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Journal of Nanomaterials
Volume 2011 (2011), Article ID 976262, 5 pages
Structural and Optical Characteristics of γ-In2Se3 Nanorods Grown on Si Substrates
1Department of Physics and Center for Nano-Technology, Chung Yuan Christian University, Chung-Li 32023, Taiwan
2Institute of Nuclear Energy Research, Longtan, Taoyuan 32546, Taiwan
3Department of Electronic Engineering, Chung Yuan Christian University, Chung-Li 32023, Taiwan
4Institute of Optoelectronic Sciences, National Taiwan Ocean University, Keelung 20224, Taiwan
Received 7 July 2011; Accepted 9 August 2011
Academic Editor: Renzhi Ma
Copyright © 2011 M. D. Yang et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This study attempted to grow single-phase γ-In2Se3 nanorods on Si (111) substrates by metal-organic chemical vapor deposition (MOCVD). High-resolution transmission electron microscopy (HRTEM) and selected area electron diffraction (SAED) confirmed that the In2Se3 nanorods are singularly crystallized in the γ phase. The photoluminescence of γ-In2Se3 nanorods at 15 K was referred to as free and bound exciton emissions. The bandgap energy of γ-In2Se3 nanorods at room temperature was determined to be ~1.99 eV, obtained from optical absorption.
The III-VI semiconductors have been the subject of many investigations due to their peculiar electrical and optical properties,and their potential applications in electronic and optoelectronic devices, such as phase-change random access memories (PRAMs), solid-state batteries, and solar cells [1–4]. Among these III-VI semiconductors, In2Se3 is a defective structure of tetrahedral bonding, where one-third of the sites is vacant and forms a screw array along the c axis. Due to many different crystalline phases existing in In2Se3, growth of high-quality In2Se3 with a single phase is a challenging task. Several different methods have been demonstrated to grow In2Se3 epilayers, such as evaporation [5, 6], the Bridgman-Stockbarger Method [7, 8], and metal-organic chemical vapor deposition (MOCVD) [9–11]. Recently, one-dimensional III-VI semiconductor nanostructures, such as nanowires and nanotubes, exhibited novel and device applicable physical properties, which can be used in a wide variety of applications in nanoelectronic and nano-optoelectronic devices [12–17]. For example, α-phase layer-structured In2Se3 nanowires have been grown and have shown a large anisotropy in both structure and conductivity . These III-VI semiconductor nanostructures can afford an efficient charge carrier transfer while maintaining a small cross-section for the applications. However, so far, little attention has been given to γ-phase In2Se3 (γ-In2Se3) nanorods. Bulk γ-In2Se3 has been of particular interest for photovoltaic applications because it can be an absorbing layer in a solar cell. The one-dimensional γ-In2Se3 nanostructures may be more interesting materials since they exhibit excellent light absorption owing to their high surface-to-volume ratio. To be an absorbing layer in solar cells, γ-In2Se3 requires deposition on different substrates with a high crystalline quality. It is well known that Si can be a good substrate to grow nanostructures because it offers many attractive advantages, such as good doping properties and thermal conductivity. If Si substrate can be utilized in growing γ-In2Se3 nanostructures, various devices on Si-based integrated circuits could be developed in the future.
In our previous work, energy relaxation of hot electrons in γ-In2Se3 nanorods has been investigated . It was found that the main path of energy relaxation for the hot electrons is LO-phonon emission. In this study, the detailed structures of the γ-In2Se3 nanorods on Si substrates were investigated by scanning electron microscopy (SEM), transmission electron microscopy (TEM), and selected area electron diffraction (SAED). Also, the optical properties of γ-In2Se3 nanorods were explored by photoluminescence (PL), cathodoluminescence (CL), and the optical absorption spectra.
The γ-In2Se3 nanorods were directly grown on Si (111) substrates without any buffer layers using an MOCVD system with a vertical reactor . The nanorods were grown using liquid MO and a trimethyl-indium (TMIn) compound at atmospheric pressure. Gaseous H2Se was employed as the reactant source material. Gaseous N2 was used as the carrier gas in this process. Before growth, Si substrates were baked at 1100°C for 10 min in gaseous HCl and H2 in order to remove the native oxide. After the thermal etching process, the reactor cooled down to 425°C and then started to grow γ-In2Se3 nanorods. The total growth time was 50 min. The gaseous flow rate was kept at 3 μmol/min for TMIn and 40 μmol/min for H2Se. Gaseous H2Se was mixed with 85% hydrogen and 15% H2Se. The gaseous flow rate and temperature play an essential role in growing nanorod structures in γ-In2Se3. The TEM lattice image and the SAED pattern of an individual In2Se3 nanorod were taken by a JSM-2100F (JEOL Company) Transmission Electron Microscope. The room temperature CL measurement and morphology of the nanorods image were measured by using the JSM-7001F (JEOL Company). The PL measurements were performed using a 532 nm semiconductor laser as the excitation source. The temperature-dependent PL spectra were measured by a close-cycle helium cryostat and were analyzed by means of a 0.75 m monochromator and silicon detector.
