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Design of a Metal-Oxide Solid Solution for Sub-ppm H2 Detection
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Design of a Metal-Oxide Solid Solution for Sub-ppm H2 Detection
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  • Elena Spagnoli*
    Elena Spagnoli
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
    *Email: [email protected]
  • Andrea Gaiardo*
    Andrea Gaiardo
    MNF-Micro Nano Facility Sensors and Devices Center, Bruno Kessler Foundation, via Sommarive 18, Trento 38123, Italy
    *Email: [email protected]
  • Barbara Fabbri
    Barbara Fabbri
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
  • Matteo Valt
    Matteo Valt
    MNF-Micro Nano Facility Sensors and Devices Center, Bruno Kessler Foundation, via Sommarive 18, Trento 38123, Italy
    More by Matteo Valt
  • Soufiane Krik
    Soufiane Krik
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
    Sensing Technologies Lab, Faculty of Science and Technology, Free University of Bozen-Bolzano, piazza Università 1, Bolzano 39100, Italy
  • Matteo Ardit
    Matteo Ardit
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
    More by Matteo Ardit
  • Giuseppe Cruciani
    Giuseppe Cruciani
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
  • Michele Della Ciana
    Michele Della Ciana
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
    National Research Council, Institute for Microelectronics and Microsystems, via Gobetti 101, Bologna 40129, Italy
  • Lia Vanzetti
    Lia Vanzetti
    MNF-Micro Nano Facility Sensors and Devices Center, Bruno Kessler Foundation, via Sommarive 18, Trento 38123, Italy
    More by Lia Vanzetti
  • Gabriele Vola
    Gabriele Vola
    Cimprogetti S.r.l. Lime Technologies, via Pasubio, Bergamo 24044, Italy
  • Sandro Gherardi
    Sandro Gherardi
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
  • Pierluigi Bellutti
    Pierluigi Bellutti
    MNF-Micro Nano Facility Sensors and Devices Center, Bruno Kessler Foundation, via Sommarive 18, Trento 38123, Italy
  • Cesare Malagù
    Cesare Malagù
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
  • Vincenzo Guidi
    Vincenzo Guidi
    Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
Open PDFSupporting Information (1)

ACS Sensors

Cite this: ACS Sens. 2022, 7, 2, 573–583
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https://doi.org/10.1021/acssensors.1c02481
Published February 16, 2022

Copyright © 2022 The Authors. Published by American Chemical Society. This publication is licensed under

CC-BY 4.0 .

Abstract

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Hydrogen is largely adopted in industrial processes and is one of the leading options for storing renewable energy. Due to its high explosivity, detection of H2 has become essential for safety in industries, storage, and transportation. This work aims to design a sensing film for high-sensitivity H2 detection. Chemoresistive gas sensors have extensively been studied for H2 monitoring due to their good sensitivity and low cost. However, further research and development are still needed for a reliable H2 detection at sub-ppm concentrations. Metal-oxide solid solutions represent a valuable approach for tuning the sensing properties by modifying their composition, morphology, and structure. The work started from a solid solution of Sn and Ti oxides, which is known to exhibit high sensitivity toward H2. Such a solid solution was empowered by the addition of Nb, which─according to earlier studies on titania films─was expected to inhibit grain growth at high temperatures, to reduce the film resistance and to impact the sensor selectivity and sensitivity. Powders were synthesized through the sol–gel technique by keeping the Sn–Ti ratio constant at the optimal value for H2 detection with different Nb concentrations (1.5–5 atom %). Such solid solutions were thermally treated at 650 and 850 °C. The sensor based on the solid solution calcined at 650 °C and with the lowest content of Nb exhibited an extremely high sensitivity toward H2, paving the way for H2 ppb detection. For comparison, the response to 50 ppm of H2 was increased 6 times vs SnO2 and twice that of (Sn,Ti)xO2.

