1 Introduction
Silicon-based light-emitting structures are likely to provide the pivotal technology in future full-silicon optoelectronic integration. Unfortunately bulk silicon is an indirect bandgap (
Eg~1.12 eV) semiconductor which emits light at a negligibly low efficiency. Since the first discovery of visible photoluminescence (PL) from porous silicon at room temperature by Canham in 1990 [
1], arduous efforts have been made to squeeze light from silicon, and a great multitude of exciting results, both theoretical and experimental, concerning the optical and electronic properties of diversified structures have been acquired [
2−
9].
For a long period, the fabrication of nanostructured systems which are expected to give appreciable light emission following the quantum confinement effect (QCE) [
3,
5,
9], as confirmed in size-separated silicon nanoparticles [
2], has attracted much research interest. Various silicon based structures have been investigated in an effort to obtain applicable light emission. These include, for instance, Si nanocrystals in amorphous silicon matrix [
3], free-standing film of silica containing Si nanocrystals [
9], silicon nanoparticles embedded in a diamond matrix [
10], and so forth. So far, PL in the spectral range from infrared to even ultraviolet has been registered in many silicon nanostructures.
As one of the workhorse materials for microelectronics, silicon oxide is the most widely studied among the various matrix choices to quantum confine silicon nanoparticles which are intended to be made into efficient emitting centers. However, the ultimate goal of silicon-based light emitting material design is not the realization of photoluminescence but to obtain applicable electroluminescence. Therefore, carrier injection through the insulating matrix (clearly only possible via the tunneling mechanism) is of practical concern. In this sense, SiO2 is obviously a bad choice because of its extremely large bandgap (Eg~8. 5 eV) — the operation voltage for a light-emitting diode based on Si-in-SiO2 structure would be unacceptably high. To circumvent this difficulty for later implementations, and also to explore the light emission properties of silicon nanoparticles embedded in other materials, the compounds of nonstoichiometrical silicon nitride (Eg~ 5.0 eV), denoted as SiNx, and the stoichiometrical SiC (Eg ranging from~2.3 to 3.4 eV. For the amorphous SiC concerned here, it is~3.2 eV) have been employed and the PL from such composite nanostructures has been extensively investigated in recent years.
In this article, we present a brief review of the progresses along the line of fabricating Si-in-SiNx and Si-in-SiC nanostructures to obtain intense and tunable light emissions via QCE. By using a low-temperature growth procedure, the sizes of the silicon nanoparticles can be reduced down to~1.2 nm, and the external quantum efficiency of PL thereof amounts to over 3.0 %. Moreover, the decay time has been reduced to within one nanosecond.
2 Experimental details
The Si-in-SiNx and Si-in-SiC composite films were deposited onto single-crystalline Si (100) wafers by a custom-designed capacitance-coupled PECVD setup (Fig. 1) operated at an RF power of 35 W and at a typical working pressure of 3.0×10−1 mbar. Precursors are a gas mixture of high-purity SiH4 (diluted with H2 to 2.0 vol. %) and H2 with the addition of N2 for the nitride and of CH4 for the carbide system, respectively. No intentional substrate heating was applied, thus the substrate temperature was maintained at below 60℃ by end of deposition. The film thickness can be controlled by varying the growth time; it generally spans a range of 0.5−1.5 µm. As to the size of the silicon nanoparticles, it can be well controlled by adjusting the plasma conditions through changing the total pressure, the power density and/or the fraction of silane in the precursor, therefore the relevant parameters will be specified at places where it is proper.
The local atomic environments and bonding configurations in the deposits were characterized by infrared absorption measurement performed on a Perkin-Elmer 2000 Fourier-transform infrared system and by inspecting the Si 2p line excited with Mg Kα radiation on an X-ray photoelectron spectrometer (ESCALab Mark-II). Formation of silicon nanocrystals in the films was also verified by micro-Raman scattering using a confocal laser Raman spectrometer (JY-6400). The size and spatial distribution of the innate silicon nanoparticles were investigated from bright-field images obtained with a Tecnai-20 transmission electron microscope (TEM), for which a proper defocus value had to be chosen to accomplish an enhanced contrast. Size determination suffers from a large uncertainty due to the amorphous nature of the silicon particles and the less pronounced particle/matrix absorption contrast.
