Chin-An
Lin
,
Dung-Sheng
Tsai
,
Cheng-Ying
Chen
and
Jr-Hau
He
*
Graduate Institute of Photonics and Optoelectronics, and Department of Electrical Engineering, National Taiwan University, Taipei, 10617, Taiwan (ROC). E-mail: jhhe@cc.ee.ntu.edu.tw; Fax: +886-2-2367-7467; Tel: +886-2-33669646
First published on 24th January 2011
Surface plasmon (SP) mediated emission from ZnO nanorod arrays (NRAs)/Ag/Si structures has been investigated. The ratio of visible emission to UV emission can be increased by over 30 times via coupling with SP without deterioration of the crystal quality. The fact that the effect of SP crucially depends on the size of Ag island films provides the feasibility to significantly enhance the yellow–green emission of the ZnO nanostructures without sacrificing the crystallinity of ZnO.
Ag is well known for its strong interactions with visible light via the resonance of the oscillations of the electrons within the particles. These local electromagnetic fields near Ag can be many orders of magnitude higher than the incident fields, which include so-called surface plasmons (SPs). Generally SP-enhanced emission involves two sequential processes. Firstly, the excited energy in the emitter is transferred into SPs instead of photons. The resonant coupling of the excited states into SPs occurs when the energy of the excited states in the semiconductor approximates the SP energy of the metal layer.16 Secondly, SPs radiate light to far field if the momentum values match.16,17 In contrast, SPs are unable to generate photons directly while the momentum values of SPs and light do not match. Consequently, the SP energy trapped at the interface is dissipated as heat, leading the reduction of the luminescent efficiency.17 However, SP-mediated energy can be transferred by some methods. For example, as the grating structures with the periodicity or the interface corrugation are introduced appropriately, these SPs alter their momentum and thus couple to light, leading to the enhanced luminescent efficiency for light emission devices.16 Since metal-capped thin-film structures of emitters are usually adopted,18–21 it is difficult to investigate the influence of the interface roughness which is essential to enhance emission. To our knowledge, the effect of interface corrugation on the luminescent enhancement of ZnO nanostructures has not yet been investigated.
In this study, based on the ZnO NRAs/Ag/Si structure using a low-temperature hydrothermal method, the investigation on the effect of interface morphology on the enhancement of SP-mediated emission becomes possible without altering the crystal quality. The ratio of visible emission to UV emission can be increased by over 30 times via coupling with SPs. To examine crystal quality and chemical information of the surface of ZnO NRAs, X-ray diffraction (XRD) and X-ray photoelectron spectroscopy (XPS) have been performed. The use of SPs paves the way for further development of the ZnO NRA-based light emitting devices.
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Fig. 1 The cross-sectional SEM images of ZnO NRAs grown on Ag/Si substrates with various thicknesses of Ag island films. The insets are the corresponding morphologies of Ag island films on Si substrates after annealing at 300 °C in air for 25 min. |
The structure of the as-synthesized NRAs was determined by XRD analysis. Fig. 2 shows the XRD pattern of the as-grown NRAs. A strong peak locates at 34.52° for the diffraction from (002) plane of ZnO. The recognizable peaks at 31.78°, 36.32°, 47.72° and 63.96° refer to the (100), (101), (102) and (103) planes of ZnO, respectively. All of the diffraction peaks for all samples can be ascribed to the wurtzite ZnO structure with lattice constants of a = 0.3249 nm and c = 0.5205 nm, consistent with the standard data file (JCPDS 05-0664). It can be inferred that all ZnO NRAs were preferentially oriented in the c-axis direction.
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Fig. 2 The XRD patterns of ZnO NRAs grown on Ag/Si substrates with the various thicknesses of the Ag films. |
As the substrate has a high refractive index and/or high absorption coefficient, the information contained in the extinction spectrum can be quite poor. We use the fused silica as the substrate instead of the silicon. The absorption spectra allow the observation and characterization of the excited SP resonance modes.23Fig. 3 shows the UV-visible absorption spectra of various Ag island films/fused silica substrates with and without 5 nm thick ZnO seed layers after annealing samples at 300 °C in air for 25 min. Larger Ag islands lead to the redshift of the absorptance maximum with increasing intensity. The broad absorption spectra are due to the irregular size of the Ag islands. In addition, it has been previously described that the optical properties of Ag nanoparticles depend on the external dielectric constant.24–26 By taking into account of the difference of dielectric constants between ZnO and air, one can see that different resonance frequencies between ZnO/Ag and air/Ag are obtained, i.e., the resonance frequency redshifts as the dielectric constant of the surrounding medium is increased, as shown in Fig. 3. Ag islands act as radiative antenna coupling SP into light emission.27 Generally, smaller Ag islands lead to higher SP resonance energies. As the size of Ag islands is increased with the large variation in the surface roughness, the redshift of the absorbance maximum and large inhomogeneous broadening are observed.28,29 Similar results were also investigated experimentally and theoretically in the Ag/ZnO nanocomposite films.23
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Fig. 3 The absorption spectra of Ag island films/fused silica substrates, and the 5 nm thick ZnO films/Ag island films/fused silica after annealing at 300 °C in air for 25 min. |
Fig. 4 shows a comparison of PL spectra of ZnO NRAs on 5, 10, and 30 nm thick Ag island film/Si and bare Si substrates. A control sample only consisting of ZnO NRAs on the Si substrate shows a typical PL spectrum of ZnO with a strong NBE emission at 382 nm and weak yellow–green emission at 568 nm from the deep levels related to a complex of an oxygen vacancy and zinc interstitial.9,30 Note that the peak at 760 nm results from the second-order feature of the NBE emission of ZnO. One can see that the yellow–green emission increases greatly with the thickness of the Ag island films. It has been reported that the intensity of deep level emission was enhanced while the diameter of nanowires was decreased (i.e., surface area was increased).31 In our study, however, large-diameter ZnO NRAs with the aid of the Ag films show a significant enhancement of the deep level emission, which is different from previous reports.31 We can exclude the possibility that the giant enhanced yellow–green emission is caused by the density of deep level traps. The ratio of visible emission to UV emission of ZnO NRAs with the thickness of Ag island films is listed in Table 1.
