Anyssa
Derj
a,
Hélène
Magnan
a,
Cristian
Mocuta
b,
Patrick
Le Fèvre
b,
Jocelyne
Leroy
c and
Antoine
Barbier
*a
aUniversité Paris-Saclay, CEA, CNRS, Service de Physique de l'Etat Condensé, F-91191 Gif-sur-Yvette, France. E-mail: antoine.barbier@cea.fr
bSynchrotron SOLEIL, l’Orme des Merisiers Saint-Aubin - BP48, F-91192 Gif-sur-Yvette Cedex, France
cUniversité Paris–Saclay, CEA, CNRS, NIMBE, F-91191 Gif-sur-Yvette Cedex, France
First published on 8th February 2022
Epitaxial perovskite self-oxidized oxynitride N:BaTiO3 thin films, deposited on 1% Nb-doped SrTiO3(001) single crystals, were obtained by atomic nitrogen assisted molecular beam epitaxy without supplying additional oxygen gas. Their growth, crystalline and electronic structures as well as photo-electrochemical and optical properties were investigated and compared to those of pure BaTiO3 films grown with atomic oxygen on the same substrate. More tetragonal perovskite crystalline structures, profound electronic structure modifications, improved photo-electrochemical properties and an enhanced (almost 10%) optical window for light absorption are demonstrated. This new class of compounds shows promise for a large panel of new applications based on visible light absorption.
Producing epitaxial oxynitride thin films is however very challenging. Solid-state chemistry methods use high temperature ammonia nitriding of oxide powders to produce oxynitride powders that are not easy to process further. As a matter of fact, nitriding is thermodynamically far less favorable than oxidation.6 In the present paper, we propose a new method by using atomic nitrogen plasma and an oxide substrate that will provide the required oxygen for the growth of oxynitride N-doped BaTiO3 epitaxial films, which is otherwise unfavourable because of the lattice charge imbalance. We report investigations of the influence of the N doping on the crystalline structure, electronic structure and photoanode properties for photoelectrolysis of water and discuss our observations especially in the light of the comparison with undoped BaTiO3 films of identical thickness realized with atomic oxygen plasma.7 Here we demonstrate that growing epitaxial single crystalline perovskite N doped BaTiO3 (N:BTO) is possible through this new method and that even modest doping leads to substantial and potentially useful material modifications.
Bulk BaTiO3 exhibits a ferroelectric to paraelectric phase transition at about 130 °C accompanied by a tetragonal to cubic structural transition.8 The ferroelectric phase can be stabilized at higher temperatures in strained epitaxial layers.9 In previous studies,10,11 we showed that epitaxial BaTiO3 thin films are well suited for studying the influence of the electric polarization on the photoelectrochemical properties. To get around the limitation of a large band gap, efforts were devoted to the modification of the electronic structure of BaTiO3via doping. Nitrogen-doping has proven to be an efficient method to decrease the optical band gap for several wide band oxides12 including BaTiO3.13 More generally, combining oxides and nitrides into a single material can be promising to improve the photoanode properties by providing a new class of materials without the drawbacks of oxides and semiconductors. However, realization of such oxynitride compounds remains very challenging with conventional methods.
The N:BTO layers’ crystalline structure was investigated by X-ray diffraction (XRD) and X-ray Reflectivity (XRR) measurements realized at the DiffAbs beamline, Synchrotron SOLEIL (France). The study was done at room temperature and at a photon energy of 9 keV. The instrumental broadening was determined from measurements (in capillary geometry) realized on a National Institute of Standards and Technology (NIST) standard (LaB6 powder) and was found within 0.02°–0.04° up to the highest value of accessible 2θ (i.e. 120°). The instrumental contributions to the observed peak broadenings (>1°) were thus negligible. The significant digits of lattice parameters, 0.002 Å, were determined from the maximal deviation from the average value (over all accessible orders) of the substrate fitted (Lorentzian peak shape) Bragg peak positions. All XRD peak positions were derived from the Lorentzian shape fits to the experimental data after χ2 convergence.
The photoelectrochemical (PEC) response of our films was studied using a three electrode cell with a flat quartz window.16 Undoped and N-doped BaTiO3 films, and a bare SrTiO3 substrate were used as the working electrode and mounted in a sample holder designed to prevent any contact between the substrate and the electrolyte. A Pt wire and an Ag/AgCl electrode were used as the counter and the reference electrodes respectively. A 0.1 M NaOH solution was used as the electrolyte. The measurements were carried out using a potentiostat (PAR 263) at a scan rate of 50 mV s−1. The light source was a 1000 W xenon arc lamp source with an infrared (IR) water filter, and the intensity of the light on the sample was evaluated to amount to around 100 mW cm−2. All PEC measurements were performed at room temperature. The photocurrent (Jph) is defined as the difference between the current recorded under light and without light (dark).