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Copyright © 2022 The Authors. Published by American Chemical Society
The current scenario of industrial development combined with a dramatic population growth results in a high demand for energy. Thereby, scientific and technological activities have been focused on the development of sustainable energy sources, aimed at reducing the carbon footprint of energy production processes. (1) Within this framework, hydrogen-based energy generation has become a globally accepted practice to obtain clean energy. (2) Moreover, hydrogen (H2) is largely employed in various industrial processes, such as methanol and ammonia production and petroleum refinery. In 2019, the global market of hydrogen generation was valued at USD 117.49 billion, and it is expected to grow steadily in the future. (3) However, the production, storage, and transportation of H2 are very risky because of its high energy density and explosivity even at concentrations as low as 4%, (2) and therefore, H2 monitoring is a relevant challenge.
Several technologies have been developed to monitor H2 concentration. Analytical techniques, such as quadrupole mass spectrometry, gas chromatography, mid-infrared spectroscopy, atomic absorption spectrometry, and proton-transfer reaction mass spectrometry, can reliably detect H2 even in traces. (4−8) However, instruments large size and weight, time-consuming process, high cost, lack of portability, need for continuous maintenance, and calibration, along with the requirement of trained personnel, (2) have negatively impacted the widespread use of such analytical tools in many applications.
The advent of solid-state gas sensors, such as chemoresistive gas sensors, has partially overcome these issues, and several types of small and low-cost gas sensors have been investigated for H2 detection. (2)
About 90% of the metal oxides (MOXs) utilized as sensing films in chemoresistive devices belong to a restricted class of semiconductors, i.e., SnO2, ZnO, TiO2, WO3, In2O3, and CuO. (9) The paucity of reactive metal oxides may limit the sensing performance expressed by the 3S rule (selectivity, sensitivity, and stability). (10,11) A solid solution of two individually sensitive metal oxides would allow to vary with continuity the sensing properties of the solution, with the relative proportion of the metal as a free parameter to be optimized. The aim is to magnify the qualities of single oxides and to possibly mitigate their deficiencies. As a practical example, a solid solution of Sn and Ti oxides combines high sensitivity toward reducing gases typical of SnO2 (12−17) and the peculiar low influence by humidity on the sensing properties of TiO2. (12,16)
Addition of a metal to a sensing metal oxide or to a sensing solid solution may also be beneficial. (18−21) Ferroni and Guidi et al. first investigated the effect of Nb5+ incorporation within a TiO2 lattice, proving that it can inhibit grain growth and anatase-to-rutile transition. (22,23) Moreover, Nb doping increased the bulk conductivity of titania. (24) Carotta et al. demonstrated the influence of Nb on the solid solution of Sn and Ti for a single level of concentration of Nb. (25)
The aim of this article is to study H2 sensing by varying Nb concentration in a solid solution of Sn and Ti oxides. Such a material was obtained through the sol–gel technique using different Nb concentrations (1.5 to 5 atom %), while the Sn–Ti ratio was kept constant to 70:30 mol/mol, i.e., the best Sn–Ti proportion for H2 detection. (25) Such solid solutions were thermally treated at 650 and 850 °C. The sensor based on the solid solution calcined at 650 °C and with the lowest content of Nb exhibited an extremely high sensitivity toward H2 and significant selectivity. The films exhibited relevant responses even down to 0.4 ppm with an extraordinary potential to sense through almost the whole ppb range. The effect of possible interferents for applications, e.g., carbon monoxide, methane, nitrogen dioxide, ethanol, and acetaldehyde, resulted in a marginal influence on the response.

Experimental Section

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Synthesis of SnO2, (Sn,Ti)xO2, and (Sn,Ti,Nb)xO2 Powders

All of the chemicals, with reagent-grade purity and without any further purification, were from Sigma-Aldrich. Double-distilled water, passed through a Millipore Elix water purification system, was used.
SnO2 and (Sn,Ti)xO2 powders were prepared according to the procedures previously described. (16,26) Both powders were calcined at 650 °C for 2 h under air in a muffle oven.
Different samples of (Sn,Ti,Nb)xO2 were prepared by maintaining a Sn–Ti molar ratio of 70:30 and modifying the content of Nb to 1.5 and 5 atom %. In a typical synthesis procedure, required stoichiometric proportions of Sn(II)ethylhexanoate, Ti(IV)butoxide, and NbCl5 were dissolved in a hydroalcoholic solution. The total cation concentration was kept at [Mn+]tot = 0.1 M for each synthesis batch. The three-component (Sn,Ti,Nb) solution was obtained by dissolving Ti(IV)butoxide and NbCl5 separately in two different beakers each containing 35 mL of 2-propanol. The two transparent solutions were mixed in an ice bath, and Sn(II)ethylhexanoate was slowly added. Then, 1 mL of 0.1 M HNO3 solution was added dropwise to hydrolyze the metal–organic molecules, and 30 mL of mQ water was added to achieve a pale yellow colloid. The entire process was carried out by maintaining the solution under gentle stirring. The colloidal solution was kept in the ice bath for 3 h and left to rest overnight. The colloid was separated from the solution by vacuum filtration and washed several times with 2-propanol and water. The resultant xerogel was dried in air at 110 °C for 4h and calcined at either 650 or 850 °C for 2 h under air in a muffle oven.
As summarized in Table 1, SnO2, (Sn,Ti)xO2, and (Sn,Ti,Nb)xO2 powders were labeled according to the molar ratio between Sn, Ti, and Nb used for the synthesis and the calcination temperature.
Table 1. SnO2, (Sn,Ti)xO2, and (Sn,Ti,Nb)xO2 Sample Label According to the Molar Ratio between Sn, Ti, and Nb Used for the Synthesis and the Calcination Temperature
Sn/Ti/Nb molar ratiocalcination temperature (°C)label
100650SnO2 650
70:30:0650ST30 650
66.5:28.5:5650STN 5 650
66.5:28.5:5850STN 5 850
69.0:29.5:1.5650STN 1.5 650
69.0:29.5:1.5850STN 1.5 850

Material Characterization

The chemical composition and the morphology of the synthesized powders were investigated by energy-dispersive X-ray spectroscopy (EDX) and scanning electron microscopy (SEM), using a Zeiss EVO 40 microscope. Gas porosity and specific surface area of the powders were explored using a Micromeritics TriStar II Plus automated gas sorptometer. X-ray powder diffraction (XRPD) data were collected at room temperature on a Bruker D8 Advance Da Vinci diffractometer. X-ray photoelectron spectroscopy (XPS) analyses were performed using a Kratos AXIS Ultra DLD. XPS quantification was performed using the instrument sensitivity factors and high-resolution scans.
All specifications about instruments, equipment, data collection, and evaluation are reported in the Supporting Information.