A cross-section image of the SEM for the grown In2Se3 nanorods is shown in Figure 1(a). The SEM image was taken with 10 keV of electron energy to present a magnification of 30,000. As shown in Figure 1(a), the In2Se3 nanorods are straight and not tapered. The average diameter and the average height of the In2Se3 nanorods are about 64 and 460 nm, respectively. To understand the structural and morphological characteristics of nanorods, TEM investigations were carried out. Figure 1(b) shows a low magnification TEM image of In2Se3 nanorods. The diameter and height of In2Se3 nanorods are in good agreement with the SEM image shown in Figure 1(a). Figure 1(c) is a high-resolution TEM (HRTEM) image recorded from a segment of an In2Se3 nanorod. The image exhibits the ordering feature across its entire width, with a uniform periodicity of ~1.7 nm. This superlattice structure within the nanorods is a structural characteristic due to the effect of the vacancy ordering . A similar behavior was also reported for the vacancy ordering in α-In2Se3 nanowires and CuInSe2-CdS Core-Shell nanowires [12, 13]. The SAED pattern taken along the  zone axis of In2Se3 nanorods is displayed in the inset of Figure 1(c). The SAED pattern shows a rectangular array with characteristic distances of nm and nm, respectively. These regular spots in SAED suggest an epitaxial orientation relationship between the In2Se3 nanorods and substrates; that is, the In2Se3 nanorods are single crystalline. The SAED pattern is consistent with the previous established pattern for γ-In2Se3 with basis vectors of (−1,1,0) and (0,0,6) . It is noted that the growth direction of the nanowire in Figure 1(c) is not along the  direction, but it makes an angle of 13.7° with respect to the  direction. Anyhow, the HRTEM image allows us to confirm that the grown In2Se3 nanorods are well crystallized in the γ phase.
The PL spectrum of the γ-In2Se3 nanorods on Si (111) substructure at 15 K is shown in Figure 2. Three Gaussian components, peaked at 2.126, 2.147, and 2.155 eV, are resolved in Figure 2. The full width at half maximum (FWHM) of the PL peak at 2.155 eV is 8 meV, indicating good crystal quality for the γ-In2Se3 nanorods. In previous reports, the PL peak of γ-In2Se3 epilayers at low temperatures was referred to as the exciton-related emission . Therefore, the main PL peak positioned at 2.155 eV is suggested to be the free exciton emission and the peaks in the lower energy side are suggested to be the bond exciton emissions. Figure 3 shows the temperature-dependent PL spectra from 15 to 180 K. The peak energy of the PL in γ-In2Se3 nanorods is red-shifted with increased temperature. The open circles in the inset of Figure 3 show temperature-induced bandgap shrinkage extracted from the PL spectra in Figure 2. This relation was fitted by the Varshini Empirical Formula as where is the bandgap at 0 K,is the average temperature coefficient and is the Debye temperature of the material. Experimental data fitting is shown by the solid line in the inset in Figure 3. The experimental results show good agreement with data that fits using Varshini’s Equation with eV, eV/K, and K. By analyzing the variation of PL peak energy as a function of temperature and ability to fit with the Varshini Equation, the room temperature peak energy of the PL in the γ-In2Se3 nanorods was evaluated to be ~1.95 eV.
To explore the bandgap energy of γ-In2Se3 nanorods at room temperature, the CL and optical absorption spectra were investigated. The room temperature CL spectrum of γ-In2Se3 nanorods is shown in Figure 4(a). The peak energy of the CL is 1.95 eV, in good agreement with the predicated value by Varshini’s relation, as displayed in the inset of Figure 3. The optical absorption spectrum taken at room temperature is displayed in Figure 4(b). It is known that γ-In2Se3 is a direct bandgap semiconductor. Thus, the absorption coefficient near the band edge follows the relation of a direct bandgap transition  as where is a constant, is the photon energy and is the energy, gap between the valence band and the conduction band. The bandgap can be derived from extrapolating the linear part of the curve to zero absorption. The straight line in Figure 4(b) shows the extrapolation, and the bandgap energy was estimated to be ~1.99 eV. Obtaining the bandgap energy and absorption coefficient is essential for developing γ-In2Se3 nanorods as absorber layers in photovoltaic applications.
Figure 5(a) shows the PL spectrum of γ-In2Se3 nanorods at 15 K in the infrared spectral range. A broad PL peak located at 1.24 eV was observed. The sharp peak with energy at 1.16 eV is the emission related to the excitation laser. To find out origin of the 1.24 eV PL, the dependence of PL intensity on the excitation intensity was studied. The PL spectra with the excitation power density varied from 17 to 270 W/cm2 were shown in Figure 5. The open circles in Figure 6 show the PL intensity as a function of the laser excitation density, indicating a linear increase of the PL intensity with excitation density. The dependence of the PL intensity on the excitation density can be fitted by a relation : where and are constants. The exponent depends on the mechanism of recombination: for an excitonic recombination , while for free carrier recombination . When , it may indicate a transition associated with the donor-acceptor pair transition or free-to-bound transition [20, 21]. The solid line in Figure 6 displays the fit from (3). A value of was determined to be around 0.6, which corresponds to the emission from the donor-acceptor pair transition or free-to-bound transition. In Figure 6, the PL peak at 1.24 eV shifts to the high-energy spectral region with increasing the excitation density. This blue shift, originating from the increase of the interaction between more closed donor-acceptor pairs, is a characteristic of the donor-acceptor pair transition. Therefore, according to these observations, the observed PL peak at 1.24 eV can be ascribed to the donor-acceptor pair transition in γ-In2Se3 nanorods.
In summary, γ-In2Se3 nanorods deposited on Si (111) substrates were grown by MOCVD using dual-source precursors.The crystal structure and morphology of In2Se3 nanorods were characterized by SEM and HRTEM. The SAED analysis taken along  reveals a rectangle spot pattern, confirming the single crystalline in the γ phase. The optical absorption, CL, and temperature-dependent PL have been investigated. The PL at 15 K contains three peaks, which are identified with recombination of free excitons and bound excitons. The energy of the direct bandgap at room temperature was found to be ~1.99 eV. An infrared PL, peaked at 1.24 eV, was observed in 15 K and assigned to be the donor-acceptor pair transition.
This project was supported in part by the National Science Council under Grant nos. NSC97-2112-M-033-004-MY3 and NSC 97-2627-B-033-002 and the Institute of Nuclear Energy Research under Grant no. 1002001INER042.
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