The measure of the photocurrent as a function of the wavelength was carried out under monochromatic light, at a bias voltage of 0.5 V vs. Ag/AgCl using a Cornerstone 130 model 74004 monochromator (Newport). The wavelength was varied between 200 and 600 nm, with 5 nm steps. In order to increase the signal to noise ratio, we used modulated light. More precisely we used a PAR 5210 lock-in amplifier and an optical chopper at a reference frequency of 20 Hz.
Further investigations were performed using AES. The AES spectra recorded after growth are reported in Fig. 1b for doped and undoped samples. The spectra are very similar. The uncorrected TiLMM/BaMNN ratio is 1.3, which is close to the expected value for a 1:1 stoichiometry for Ti:Ba as it was reported in the literature.7,17 A closer inspection of the Auger spectra shows that the TiLMV peak presents two components with slightly different relative intensities, which were widely used to determine changes in the stoichiometry of Ti compound surfaces, as well as variations in the surface oxygen stoichiometry after metal deposition.18 Rao et al.19 considered the evolution of the TiL2,3M2,3V Auger spectra through a series of compounds presenting a gradual reduction of the titanium ion from TiO2 to metallic titanium. The spectrum evolves from a unique line around a kinetic energy of 408 eV in TiO2, to a unique line at around 414 eV in metallic titanium. By convention, when the metal is oxidized, the low kinetic energy component has been assigned to a so called “interatomic L3MV(O)” decay, while the other (metallic) component has been associated with an “intra-atomic L3MV(Ti)” process20,21 where V(O) and V(Ti) refer to O and Ti contributions to the oxide valence band, respectively. One observes in Fig. 1(c) that the first component is reduced in the N doped sample suggesting less oxidized Ti species in this sample. Importantly, such a modification of the electronic structure suggests an incorporation of the N atoms in the lattice of the material and/or oxygen vacancies.
The crystalline structure of the N:BTO layers was investigated by X-ray diffraction (XRD) and X-ray reflectivity (XRR). Fig. 2a shows the reflectivity curve as a function of the wave vector transfer Qz, measured on the N:BTO film as well as the calculated reflectivity for the best fit model (straight line) refined using the REFLEX software.22 While a single layer model failed to represent the data, a simple 2-layer model allowed the reproduction of experimental measurement very well (χ2 = 0.007). The best fit gives a homogeneous layer of thickness 12 nm covered by a surface layer of 2 nm with a lower density. The inset in Fig. 2a reproduces the density profile of the best fit model. The substrate roughness was 0.27 nm r.m.s. and the top layer roughness was of ca. 0.33 nm r.m.s. Given the growth method, the sharp layer model obtained here is a striking feature.
Fig. 2b shows the wide angle XRD patterns of the N:BTO sample. All Bragg peaks could be well fitted using Lorentzian shaped peaks. The widths of the diffraction peaks of SrTiO3(001) are limited by the instrumental contribution and are thus very sharp and point out the high crystalline quality of the single crystalline substrate. The specular Bragg peaks of N:BTO appear in the form of broad peaks on the low L side of the Nb:SrTiO3 Bragg peaks and contain information about the film thickness and strain.23–26 Epitaxial single crystalline films only exhibit a single family of Bragg peaks along [00L] limiting the number of peaks that can be taken into account in a structural size–strain nanoparticle analysis.27 The peak widths and positions were determined and reported in the corresponding Scherrer plot (refer to Fig. S1 in the ESI†), which leads to an average particle size of (10.1 ± 2.7) nm which is essentially close to the film thickness. Thus, the widths of the specular peaks are dominated by the finite film thickness preventing the extraction of information about the strain in the layer. Indeed, broad peaks in the perpendicular reciprocal space are intrinsically expected for films of reduced real space thickness. Rocking scans, measured for all accessible specular Bragg peaks, revealed very narrow peaks (∼0.022°) limited by the experimental resolution stressing the high crystalline quality of the layer. The film exhibited also well-defined in-plane Bragg peaks (Fig. 2b inset) accessible in grazing incidence geometry, i.e. at an incidence angle of 0.5°, which is close to two times the critical angle for total external reflection at the measurement photon energy. In surface plane rocking scans were performed on all accessible peak positions. The in-plane Bragg peaks widths (full widths at half maximum, FWHM), Δ, decrease steadily with increasing momentum transfers. They are indeed expected to follow equation Δ2 = Ω2 + (2π/(Q × D))2, where Ω is the in-plane mosaic spread (i.e. a constant angular width), and D a finite domain size, which leads to a constant broadening with respect to the momentum transfer, Q, and is related to the angular width Δω by D = 2π/(Q × Δω). Both values can be easily retrieved from the linear fit to the Δ2 = f(1/Q2) plot (refer to Fig. S2 in the ESI†).28 For our layer we obtain a mosaic spread as small as 1.27° and a domain size of 7 nm, confirming the epitaxial single crystalline nature of the layer. The lattice parameters were determined from the averaged Bragg peak positions and were a = (0.398 ± 0.001) nm and c = (0.408 ± 0.003) nm. As is illustrated in Table 1, the doped layer is significantly more tetragonal (c/a = 1.025) than the undoped one (c/a = 1.010).7 This difference may find its explanation in the substitution of oxygen by nitrogen atoms in the lattice due to the charge imbalance and an increased presence of vacancies. Also for AES, these results suggest that N has been incorporated in the lattice of the N:BTO layer.