Gas Sensor Preparation and Characterization

The powders were ground in an agate mortar and mixed with organic vehicles to form homogeneous pastes. Then, the pastes were screen-printed onto alumina substrates, equipped with interdigitated gold electrodes on the top side and a heater on the back side. (27,28) The deposition thickness for each device was about 20–30 μm, with an area of 1.22 × 1.60 mm2. (27) The devices were calcined at 650 °C for 2 h and finally packaged with a standard TO-39 support using thermocompression bonding and a gold wire. (27,29)
The sensing properties of STN sensors were investigated using a dedicated apparatus, including a customized sealed gas test chamber and a data acquisition system. (30) All specifications about the system for gas injection, chamber characteristics, and electronics are given in the Supporting Information.
The sensor response was defined as
(1)
(2)
where Gair and Ggas are the steady-state conductance values in air and gas, respectively.
The gas sensing characterization was carried out under both dry (20% of O2 and 80% of N2) and wet conditions.
Sensor signal baselines were stabilized at the beginning of each measurement by keeping the sensors at their working temperature under a continuous flow (500 sccm) of either synthetic dry or wet air, in the range of 1.7–55% relative humidity (RH %).
The response and recovery times were calculated as the time needed to reach 90% of the response value and the time required to switch back to 90% of the baseline value, respectively.
To estimate the best working temperature, the responses to 50 ppm of H2 in dry air were compared by heating the film to four different temperatures (350, 400, 450, and 500 °C). The sensitivity was examined by exposing the sensors to increasing H2 concentrations. The repeatability of the dynamic responses vs 0.4 and 100 ppm of H2, i.e., the extreme concentrations of the calibration curves, was studied for the sensors with better sensitivity.
To investigate the sensor selectivity vs H2, the films were exposed to water vapor and several possible interfering gases such as carbon monoxide (CO), methane (CH4), acetaldehyde (C2H4O), ethanol (C2H5OH), and nitrogen dioxide (NO2). For the sake of comparison, all of the concentrations were set at the same level as that of H2, i.e., 10 ppm. The only exception was NO2, which was set at 1 ppm, which is its low TLV (threshold limit value) for short-term exposure based on European directives. (31)
The investigation of selectivity through CO and CH4 is mandatory because they are both involved in steam reforming of methane (SRM), i.e., the predominant industrial process for manufacturing hydrogen and syngas. Here, steam endothermically reacts with methane to produce H2 and CO. (32,33) Moreover, the films were probed vs an aldehyde (C2H4O), an alcohol (C2H5OH), and an oxidizing gas (NO2), which are thought as representative of chemical compounds with different functional groups.
The Arrhenius plots and energy barrier measurements in air and vs 25 ppm H2 were carried out for all of the films. (34)

Results

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Morphological, Structural, and Chemical Characterization

Powder morphologies were observed by SEM, as shown in Figure S1. All of the samples were composed of spheroidal nanograins. Figure 1 shows the particle-size distribution of the powders with Nb contents of 1.5 and 5 atom % and at calcination temperatures of 650 and 850 °C. Particle sizes of STN 1.5 650 ranged within 10–15 nm, while a wider distribution ranging within 25–60 nm was recorded for STN 5 650. The relative proportion of Sn, Ti, and Nb played a fundamental role in particle growth in solution since a higher concentration of Nb5+ led to a wider dispersion of the particle-size distribution. At the same time, the addition of a higher concentration of Nb5+ prevented grain coalescence at high temperatures. (23) Indeed, for the sample STN 5 850, the distribution of the particle diameters remained almost unchanged compared to STN 5 650. On the contrary, the average particle size increased from 15.8 nm at 650 °C to about 27.8 nm at an 850 °C firing temperature for the STN 1.5 samples.

Figure 1

Figure 1. Distribution of particle diameters (nm) in STN samples, revealing the influence of annealing temperature on grain coalescence. Black dotted lines indicate the mean value of the distributions.