The as-deposited films would be first examined under an ultraviolet lamp to confirm the presence of PL. Room-temperature PL measurements were carried out on an FLS 920 (Edinburgh Instruments Ltd.) fluorescence spectrometer with a xenon lamp as excitation source. Time-resolved analysis was made on a spectrophotometer (Horiba NAES-1100) with the excitation at 375 nm from a hydrogen lamp (chopper frequency 10 kHz, pulse width 2.0 ns) to determine the decay times at different emission wavelengths registered within less than 1.0 nm. The temporal resolution of the SSU-112 photomultiplier employed is 0.1 ns. As to the external quantum efficiency, it was determined by spectrophotometric measurement with the aid of an integrating sphere which collects both reflected and emitted light without wavelength discrimination. Other parameters or methods associated with the preparation or characterization of a particular sample will be indicated where needed.
3 Si-in-SiNx compound films
By varying the nitrogen-to-silane flow rate ratio between 1.0 and 5.5, we deposited a group of Si-in-SiNx films. Grown under conditions favorable for the formation of distinct silicon particles, the matrix material silicon nitride is generally slightly nitrogen-deficient, that’s why we employ the notation SiNx. According to the X-ray photoelectron spectroscopic and electron energy loss spectroscopic characterizations, the “x” value was found to change only slightly, scattering around 1.10.
The morphology of the as-deposited Si-in-SiNx films was revealed by the SEM micrographs exemplified in Fig. 2. Seen from the cross section and plan view, the film exhibits a compact surface morphology and assumes a good adhesion to the substrate.
The presence of silicon particles in the films can be confirmed by IR absorption measurement and/or by the occurrence of the 520 cm−1 peak on the Raman spectrum. From the high-resolution TEM micrograph (Fig. 3) of a sample grown with gas flow rates (in sccm) SiH4:N2:H2=8.0: 8.0:10, we see that silicon nanoparticles with sharp boundaries are homogeneously distributed throughout the film, with an average size of about 1.8 nm. The density of silicon particles amounts to about 1.07×1013/cm2. Because of the very high number density, some weakly connected clusters of particles have been observed. The particles are quite uniform in size with only a slight fluctuation.
The Si-in-SiNx films prepared with the aforementioned procedure can emit strong blue-violet light which can be easily detected at room temperature. In Fig. 4, the PL spectrum of an as-deposited compound film was displayed against that from a single crystalline GaN sample both excited by the 325 nm line from a He-Cd laser. In comparison with GaN, a remarkable feature for the PL spectrum of the Si-in-SiNx film centered at 428 nm was its relatively enormous width, though their integral intensities were roughly equal. The full width at half maximum (FWHM) is 70 nm for the Si-in-SiNx sample which corresponds to a half-width of 0.47 eV in photon energy, indicating a relatively serious effect of size fluctuation for particles that small.
For the sample containing silicon particles of about 1.8 nm in size, Fig. 5 plots PL profiles obtained under various excitation wavelengths, and the spectral features including the peak position, integral intensity and the full-width-at-half-maximum as functions of the excitation wavelength. The fine-scan PL spectra were achieved with an excitation wavelength between 300 and 450 nm (4.1−2.8 eV) at room temperature. No strong PL can be detected under excitations beyond this range. The emission profile excited by the 300 nm line even extends considerably to below 400 nm, and at the excitation wavelength of 450 nm the peak position of the emission has been approximately shifted, in a roughly linear manner, from 416 to 510 nm [Fig. 5 (a),(b)]. The spectral profiles possess a quite standard Gaussian shape when displayed accordingly versus the photon energy, which facilitates the calculation of the integral intensity and the spectral width from the incomplete emission spectra due to the cut-off at the short-wavelength side. From the curve for the integral intensity variation [Fig. 5(c)], we see that the most effective excitation occurs at~375 nm, as confirmed by the PL excitation spectrum monitored at an emission wavelength of 455 nm (not shown here, see Ref. [
11]). Remarkably, a plateau of emission integral intensity appears within 340 to 410 nm. This implies an enormous flexibility in choosing the excitation source and the emitted wavelengths for applications. The FWHM of the PL profiles increases rapidly at shorter excitation wavelength [Fig. 5(d)]. The data point at 300 nm is unreliable because of the poor profile quality for the very weak emission]. This is quite understandable in the scenario of QCE. The PL under a shorter excitation wavelength clearly involves more particles of smaller sizes, to which an equally large size fluctuation implies an enhanced fluctuation in the energy for the emitted photons. The effect is obviously more pronounced, and asymmetrical, when the spectrum is displayed versus wavelength.
