Kaiyang
Wang†
a,
Shang
Sun†
b,
Chen
Zhang
b,
Wenzhao
Sun
a,
Zhiyuan
Gu
a,
Shumin
Xiao
*b and
Qinghai
Song
*ac
aIntegrated Nanoscience Lab, Department of Electrical and Information Engineering, Harbin Institute of Technology, Shenzhen, 518055, China. E-mail: qinghai.song@hitsz.edu.cn
bIntegrated Nanoscience Lab, Department of Material Science and Engineering, Harbin Institute of Technology, Shenzhen, 518055, China. E-mail: shumin.xiao@hitsz.edu.cn
cState Key Laboratory on Tunable Laser Technology, Harbin Institute of Technology, Harbin, 158001, China
First published on 19th August 2016
Lead halide perovskite based micro- and nano-lasers have been widely studied in the past two years. Due to their long carrier diffusion length and high external quantum efficiency, lead halide perovskites have been considered to have a bright future in optoelectronic devices, especially in the “green gap” wavelength region. However, the quality (Q) factors of perovskite lasers are unspectacular compared to conventional microdisk lasers. The record value of full width at half maximum (FWHM) at the threshold is still around 0.22 nm. Herein we synthesized solution-processed, single-crystalline CH3NH3PbBr3 perovskite microrods and studied their lasing actions. In contrast to entirely pumping a microrod on a substrate, we partially excited the microrods that were hanging in the air. Consequently, single-mode or few-mode laser emissions have been successfully obtained from the whispering-gallery like diamond modes, which are confined by total internal reflection within the transverse plane. Owning to the better light confinement and high crystal quality, the FWHM at the threshold has been significantly improved. The smallest FWHM at the threshold is around 0.1 nm, giving a Q factor over 5000.
While the lead-halide perovskite lasers have been widely studied in polygon microcavities,14–17 microrods,11–13 nanorods,10 spherical cavities,19 as well as random lasers in microcrystal networks or clusters,20,21 their quality (Q) factors are usually much lower than conventional microlasers. The reported full width at half maximum (FWHM) at the lasing threshold in hexagonal microdisks and square microdisks is usually larger than 0.5 nm.14–17 In 2015, Zhu et al. improved the crystal quality of perovskites and reduced the FWHM at the threshold to record low values around 0.22 nm.10 However, this value is still far from that of GaAs based circular microdisks or deformed microdisks.22 Herein, we synthesize CH3NH3PbBr3 perovskite microrods and study their lasing actions. In general, the quality factor is dependent on the absorption loss, radiation loss, and scattering loss following the equation 1/Q = 1/Q_rad + 1/Q_sca + 1/Q_abs. The absorption loss and scattering loss can be decreased by improving the crystal quality, whereas the radiation loss is mostly associated with the resonators and some additional mechanisms. By improving both the crystal quality and the cavity design, we have further decreased the FWHM at the lasing threshold to around 0.1 nm, giving a Q factor over 5000.
Then the optical properties of the synthesized microrods were studied by optically exciting them under a home-made micro-photoluminescence system (see Experimental section). We first tested the conventional Fabry–Perot (F–P) modes along one microrod on the substrate. With the increase of pumping power, sharp peaks emerged in the laser spectrum. However, as we have reported recently, these F–P lasers usually have very large FWHM and very low factors (∼a few hundred).12 These kinds of low Q factors can be simply understood. The F–P mode along the axis of the microrod is usually confined by the reflections between two end-facets. While the refractive index of lead halide perovskites is relatively high (n ∼ 2.55), the transmission losses are still large. In this sense, the Q factors of F–P modes along the axis of the microrod are usually low and they are unable to support high Q lasers.
In addition to F–P modes, the cross-sections of perovskite microrods are large enough to support other types of resonances in the transverse plane. In general in microrods or nanorods, such kinds of resonances cannot be excited because F–P modes have much longer amplification lengths. In some particular designs, the F–P modes can be suppressed and the transverse lasing modes can be excited. One example is shown in Fig. 2. From the SEM image in Fig. 2(a), we can see that several microrods join together and form a big cross. As the reflections of waveguide modes between two end-facets will be broken at the joint position, the radiation loss of F–P modes along the arms of the cross increases significantly and the Q factors of F–P modes are strongly reduced. Fig. 2(b) shows the recorded laser spectra of the cross by partially pumping the selected microrod (see Fig. 2(a)). When the pumping density is low, a broad photoluminescence peak is achieved. With the increase of pumping power, a few narrow peaks appeared around 556.4 nm and quickly dominated the emission spectra. One additional laser peak appeared with a further increase in pumping power. The spectra of light emissions from partially pumped microrods are quite different from the reported F–P microrod lasers and are well consistent with the above analysis.
The emergence of narrow peaks usually corresponds to the transition from spontaneous emission to lasing actions. And this kind of transition can be seen more clearly in Fig. 2(c). When the pumping density is below 2.37 μJ cm−2, the slope of output intensity is around 0.8. Once the pumping density is above 2.37 μJ cm−2, the slope dramatically increases to ∼8. The superlinear slope and the sharp peaks clearly demonstrate a threshold behavior at 2.37 μJ cm−2. The squares in Fig. 2(c) illustrate the laser FWHM as a function of pumping density. When the pumping density is below the threshold, the FWHM is over 30 nm, which is well consistent with the spontaneous emission. Once the pumping density is above the threshold, the FWHM is dramatically reduced by more than two orders of magnitude. Due to the band filling effect,23 the FWHM increased again above the threshold. Thus the smallest FWHM at the threshold, which is as small as 0.132 nm, is achieved at the laser threshold. This value is almost half of the previously reported record narrow laser peak and gives a high Q factor around 4200. The FWHM and Q factor can be even further improved by getting rid of the instrumental broadening of our spectrometer (∼0.11 nm).