To further investigate the influence of temperature on sample morphology, the adsorption and desorption isotherms of representative samples were carried out (Figure S2).
The corresponding N2-Brunauer–Emmett–Teller (BET) surface area and the average pore size diameters are reported in Table 2. The BET specific surface area of the powders treated at 650 °C was similar. The treatment at 850 °C of the powder with 1.5 atom % of Nb halved its BET specific surface area compared to its counterpart when heated at 650 °C. From the calculated pore size, it can be inferred that the sample exhibited mesoporosity. (35) The samples heated at 650 °C showed an average pore diameter remarkably lower than that of STN 1.5 850.
Table 2. BET Specific Surface Areas and Pore Size Distributions of Representative Solid Solution Powders, Highlighting Dissimilarity Especially between Samples with Different Heat Treatments
samplespecific surface area by BET method (m2/g)pore size: D-H desorption average pore diameter (4V/A) (nm)
ST30 65050.4212.66
STN 1.5 65043.7216.71
STN 5 65048.3612.52
STN 1.5 85022.6323.95
XRPD patterns collected at room temperature in the 2θ angular range of 22–57° are shown in Figure 2. Peak positions for ST30 650 were shifted toward higher 2θ angles compared to those for STN samples as a result of smaller lattice parameters. In all of the investigated samples, the main phase (ranging from 96.9 to 99.0 wt %, see Table S1) was a tetragonal rutile-type phase (space group, s.g. P42/mnm). A variable amount of tetragonal anatase-type phase (s.g. I41/amd) was detected as the remaining fraction. The main rutile-type phase (starting structural model from Hirata) (36) along with the associated anatase-type phase (starting structure model from Howard et al.) (37) was modeled by carrying out a multiphase refinement in which only the scale factors and unit-cell parameters were varied. As an example of the approach used for the XRPD pattern analysis, the Rietveld refinement plot for the sample STN 1.5 650 in the 2θ range of 10–90° is shown in Figure S3.

Figure 2

Figure 2. X-ray powder diffraction patterns collected at RT. Gray lines parallel to the y axis mark peak positions for ST30 650 to highlight the shift for STN peaks. The fractions of rutile-type (s.g. P42/mnm) and anatase-type (s.g. I41/amd) phases were ∼98 and 2 wt %, respectively.

Useful information on the synthesized solid solution can be achieved by plotting the lattice parameter ratio (a/c) of the rutile-type phase versus its volume (V) (Figure S4). By contrasting the lattice parameters of the investigated samples to those of pure TiO2 and SnO2 from the literature, it emerged that the rutile-type phase was a solid solution where the smaller [6]Ti4+ (ionic radius, i.r. = 0.605 Å) and [6]Nb5+ (i.r. = 0.64 Å) replace about 17% of the larger [6]Sn4+ (i.r. = 0.69 Å) at the octahedral site (ionic radii from Shannon). (38) Nb incorporation in the solid solution of Sn and Ti resulted in a bigger cell volume (Table S1), especially for samples STN 5 650 and 850. On the other hand, the unit-cell volume of the anatase-type phase was close to that of other TiO2 nano-anatase from the literature.
EDX and XPS characterizations allowed us to estimate the composition of the films in the bulk and at the surface (see Table 3). The Sn/Ti/Nb atomic proportion obtained through EDX was about 72:23:5 and 74:24.4:1.6 for STN 5 and STN 1.5, respectively. The obtained atomic proportion was slightly different from the synthesis starting stoichiometry, and a relative deficiency of Ti was observed. XRPD phase analysis revealed the presence of a small amount of nano-anatase phase mainly composed of TiO2. Such small nanoparticles can be partly lost during the supernatant filtration and powder washing, explaining the relative deficiency of Ti in the final samples compared to that in the batch of synthesis. The proportion of Sn, Ti, and Nb obtained through the XPS analysis revealed higher contents of Ti and Nb than those detected by the EDX analysis (Table 3), an evidence that Ti and Nb partially segregated on the surface of the STN nanoparticles. The same behavior has been already observed in the synthesis of other MOX solid solutions and perovskites, in which the driving force for a surface segregation was the lower surface energy of the component that segregated at the surface, as well as a difference in cation mobility under an applied gradient. (39,40)
Table 3. Compositional Proportion of Sn, Ti, and Nb in STN Samples, Obtained through EDX and XPS analyses, Highlighting the Slightly Different Composition of Bulk and Surface
EDXSTN 1.5 650STN 5 650STN 1.5 850STN 5 850
Ti22.022.726.721.2
Nb1.75.31.45.0
Sn76.372.071.973.8
XPSSTN 1.5 650STN 5 650STN 1.5 850STN 5 850
Ti29.330.229.425.2
Nb3.89.83.412.4
Sn66.960.067.262.4
The differences in Sn, Ti, and Nb composition between STN 1.5 and 5 evidenced by EDX and XPS analyses would impact the bulk and surface properties of the materials, influencing their behaviors as a gas sensor.
Figure S5 shows the high-resolution scans of Sn 3d, Ti 2p, and Nb 3d core levels. The high-resolution spectra of the Sn 3d and Nb 3d regions showed peaks located at binding energies Sn 3d3/2 = 594.9 eV, Sn 3d5/2 = 486.5 eV and Nb 3d3/2 = 207.1 eV, Nb 3d5/2 = 209.7 eV, ascribed to Sn4+ and Nb5+, respectively. (41,42) The peaks in the high-resolution spectrum of the Ti 2p region, mostly attributed to the Ti4+ oxidation state at binding energies Ti 2p1/2 = 464.5 eV and Ti 2p3/2 = 458.7 eV, (43) showed a shoulder due to a small content of Ti3+ (Ti 2p1/2 = 463.3 eV and Ti 2p3/2 = 457.0 eV). (43,44) Sn 3d, Ti 2p, and Nb 3d core-level fits for STN 5 850 are displayed as an example in Figure S6.