Sample | a (nm) | c (nm) | c/a | Electrochemical band gap (eV) |
---|---|---|---|---|
BaTiO3 | 0.399 | 0.403 | 1.01 | 3.62 ± 0.01 |
BaTiO3−yNy | 0.398 | 0.408 | 1.025 | 3.61 ± 0.01 |
The electronic structure of our N:BTO layer was examined by XPS measurements and compared with that of the well documented BTO case.29–36 The main photoemission peaks are represented in Fig. 3 for doped and undoped samples. Both samples showed a main O-1s line at 529 eV binding energy (refer to Fig. S3 in the ESI†). While this line cannot be quantitatively interpreted because of the air exposure, its overall shape remains of interest to evidence the presence of a well marked contribution at lower binding energy. The main O-1s line positions were found to be symmetric, which indicate a well defined single electronic state for the oxygen atoms incorporated into the oxide structure. With respect to Ti-2p the intensity of the integrated O-1s XPS peak is 1.8% lower for the N-doped BaTiO3 layer which is consistent with the partial substitution of O by N. The N-doped film displayed a N-1s XPS peak (Fig. 3b), which can be decomposed into two components. The peak observed at binding energy 398.3 eV can be ascribed to Ti–O–N bonds or surface adsorbed nitrogen while the peak located at 395.5 eV can be assigned to Ti–N bonds.37 The composition of the sample was determined from XPS data using the CasaXPS software. It allows establishing the N/Ti and N/Ba ratios of 3.8% and 2.9%, respectively, which correspond to a N/O ratio of ca. 1% which is a rather remarkably high value for a perovskite lattice built without charge compensating cations. The Ti-2p3/2 line shows a narrow single feature located at 457.8 eV binding energy for the undoped sample which is slightly shifted to 457.6 eV for the N-doped one (Fig. 3a). A similar shift of about ∼0.2 eV was reported by Wang et al.38 in a N doped SrTiO3 sample. Since the electronegativity of N is smaller than that of O, after the incorporation of nitrogen the electron density increases on Ti. This mechanism may explain the energy shift. Importantly, the Ti-2p line cannot be decomposed into several components for the doped sample indicating that Ti atoms adopt a well defined oxidation state, as expected for a homogeneous material.
Fig. 3 Photoemission spectra of undoped (black) and N-doped (red) BaTiO3 layers for (a) Ti-2p, (b) N-1s core levels, (c) the valence band region, (d) Ba-3d, (e) Ba 3d5/2 (undoped), the green contribution corresponds to the α component and the blue one to the β component, and (f) Ba 3d5/2 (doped). For (e and f) symbols stand for experimental data. For (b, e and f) thin bottom lines correspond to Shirley type backgrounds and thick straight lines to best fits. The best-fit parameters are reported in Table 2. |
The valence band (VB) region measured shows also modifications upon doping (Fig. 3d). The valence band of the N-doped sample is shifted by 0.2 eV towards lower binding energies, as was predicted by Zou et al. in N doped SrTiO3.39 The resulting shift stresses the presence of vacancies in the film.40 The shape of the valence band of BTO has been studied in detail in previous reports and consists of 3 well defined contributions (labelled A, B, and C in Fig. 3c). It was shown that it is composed of a pure O-2p π contribution for the low energy part and O-2p σ hybridized with Ti-3d levels for the high-energy contributions. This fine structure is modified for the doped sample. These modifications of the valence band shape can be related to changes in the crystallographic structure and in hybridization between Ti and O orbitals.
