45
2D spectroscopy also allows us to monitor a slower process leading to the disappearance of the negative signal below the diagonal in panel 2 (the negative signal below the A peak in Fig. 1). This can be understood as a process analogous to heterogeneous line shape dynamics in the 2D spectra of chlorosomes,46i.e. as relaxation and equilibration between closely spaced states. Such additional levels within a band appear both in descriptions based on density functional theory17 and when the effective mass model is extended by including crystal anisotropy.47 Additionally, phonons contribute to the level structure.47
Panel 5 presents a more complicated picture, due to the larger numbers of decay pathways theoretically possible from higher energies. |X4〉 is also the first state where the electron is in the 1Pe state rather than the 1Se state, which means that we need to consider both hole and electron relaxation processes in addition to trapping.
The diagonal peak for the |X4〉 state disappears within 20 fs (ESI†). For the 1P3/2 hole, two pathways are possible: the hole could either relax to the 1S3/2 state (a process with time constant ∼10 fs18), from whence it would be trapped, or it could be trapped directly. It seems likely that trapping from 1P3/2 should have a time constant similar to the other hole trapping processes, meaning that relaxation to 1S3/2 should outcompete direct trapping, but the present data do not allow us to clearly distinguish the two scenarios. These hole relaxation processes would occur on the same timescale as the electron decay, giving rise to a number of possible electron–hole state combinations. Their short lifetime and the number of combinations make the spectroscopic identification difficult.
For the 1Pe electron in the |X4〉 state, three decay pathways can be imagined. One is Auger relaxation to the 1Se state, which takes place on a timescale of 150–250 fs.18 Auger relaxation involves energy transfer to the hole, which ends up in a high-energy state such as 2S1/2, and can occur if the hole is not yet trapped. If the hole is trapped, relaxation to the 1Se state is still possible, but takes place via a much slower process (a few picoseconds) mediated by surface states.17,18 Additionally, trapping of the electron might be possible.
Getting back to what we observe in the current measurements, in a broad region around ℏω3 = 17300 cm−1, a strong negative band grows in, i.e. an excited-state absorption signal (the F peak in Fig. 1). Even though it is very strong at high ℏω1, it is negligible at low ℏω1. This means that it should come from a state that is only accessible from high-energy excitons. Two such possible states could be a second hole trap or an electron trap. If it is a hole trap, the signal should be growing after Auger relaxation has brought the holes to otherwise unpopulated high-energy hole states but before hole trapping inhibits Auger relaxation. Considering that the band grows in as a single exponential with a lifetime of 200–300 fs (ESI†), this explanation appears unlikely, and electron trapping from the 1Pe state is instead suggested as the cause. The data cannot reveal the origin of the electron trap; however, clearly the trapping cannot occur for energies close to the band gap, which is also consistent with previous observations.21 P states are on average further from the QD center than S states, so the 1Pe state should be expected to have a better spatial overlap with a trap state on the surface of the QD.
Considering the timescales, Auger relaxation can still be expected to make a minor contribution to the electron relaxation, in competition with the trapping processes. The decay pathway followed by the hole after Auger relaxation would be hard to distinguish from the hole relaxation from the |X3〉 state. The electron would cause a growing bleach in the 16200 cm−1 band, again overlapping with signals from the |X3〉 decay pathway. Finally, a simple calculation can show that the bleach signal (induced by electrons) normalized by the number of e–h pairs is much lower for the |X4〉 state compared to the |X1〉 state. This implies that only a minor part of the electrons excited via |X4〉 reaches the 1Se level. If no electron trapping would occur, this band would be much stronger, further supporting the existence of the trap.
One could imagine that the negative band is in fact constant, but hidden by positive signals at early times. However, excited-state absorption signals can only come from populations, so this scenario would require excitons to remain in the |X4〉 (or possibly |X3〉) state without decaying over the experimental timescale, which is clearly contradicted by earlier experiments.18
Putting this information together, we see that the endpoint of the main |X4〉 decay pathway on a 10 ps timescale is a state where both the electron and the hole are trapped. We call this state |R2〉. Several paths to this state are possible depending on the order of trapping of the carriers and whether |X4〉 relaxes to 1S3/2–1Pe initially. A minor pathway leads via Auger relaxation to the |R1〉 state.
We summarize the initial and final states of all decays in Fig. 3 and show the decay pathways in Fig. 5. 2DES shows that almost all carriers end up trapped – in agreement with the low fluorescence quantum yield (below 10%) of thiol-capped QDs. This contrasts with the relaxation processes in OA-capped QDs.18 In natively MPA-capped QDs with an intermediate density of traps,22 one would expect a more pronounced competition between the two types of pathways.
Footnotes |
† Electronic supplementary information (ESI) available: Sample characterization, average number of excitons per QD (〈N〉), 2D experiments, energy levels, and population dynamics. See DOI: 10.1039/c6cp04190f |
‡ This analogy has to be taken with care since in pump–probe, high spectral resolution in ℏω1 leads to low time resolution in T – a limitation which is avoided in 2D spectroscopy. To achieve the same ℏω1 resolution here using pump–probe spectroscopy, the T pulses would need to be 300 fs long. |
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