Gas Sensing Properties

The optimal response of STN films was determined by measuring the conductance change before and after injection of 50 ppm of H2 at different working temperatures within 350–500 °C. Two different trends were observed (Figure S7). The influence of the working temperature on the response of STN sensors calcined at 650 °C was significant. Indeed, at 450 °C, the response peaked 2.5 times more than that recorded at 400 and 500 °C. On the other hand, the responses of the STN sensors calcined at 850 °C moderately increased with working temperature. Hereinafter, the working temperature was set at 450 °C for all STN sensors to compare their sensing properties under the same operating condition.
The sensitivity was investigated by exposing the sensors to 0.4, 1, 2, 10, 25, 50, and 100 ppm of H2 (Figure 3a). At each H2 concentration, the response of STN 650 films was higher than that of STN 850, with STN 1.5 650 overperforming among the others. Figure 3b exhibits the calibration curves for all of the sensors under study. Calibration curves were fitted with a power law function R=axb, R being the sensor response and x being the gas concentration. The inset in Figure 3b shows that STN 1.5 650 exhibited a significant response even at the lowest concentration of H2 injected in the chamber (R = 5.55 at 0.4 ppm). Thus, a very low theoretical limit of detection (LOD) is expected. A linear fit (R = cx) was adopted to better extrapolate the sensor responses at lower concentrations (see the inset in Figure 3b) and to determine the theoretical LOD, which was estimated as in ref (45). The estimated theoretical LOD was 5 ppb, i.e., the lowest LOD obtained so far for MOX gas sensors vs H2, to the best of our knowledge. Power law function parameters a and b and linear fit parameters c are listed in Table S2.

Figure 3

Figure 3. (a) STN film dynamical responses at 450 °C to 0.4, 1, 2 (inset) 10, 25, 50, and 100 ppm of H2 in dry air and (b) their calibration curves fitted with a power law function. A linear plot for concentrations lower than 2 ppm (inset) was used to estimate the theoretical LOD. (c) Response to four-cycle injection of 0.4 and 100 ppm of H2 as a function of time. (d) Comparison between the responses of STN, ST30 650, and SnO2 films to the same concentration of H2 (sensors performing at their optimal working temperature of 450 °C for STN and ST30 650 and 400 °C for SnO2 650). (25) The legend of graph (d) also applies to graphs (a), (b), and (c).

The repeatability of the dynamic response vs H2 was investigated for the sensors with better sensitivity, namely, STN 1.5 650 and STN 5 650. Figure 3c shows the dynamical responses to 0.4 and 100 ppm of H2, i.e., the concentrations extreme of the calibration curves, in four cycles.
The response and recovery times were calculated for 50 ppm (see Figure 3d), and their values are listed in Table S3. The response (about 2 min) and recovery (about 7 min) times were similar for all of the STN except for STN 1.5 650, which showed a slower response and faster recovery kinetics (about 5 min 10 s and 5 min 50 s, respectively). Response and recovery times within minutes have been already observed for traditional SnO2 and other materials in our previous works. (11,27,46−48) They were dependent on the size and geometry of the chamber and on the speed of the gas flow. (27) Since the filling time of the chamber was about 1 min 15 s, the response times of STN films should be rather fast.
The response of STN films vs H2 was compared to SnO2 650 and ST30 650 films in Figure 3d. Ti incorporation in the lattice triplicated the response of pure SnO2. The content of Nb in the solid solution and the calcination temperature showed a significant influence on the response. While the 1.5 atom % content of Nb doubled the response of ST30 650, 5 atom % did the opposite. Furthermore, a calcination temperature of 850 °C completely hindered the beneficial effects of both Ti and Nb, resulting in films with a response even lower than SnO2 650.
The effect of humidity was considered because water vapor can dissociate when interacting with the film, affecting its conductance. (46,49) To this aim, 50 ppm of H2 were injected in the gas chamber at different relative humidity percentages up to 55 RH % (see Figure 4). Water vapor did not significantly change the sensor baselines, but it affected the sensor conductance after injection of H2. Figure 4 highlights a significant decrease of the sensor signal up to 17 RH %. At higher humidity levels, the sensor signal to H2 kept rather constant, with STN 1.5 650 still sensing at a high level.

Figure 4

Figure 4. Influence of humidity on the conductance baseline and conductance after injection of 50 ppm of H2. The temperature inside the chamber was 29 °C in the whole range of RH %.

Film selectivity was explored by exposing the sensor to 10 ppm of CO, CH4, C2H4O, and C2H5OH and 1 ppm of NO2. The responses, defined as in eqs 1 and 2 and shown in Figure 5, highlighted that the STN 1.5 650 film was more reactive to hydrogen than to other gases, while the selectivity was lower for STN 5 650, STN 1.5 850, and STN 5 850.

Figure 5

Figure 5. Bar graph of STN film responses (see eqs 1 and 2) to 10 ppm of CO, H2, CH4, C2H4O, and C2H5OH and 1 ppm of NO2.