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Fig. 4 The PL spectra of ZnO NRAs on bare Si substrate and Ag/Si substrates with the various thicknesses of the Ag films. |
Thickness of Ag films (nm) | Ratio of visible emission to UV emission |
---|---|
0 | 0.32 |
5 | 1.72 |
10 | 5.35 |
30 | 10.11 |
It has been known that the recombination of deep levels responsible for visible emission in ZnO nanostructures is located at the surface (<30 nm in thickness).31 To judge if the enhancement of yellow–green emission is related with the deteriorated crystal quality, the results of XRD and XPS were investigated. Fig. 2 presents the XRD pattern of the ZnO NRAs grown on a Ag/Si substrate. Stronger ZnO (002) peak was observed in all Ag/Si substrates than that on bare Si substrates, which demonstrated that the crystal quality of the ZnO NRAs was somewhat improved when it was deposited on an Ag interlayer. XPS, also known as electron spectroscopy for chemical analysis, is a widely used technique for obtaining chemical nature from the material surfaces (3–5 nm in depth) with the detection limit of 1 at.%. Fig. 5 shows the O 1s and the Zn 2p3 core level spectra of ZnO NRAs on Ag island films/Si and bare Si substrates. The binding energy of the O 1s and Zn 2p3 were recorded to be 530.8 eV and 1022.2 eV, respectively. Since the number of photoelectrons of an element depends on the atomic concentration of that element in the samples, XPS is used to not only identify the elements but also quantify the chemical composition. Moreover, the XPS measurements have been carried out to investigate the chemical states of the O 1s and Zn 2p3 in the ZnO.32–35 O 1s of ZnO NRAs can be deconvoluted by three nearly Gaussian curves, centered at 530.1, 530.8, and 531.9 eV in all samples. An example is O 1s of ZnO NRAs without Ag island films as shown in Fig. S2.† The high binding energy component located at 531.9 eV is usually attributed to chemically absorbed oxygen on the surface of the ZnO NRAs. The component near 530.1 eV is attributed to O2− ions surrounded by Zn atoms with their full complement of nearest-neighbor O2− ions. The intensity of this component is related to the amount of oxygen atoms in a fully oxidized stoichiometric surrounding. The binding energy component, centered at 530.8 eV, is associated with the amount of O2− ions in the oxygen deficient regions within ZnO NRAs. Therefore, the change in ratio of intensities of three components can be connected to the variations in the concentration of oxygen deficiencies. In the present study, the quite similar shape of O 1s leads to an invariable ratio of intensities of three components in all samples, indicating that the concentration of oxygen deficiencies was not varied with the thickness of Ag island films. After the value of peak intensity (the peak area after background removal) is obtained, the atomic concentration of an element (Ci) can be expressed as:
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Fig. 5 The XPS spectra of (a) O 1s and (b) Zn 2p3 core levels of ZnO NRAs on Ag/Si substrates with the various thicknesses of the Ag films. |
Thickness of Ag films (nm) | Atomic concentration of oxygen (%) | Atomic concentration of zinc (%) |
---|---|---|
0 | 46.01 | 53.99 |
5 | 47.40 | 52.60 |
10 | 47.60 | 52.40 |
30 | 47.86 | 52.14 |
It has been found that scattering cross section of the SP increases with the square of metal island volume.36 With the increase of the Ag island size, the scattering efficiency of the SPs is raised. Thus, we attribute this enhancement to SP-mediated emission, in which the deep level emission within ZnO NRAs couples into the SP modes at the Ag/ZnO interface when the excited energy and the SP energy are similar. Then, the spontaneous recombination produces SPs instead of photons. The coupled SP energy can be recovered as free space photons when the interface is rough appropriately to scatter the photons. The ratio of visible emission to UV emission can be increased by over 30 times via coupling with SPs. Moreover, the decrease of UV emission with the increasing thickness of Ag island films was observed. It can be attributed to the enhanced recombination rate of the deep level emission due to the coupling of the emission with SPs at the Ag-ZnO surface. The recombination rate is enhanced through the ZnO-SP coupling rate, which is expected to be very fast compared to the radiative and nonradiative recombination rates.37 Thus, the UV emission is quenched while the visible emission is enhanced. In addition, this difference of enhanced ratio of visible emission to UV emission disproves the possible attribution of the stronger PL intensity of ZnO NRAs to the metal reflection.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/c0nr00732c |
This journal is © The Royal Society of Chemistry 2011 |