We know a surprising fact that the FWHM can be simply improved by exciting the transverse lasing modes. To understand the experimental observations, we have numerically studied the microrods using finite element method based commercial software (Comsol Multiphysics 3.5a).24 All the parameters of perovskite microrods are taken from SEM images. Considering the situation of microrods, a two-dimensional object has been employed to mimic the lasing properties. Both the width and thickness of the selected microrod under consideration are 1.964 μm. The refractive index of perovskites is fixed at 2.55. As the microrod is standing on one edge, the surrounding medium is set as n = 1. Following the experimental results, only transverse electric (TE) modes are considered. Fig. 3(a) shows the calculated Q factors (Q = Re(ω)/2|Im(ω)|, here ω is the resonant frequency) around the gain spectral region. We can see that most of the resonances have relatively low Q factors except modes 1–3 marked in Fig. 3(a). This is because the resonances inside rectangle shaped microcavities follow the equation:24
(1) |
Fig. 3 Resonant modes in the transverse plane of microrods. (a) The calculated Q factors of resonances inside the transverse plane of the microrod marked in Fig. 2(a). (b) The field distribution (|Hz|) of mode-2 in (a). |
We note that the high Q factors are not limited in this particular sample. Similar phenomena have been widely observed in a number of microrods. Parts of the results are shown in Fig. 4. Here we excited the transverse lasing modes of microrods suspending in air. The samples could be found from randomly synthesized perovskite microrods or constructed by placing the microrods on a perovskite block with one end suspending in the air via micro-manipulation.12 Because the perovskite block can introduce significant radiation loss in the longitudinal direction, the F–P lasing modes can also be suppressed and transverse modes are excited. From the insets in Fig. 4(b), (d) and (f), we know that these microrods are also quite uniform and flat, providing the chances to reach small FWHM. The experimental results are shown in Fig. 4. While their exact transverse shapes and thresholds are different, their FWHMs at the lasing threshold are always around 0.1 nm. The details of microrod sizes, and measured and numerically calculated Q factors are listed in Table 1. It should be noted that the lasing spectra shown in Fig. 4 were taken above the threshold to maintain a high signal to noise ratio (SNR). Considering the band filling effect,23 the FWHM at the threshold is the smallest. To obtain the exact and true FWHMs, the FWHMs (corresponding to Q factors) in Table 1 are extracted at the lasing threshold. We know that the smallest FWHM can be as small as 0.1 nm, giving a Q factor over 5000. Interestingly, we found that almost all the calculated Q factors were much larger than the experimentally measured values. This means that the current Q factors are limited by the material instead of the cavity shape again and thus they can be further increased by improving the crystal quality.
Sample # | Width (μm) | Height (μm) | Q_mea | Q_sim |
---|---|---|---|---|
1 | 1.469 | 1.394 | 5968 | 8763 |
2 | 1.537 | 1.456 | 5697 | 5175 |
3 | 2.573 | 1.897 | 4971 | 27506 |
4 | 2.516 | 2.516 | 4846 | 257561 |
5 | 1.491 | 1.491 | 4417 | 15744 |
6 | 0.895 | 0.895 | 4384 | 4205 |
7 | 5.969 | 0.7 | 4380 | 3332 |
8 | 1.303 | 1.303 | 4302 | 8973 |
9 | 2.886 | 2.886 | 4215 | 330205 |
10 | 1.401 | 1.401 | 4207 | 26967 |
One may also wonder why the high Q factors have not been observed in the microplate lasers, whose resonances are also confined by total internal reflections.14–17 In principle, the microplates have much larger cavity sizes and should have much larger simulated Q factors. But the experimentally recorded FWHMs are usually around or far larger than 0.5 nm.14–17 Some values are almost an order of magnitude larger than our observations.14–17 This deviation is generated by the substrate. Different from the microrod in Fig. 2(a), all the microplates are attached on the substrate after the synthesis. Thus the influence of substrates must be considered. Compared with the two-dimensional calculation, there are vertical losses to the substrate. Sometimes, the vertical losses are even much larger. For example, when the microrod in Fig. 3 is placed onto a glass substrate, the Q factor of mode-2 will be degraded by more than an order of magnitude. Once the ITO (n = 1.8) layer on the substrate is considered, the Q factor is even lower. Meanwhile, most substrates cannot be as flat as the single-crystalline samples. Additional scattering losses will also decrease the cavity Q factors. In addition, there are always some flaws in synthesized devices (see insets in Fig. 4(a), (c) and (e)). The transverse modes can be selectively formed at the flawless positions. However, the resonances in microplates and F–P modes in microrods cover most of the devices and cannot fully avoid such scattering centers. Therefore, long-lived resonances are much easier to be formed in the transverse planes of freestanding microrods than F–P modes in microrods and whispering gallery like modes in microplates.
Footnote |
† These two authors contributed equally to this manuscript. |
This journal is © the Partner Organisations 2017 |