The response of STN 1.5 650 to H2 and that of other sensing films based on different metal-oxide semiconductors from the literature are reported in Table 4.
Table 4. Comparison of the Hydrogen-Sensing Performance of STN 1.5 650 and STN 5 650 films to Recently Achieved Frequently Used Metal-Oxide Sensors in the Literatureb (50−55)
materialconcentrationresponseoptimal operating temperature (°C)LODreference
STN 1.5 650100 ppm80a4500.4 ppm/5 ppbfthis work
STN 5 650100 ppm34a4500.4 ppm/13 ppbfthis work
SnO2100 ppm15c400  (50)
Pd/SnO2100 ppm28.5c1600.25 ppm (51)
Co/SnO2100 ppm23c330  (52)
WO3100 ppm4.82500.25 ppmf (53)
WO3–CuO100 ppm392500.31 ppmf (53)
CuO100 ppm1.7d2002 ppm (54)
ZnO100 ppm0.95e250  (55)
Ag/ZnO300 ppm4.79e2505 ppm (55)
a

Gas response ,

b

Gas response,

c

Gas response ,

d

Gas response ,

e

Gas response , where G is the conductance, R is the resistance, and V is the voltage.

f

Indicates theoretical LOD.

STN 1.5 650 performed better than several semiconductors, including highly accredited materials such as SnO2 and Pd-decorated and Co-doped SnO2, (50−52) WO3, (53) CuO, (54) WO3–CuO junction, (53) ZnO, and Ag-doped ZnO. (55) Moreover, its experimental LOD of 0.4 ppm was far lower than that reported in some recently accredited works. (52,53) As far as our knowledge is concerned, the best experimental result regarding H2 sensing was obtained by Wang et al., (51) recording a LOD of 0.25 ppm at Rair/Rgas = 3. However, the LOD for STN 1.5 650 was 0.4 ppm, but with a response of 5.6.
Based on this experimental result, we concluded that STN 1.5 650 highlights remarkable, still experimentally unexplored, potential for detecting very low concentrations of H2. To assess such limits, we used the method described by Huang and Wan. (45) The theoretical LOD turned out to be as low as 5 ppb, i.e., the lowest theoretical LOD obtained so far by metal-oxide gas sensors.