The external quantum efficiency was determined by spectrophotometric measurements using an integrating sphere which collects both the reflected and emitted light of longer wavelength without wavelength discrimination. In Fig. 6, the spectrum of reflectance was measured with a separate spectrometer in a differing wavelength range. The strong multiply-reflected light beam inside the integrating sphere also excited PL from other parts than the sample, resulting in a disturbing contribution to the collected intensity which has to be extracted by the calculation of external quantum efficiency. This disturbing contribution can roughly be calibrated with the same measurements in a stoichiometric Si3N4 sample (not shown here), which exhibits a difference of 6.0 % for the two curves (in percentage of the incident intensity) at the pumping wavelength of 600 nm, where no PL from either the stoichiometric or the nanostructured samples is expected. At 325 nm, for example, the difference between the collected intensity and the reflected intensity is 4.9 %, being slightly less than that at 600 nm. Accordingly, in order to make a cautious estimation of the external quantum efficiency, we assume the same value for the disturbing contribution to the collected intensity at the pumping wavelength of 325 nm as that at 600 nm, i.e., 5.3 % as read from the curves at 600 nm (Fig. 6). At 325 nm, the difference between the collected intensity and the reflected light is about 11.5 %. Taking off the contribution of irrelevant PL, this implies a power ratio of IPL/Iincident≈6.2 %. From the formula , where ≈428 nm is the weight averaged wavelength of PL, and C is a correction factor for the varying detector sensitivity. C is assigned a value of about 0.5, bearing in mind that the PL centers at 428 nm, while the detector manifests a doubled sensitivity at 550 nm than at 325 nm. An external quantum efficiency of over 3.0 % can be consequently derived.
Time-resolved analysis revealed a very short radiative lifetime in the order of 1.0 nanosecond for the Si-in-SiN
x sample concerned here, which is in strong contrast to the porous silicon where the typical decay times for emission are generally in milliseconds. Figure 7 displays an emission spectrum under the excitation of the 375 nm line, together with the decay times for the emissions at various wavelengths. The decay times are the results of fitting the decaying process (see the inset) with a double exponential decaying function, thus there is a long decay time attribute and a short decay time attribute. Such a fitting procedure has been employed by many researchers [
12], to which the tacit assumption is that two decaying paths are responsible for the decaying process. In a model proposed by Calcott
et al. [
13] for porous silicon, it states that the electron — hole exchange interaction splits the excitonic levels by an energy
D due to quantum confinement, and the upper level (a triplet state) and the lower level (a singlet state) have different radiative decay rates [
14]. This model has also been applied to silicon nanoparticles [
15,
16]. Following this model, the energy difference
D is expected to be about a few tens of meV, and the difference in the decay times can be by a factor of 10 in the range of a nanosecond when the silicon particles are about 2.0 nm large, as predicted by Leung [
16]. We see that both the long and short decay times — they differ roughly by a factor within 10 — decrease at longer emission wavelengths, i.e., the decay time is emission wavelength-dependent as found in porous silicon [
17]. Across the emission spectrum, even the long decay times (of roughly the same value as the decay time from the fitting result by using a stretched exponential decaying function) are less than 1.0 ns. This very sensitive response to optical excitation holds potential for the fabrication of silicon-based devices to operate at gigahertz.
4 Si-in-SiC compound films
Silicon carbide as an important semiconducting material possesses potential applications in high-temperature, high-power, high-frequency, and radiation-hardened fields. However, drawing light from silicon carbide has proven to be a very difficult enterprise due to the material’s intrinsic indirect band gap structure. Researchers have manufactured several nanostructures such as quantum wells [
18] and SiC nanocrystals [
19−
21] in order to engineer a direct band gap following the QCE. However, silicon particles survived in silicon carbide matrix should also emit light though SiC will constitute a relatively weaker confinement. The study of light emission from the nanostructured Si-in-SiC compound films will be of essential interest in its own right [
22].