For the undoped film, the decomposition in individual lines of the Ba-3d5/2 peak reveals the presence of two components. They have been associated with two different chemical states already in early studies41 of BaTiO3 surfaces and are usually labeled α and β (Fig. 3e and f). The best fit parameters of the decomposition in individual lines are reported in Table 2. Already in the pioneering work of Mukhopadhyay et al.,41 the α component was attributed to the bulk perovskite phase and the β component to a more surface like environment. More recent studies7 demonstrated that the surface layer was likely made of Ba oxides that can be removed by ethanol etching. This interpretation was finally refined recently in two studies42,43 concluding that the β component is likely associated more precisely with a surface Ba peroxide (BaO2) layer. For the N-doped BaTiO3 film, the Ba-3d5/2 peak shows a broad single component at an intermediate position between α and β components. The chemical environment of Ba is thus strongly modified by the presence of N in the lattice. Another difference induced by N doping can be seen in the overview XPS spectrum (refer to Fig. S4, ESI†). One observes that N doping completely prevents the segregation of Sr in the film. Residual Sr is often observed in thin films grown with atomic oxygen plasma due to easy substitution between Ba and Sr in the perovskite lattice.
Ba 3d3/2 | Ba 3d5/2 | ||||||
---|---|---|---|---|---|---|---|
Peak | EB (eV) | Δ (eV) | ρ (%) | EB (eV) | Δ (eV) | ρ (%) | |
BTO | |||||||
α | 793.6 | 1.39 | 28.5 | 778.3 | 1.34 | 40.0 | |
β | 795.1 | 1.52 | 12.1 | 779.7 | 1.68 | 19.3 | |
N:BTO | |||||||
α + β | 794.5 | 2.23 | 39.78 | 779.2 | 2.25 | 59.2 |
Oxynitride films show promise to be used as photoanodes in the framework of solar water splitting. The photocurrent measurements on BTO and N:BTO samples are shown in Fig. 4a and the PEC response is completely different from the response of a bare Nb:SrTiO3 substrate (refer to Fig. S5, ESI†). The change in magnitude and shape of the photoresponse of the films with respect to the bare substrate demonstrates that the measurements performed on films are not mingled with the signal coming from the substrate. We observe a slight improvement of the PEC properties upon N-doping, for example, at 0 V vs. Ag/AgCl, the photocurrent density (Jph) increases from 17 μA cm−2 for the undoped sample up to 19 μA cm−2 for the doped one. This difference increases with voltage and at 0.7 V vs. Ag/AgCl, the photocurrent generated in the doped sample is 63% larger than for the undoped one. This observation is consistent with the results of Xing et al.40 who reported an improvement of the PEC properties with N doping of SrTiO3 prepared by the hydrothermal method. These authors concluded that nitrogen doping not only modulates the visible light absorption feature, but also has consequences on the enhancement of charge separation efficiency, which can promote the photocatalytic activity. Although, according to their results, it was hard to give a solid conclusion about which parameter among the doping level, the crystallinity or nano-structuring was the major factor contributing to the improvements in the PEC properties.
To get insight into the spectral response of our layers we have performed photocurrent measurements as a function of the incident light wavelength. The photocurrent density data normalized to the corresponding incident light flux are reported in Fig. 4b. The Full Width at Half Maximum (FWHM) of spectral absorption is 51 nm and 54 nm for BTO and N:BTO respectively. The window of “efficient absorption” is much larger for the N-doped sample and its maximum is slightly shifted towards the Ultra-Violet (UV) light range within a nearly symmetric shape, as compared to the other situations. We estimated (Fig. 4c) the photoelectrochemical band gaps of our samples through the “efficient Tauc plot” method,44 by plotting (αhν)2vs. hν (hν being the photon energy and α the absorption coefficient of the material). The photoelectrochemical band gaps determined in this way are 3.62 eV and 3.61 eV for undoped and N-doped samples respectively. These values are very close to the band gap value from the literature for BaTiO3 (3.7 eV). When doping an n-type material, the band gap can increase or decrease. With a Fermi level near the conduction band edge, the charge carrier concentration of n-type semiconductors will increase when doped with electron donor atoms. If the Fermi level moves into the conduction band (Burstein Moss shift), the apparent band gap will increase as has been reported for various materials including non-oxide films,45 oxide nanostructured films,46 non-oxide nanosheets47 and oxide films.48 However, if electronic states are created just above the valence band, the apparent bandgap will decrease. The slight reduction of the band gap and the increase in the efficient absorption window observed in the present study are consistent with the results reported by Xing et al.40 on N doped SrTiO3. They claimed that oxygen vacancies positively shift the conduction band minimum while, to the contrary, N-doping tends to shift negatively the valence band maximum, leading thus to a reduction of the band gap value.
Footnote |
† Electronic supplementary information (ESI) available. See DOI: 10.1039/d1ma01082d |
This journal is © The Royal Society of Chemistry 2022 |