Discussion

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Since SnO2, TiO2, and Nb2O5 are three n-type semiconductors, STN is expected to be n-type as well. The conductance in nanostructured films is the result of bulk and surface properties. The bulk conductance in n-type semiconductors is given by free electrons thermally excited from donor levels near the conduction band. The electron transport in nanostructured films then involves slow percolation through a network of interconnected nanograins surrounded by the atmosphere. When a sensor is exposed to air, at the working temperature between 100 and 500 °C, atmospheric oxygen ionosorbs as molecular (O2–) and atomic (O, O2–) forms by capturing electrons at a surface state of the semiconductor. (56) According to the generally accepted conduction model, the presence of negative species on the surface of a metal oxide builds up a depletion layer, whose positive charge exactly compensates for the charge captured at the surface, leading to electroneutrality in the Schottky approximation. (57) Therefore, in nanostructured semiconductors, the mechanism of conduction is controlled by the number of free carriers and by the potential barrier built as a result of surface charge formation. Arrhenius plots and intergranular energy barrier measurements were conducted to investigate the effect of Nb addition on the conduction mechanism in the Sn- and Ti-oxide solid solution in dry air with and without H2. The Arrhenius plot in synthetic air was obtained by changing the temperature from 350 to 900 K at the heating rate of 6 K/min (Figure S8a), while intergranular energy barrier measurements (Figure S8b,c) were conducted as a function of temperature according to the method reported elsewhere. (34)
The conductance of all films increased with temperature because the number of free electrons, thermally excited from ionizable levels under the conduction band, increased. Moreover, STN films were more conductive than ST30 650 and a 5 atom % Nb content resulted in the highest conductance of the films annealed at 650 °C. The higher conductance of STN films can be explained through the substitution of Nb in the lattice, which resulted in extrinsic substitutional doping by introducing additional carriers. (22,24) This effect may be counteracted by the increase in the energy barrier ΔE, which would instead decrease the conductance of the solid solution. As an example, at 450 °C, ΔE = 0.9 eV for STN 1.5 650 and STN 5 650 compared to ΔE = 0.5 eV for ST30 650. Although it was not possible to quantify the role of ΔE on the film conductance, its change was a firm indication of bulk- and surface-defect modifications induced by the addition of Nb. The highest content of Nb and annealing temperature of 850 °C resulted in the lowest conductance for the STN 5 850 film. Indeed, in addition to providing the necessary mobility for Ti and Nb to enter the lattice of SnO2, annealing can also induce their segregation as the excess of stress in the lattice is not thermodynamically supported. (58,59) This process of self-purification would reduce the content of Nb5+, negatively impacting the conductance. The energy barriers of STN 1.5 850 and STN 5 850 laid below those of their counterparts annealed at 650 °C, i.e., ΔE = 0.7 eV at 450 °C, meaning that annealing changed bulk and surface properties too. Since n-type doping is commonly used to increase the low conductance of TiO2 films, the nature of defects that results from Nb addition and their correlation to electron transport in TiO2 has been the subject of many studies. (60,61) Despite the lack of studies on Sn, Ti, and Nb ternary solutions, it is known that the substitution of tetravalent cation (M4+) by pentavalent Nb5+, as a higher-valence cation, forms either M3+ or cation vacancies or both. (60,62) Trivalent titanium was distinguished in high-resolution scans of Ti 2p core levels. Based on these data, one may infer that the charge compensation of Nb5+ in the substitution of Ti4+ and Sn4+ was achieved by the creation of cation vacancies and trivalent cations and that, as for titania, these additional defects generated new donor states within the band gap, whose energy level depended on the properties of the defect. These defects may be generated in both bulk and surface, with the latter being active sites for redox reactions with the environment.
Under exposure to H2, adsorbed oxygen species oxidize the reactive gas generating water and free electrons as in eq 3, (63) causing conductance increase.
(3)
As discussed above, the response of STN films and their sensitivity and selectivity were evidently determined by the content of Nb and by the treatment temperature and that deserves a deeper discussion.
First, STN 650 films responded better than their STN 850 counterparts. This can be interpreted in terms of a larger surface area of the former compared to the latter as highlighted by BET measurements (see Table 2). Moreover, the intergrain energy barrier ΔE for STN 650 films decreased in the presence of H2 while it did not change for the STN 850 ones. It means that the effect of H2 on STN 650 conductance was the result of an increase of free charge carriers (see eq 3) and intergrain energy barrier decrease. Indeed, for STN 850, only free charge carriers increase occurred by reaction with H2.
Second, it was proved that STN 1.5 650 effectively improved the response of ST30 650 while STN 5 650 did the opposite. Both layers exhibited similar textural properties, thereby, unlike previous considerations, this feature cannot be called forward. However, XPS analyses highlighted that the films differ in surface relative composition of Sn, Ti, and Nb, i.e., 3.8 Nb % for STN 1.5 650 and 9.8 Nb % for STN 5 650. As discussed above, pentavalent Nb at the surface would either affect the reactivity of adsorbed oxygen bound to it or influence the receptive properties of the oxygen adsorbed to neighboring Ti and Sn atoms. Since Nb oxides do not possess qualified properties vs H2 detection, (64) evidently the presence of Nb strengthens the reactivity of neighboring sites. This would explain the improved sensing of STN 1.5 650. Probably, a superficial proportion as high as 10% in Nb at the surface would produce an excess of unreactive oxygen sites that would in turn clear up the beneficial role of Nb on its neighbors.
Third, STN 650 films were more selective to H2 than the STN 850 ones, namely, STN 1.5 650 was the most selective to this gas. The main differences between the STN 850 films and STN 650 ones were the specific surface area and the pore size. The specific surface area would only affect the magnitude of the response and not influence the selectivity. Indeed, the pore size may play a significant role as the main free path of the molecules is comparable to the length of the pores. (46,65) The pore size may affect the selectivity as is small enough to make the diffusion properties of the gases in the film dependent on their molecular diameter and mass. The pore size of the STN 650 samples is smaller than that of the STN 850 ones, e.g., 16.7 nm for STN 1.5 650 and 24.0 nm for STN 1.5 850. In this way, the STN 650 films would become more selective to H2 because H2 molecules diffuse deeper into the films than much larger molecules such as C2H4O and C2H5OH, thereby enabling a relatively wide surface for its sensing.

Conclusions

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This work investigated the effect of the addition of Nb to a solid solution of Sn and Ti oxides with regards to morphological, structural, and electrical properties and particularly to H2 sensing. Films with Nb 1.5 and 5 atom % contents were synthesized through the sol–gel technique by keeping the Sn–Ti ratio constant at the optimal value for sensing performance of the solid solution without Nb, i.e., Sn/Ti = 70:30. (25) The influence of calcination temperature was sought by heating the powders at 650 and 850 °C. SEM observations performed on the powders revealed morphologies consisting of spheroidal nanograins. Particle-size distributions of STN 5 650 and STN 5 850 were analogous, while STN 1.5 650 showed a more compact distribution and in a range of smaller sizes than STN 1.5 850. A high content of Nb prevented grain coalescence at high temperatures but made the growth of particles inhomogeneous during the synthesis. The annealing treatment strongly influenced the BET surface area of the powders, which was larger for the samples treated at 650 °C (STN 1.5 650 = 43.7 m2/g) compared to that of STN 1.5 850 (22.6 m2/g). XRPD analysis showed that Nb and Ti partly entered the bulk of rutile-type SnO2, forming a solid solution of (Sn,Ti,Nb)xO2. A small percentage of anatase-type structure (3 wt %), mainly ascribed to titania, was also detected. The remaining Nb and Ti segregated at the surface of the nanograins, as indicated by XPS. Segregation was more conspicuous for the highest content of niobium after annealing at 850 °C. According to high-resolution scans of Nb 3d core levels, Nb was located as substitutional in Ti and Sn sites, assuming a pentavalent nature. Moreover, the substitution of tetravalent cation by pentavalent Nb5+ may generate additional defects, which impact the surface reactivity.
The electric properties were significantly modified by the addition of Nb, inasmuch as it increased the conductance of all of the solid solutions by a factor of 3 to 10.
The sensing performance was probed by investigating sensitivity, repeatability, and selectivity. The content of Nb in the solid solution and the calcination temperature showed a significant influence on the response. While a 1.5 atom % content of Nb doubled the response to H2 of ST30 650, 5 atom % did the opposite. Furthermore, the calcination temperature at 850 °C completely hindered the beneficial effect of both Ti and Nb, resulting in films with a response even lower than SnO2 650. Despite STN 1.5 650 showed the highest response toward H2, the responses toward the other gases were comparable to that of the other films. This made it the most selective of the films tested. Moreover, at high humidity levels, only STN 1.5 650 was still sensing at a very high level.
In conclusion, the films made with the powders annealed at 650 °C with a 1.5 atom % content of Nb turned out to be the most interesting materials for H2 sensing. By comparing the performance to other metal-oxide films in the literature, it emerged that STN 1.5 650 exhibited an extremely high response, even at the lowest concentration of H2 (R = 5.6 toward 0.4 ppm). A very low theoretical limit of detection was estimated according to the method in ref (45). It resulted in extraordinary capability to sense as low a concentration as a LOD of 5 ppb.