Strong PL were measured in the Si-in-SiC samples thus prepared as the Si-in-SiN
x films, and such a result can be equally attributed to the QCE mechanism based on the analysis of the spectral features. The known characteristic PL emissions attributed to the defects in SiC and SiC nanoparticles [
23] are absent from our results. As a supportive evidence for the QCE mechanism, we noted a steady red shift of the emission in the Si-richer samples comprising enlarged silicon particles. The peak position shifts from 440 nm for sample A to 520 nm for sample C, as seen in Fig. 8. The rather large shift in the emission wavelength,
λ, via a seemingly small change in the particle size,
d, can be well understood from the viewpoint of the QCE model since it has ∆
λ/
λ = 2∆
d/
d. A small change from 1.2 (for sample A) to 1.32 nm (for sample C) in particle size implies an increase of emission wavelength by about 20 %. This enormous shift was also observed in other systems where silicon particles of different sizes clearly exhibit quantum confined emission [
24−
27]. Due to the extreme smallness of the particles, the size fluctuation is expected to produce a considerably broadened profile for the confined PL emission. Therefore the labeling feature of the confined PL can be found in its broadened emission profiles, as shown in Fig. 8. The enhanced size fluctuation equally means a broadened excitation spectrum for the PL process.
Figure 9 displays the PL curves of as-deposited Si-in-SiC film (refer to sample A) measured at different excitation wavelengths ranging from 290 to 515 nm, while no evident luminescence can be detected beyond this zone. Accordingly, the peak position, the integral intensity, and the FWHM are presented as functions of the excitation wavelength [Fig. 9(b), (c) and (d)] in order to analyze the properties of these PL profiles. In so doing, we assume a Gaussian profile for all the PL curves in Fig. 9(a), which is reasonably justifiable as stated in previous sections. In Fig. 9(b) the integral intensity is plotted against the excitation wavelength; it shows a typical binomial distribution (often fitted by a log normal distribution) in the case of small probability for each single event (here an effective excitation) [
28]. The peak position of the PL spectrum is linearly correlated to the excitation wavelength at longer wavelengths, indicating a constant Stokes shift (~1.10 eV), but deviation from linearity occurs at the first three shorter wavelengths since the corresponding photon energies surpass the band gap of the amorphous SiC matrix [Fig. 9(c)]. At the same time, the ever narrowing FWHM of the spectra, given in eV, at the longer excitation wavelength justifies once again the QCE mechanism for the PL process. It drops steadily from 0.35 to 0.16 eV [Fig. 9(d)]. This point has been discussed in detail in our previous publications concerning silicon particles embedded in SiN
x matrix [
24,
25,
29]. Note that the emission spectrum that extends to the violet band (below 400 nm or 3.1 eV in photon energy) loses intensity rapidly, and the corresponding photon energy has approached the band gap of the amorphous silicon carbide prepared under similar conditions (≤3.3 eV) [
30]. Therefore, we can say that the PL emission centered at 460 nm is of roughly the shortest wavelength that can be achieved in the Si-in-SiC composite structure via the quantum confinement mechanism.
The QCE mechanism for light emission from the extremely small Si particles may also indicate a very short decay time, of the order of a nanosecond, in the Si-in-SiC. Figure 10 illustrates a typical decaying process for the emission collected at the 485 nm line under the excitation of 390 nm. The decay times are obtained by fitting the decaying process with a double exponential decaying function as before. We found that, at the four chosen wavelengths for the collected emission, the decay time for the short-time attribute is 2.41 ns (390 nm), 2.63 ns (410 nm), 2.22 ns (465 nm) and 3.62 ns (505 nm), respectively. The decay time for the long-time attribute is also well below 10.0 ns. Such a short decay time, though roughly doubled as was reported on Si-in-SiN
x, is considerably shorter than those measured in porous silicon and in silicon particles embedded in oxide matrix. Noting that the two components of the decay time here are of the same order of magnitude, an alternative fitting using the stretched exponential function [
31] seems more appropriate which, to no surprise, gives a decay time of a similar size. But again, a clear picture for the underlying dynamic recombination processes is missing. This can only be resolved with more detailed measurements of the decay and excitation processes in the future.
5 Summary
In summary, silicon particles with an average size below 2 nm were grown onto cold substrates in amorphous SiNx and SiC matrices by employing a plasma-enhanced chemical vapor deposition procedure, which can serve as an exemplar system for the study of light emission following QCE. Strong PL extending to the violet band can be measured at room temperature, and an external quantum efficiency of over 3.0 % can be reached. The strong confinement implies a very short decay time which declines even to within 1.0 nanosecond in the Si-in-SiNx systems. The extremely small size of the silicon nanoparticles gives rise to emissions of considerably extended spectral profiles, in Si-in-SiC films comparable profiles can be obtained in one same sample with a flexible choice of excitation wavelengths. These features largely reinforce the feasibility of fabricating silicon-based nanostructured light-emitters in a procedure entirely compatible with modern very-large-scale-integration technology.
Higher Education Press and Springer-Verlag 2008