Supporting Information

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The Supporting Information is available free of charge at https://pubs.acs.org/doi/10.1021/acssensors.1c02481.

  • In-depth description of material characterization methods and gas sensor preparation; morphological, textural, and structural characterizations; response variation according to the temperature change; fit parameters for calibration curves; response and recovery times; and film conductance vs temperature and energy barrier measurement (PDF)

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Author Information

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  • Corresponding Authors
  • Authors
    • Barbara Fabbri - Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, ItalyOrcidhttps://orcid.org/0000-0002-0188-2178
    • Matteo Valt - MNF-Micro Nano Facility Sensors and Devices Center, Bruno Kessler Foundation, via Sommarive 18, Trento 38123, ItalyOrcidhttps://orcid.org/0000-0003-2621-5555
    • Soufiane Krik - Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, ItalySensing Technologies Lab, Faculty of Science and Technology, Free University of Bozen-Bolzano, piazza Università 1, Bolzano 39100, ItalyOrcidhttps://orcid.org/0000-0002-3986-5066
    • Matteo Ardit - Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
    • Giuseppe Cruciani - Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
    • Michele Della Ciana - Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, ItalyNational Research Council, Institute for Microelectronics and Microsystems, via Gobetti 101, Bologna 40129, Italy
    • Lia Vanzetti - MNF-Micro Nano Facility Sensors and Devices Center, Bruno Kessler Foundation, via Sommarive 18, Trento 38123, Italy
    • Gabriele Vola - Cimprogetti S.r.l. Lime Technologies, via Pasubio, Bergamo 24044, Italy
    • Sandro Gherardi - Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
    • Pierluigi Bellutti - MNF-Micro Nano Facility Sensors and Devices Center, Bruno Kessler Foundation, via Sommarive 18, Trento 38123, Italy
    • Cesare Malagù - Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
    • Vincenzo Guidi - Department of Physics and Earth Sciences, University of Ferrara, via Giuseppe Saragat 1, Ferrara 44122, Italy
  • Author Contributions

    E.S. and A.G. contributed equally to this work. E.S. contributed to the conceptualization, methodology, validation, writing (original draft), electrical characterization and data curation. A.G. contributed to the conceptualization, methodology, validation, writing (original draft) and data curation. B.F., M.V., and S.K. contributed to the writing (review and editing) and electrical characterization. M.A. contributed to the investigation and material characterization, writing (review and editing) and methodology. G.C, M.D.C., L.V., G.V., and P.B. contributed to the investigation and material characterization. S.G. contributed to the electrical characterization. C.M. contributed to data curation and supervision. V.G. contributed to supervision, writing ( review and editing) and finding acquisition.

  • Notes
    The authors declare no competing financial interest.

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  • Abstract

    Figure 1

    Figure 1. Distribution of particle diameters (nm) in STN samples, revealing the influence of annealing temperature on grain coalescence. Black dotted lines indicate the mean value of the distributions.

    Figure 2

    Figure 2. X-ray powder diffraction patterns collected at RT. Gray lines parallel to the y axis mark peak positions for ST30 650 to highlight the shift for STN peaks. The fractions of rutile-type (s.g. P42/mnm) and anatase-type (s.g. I41/amd) phases were ∼98 and 2 wt %, respectively.

    Figure 3

    Figure 3. (a) STN film dynamical responses at 450 °C to 0.4, 1, 2 (inset) 10, 25, 50, and 100 ppm of H2 in dry air and (b) their calibration curves fitted with a power law function. A linear plot for concentrations lower than 2 ppm (inset) was used to estimate the theoretical LOD. (c) Response to four-cycle injection of 0.4 and 100 ppm of H2 as a function of time. (d) Comparison between the responses of STN, ST30 650, and SnO2 films to the same concentration of H2 (sensors performing at their optimal working temperature of 450 °C for STN and ST30 650 and 400 °C for SnO2 650). (25) The legend of graph (d) also applies to graphs (a), (b), and (c).

    Figure 4

    Figure 4. Influence of humidity on the conductance baseline and conductance after injection of 50 ppm of H2. The temperature inside the chamber was 29 °C in the whole range of RH %.

    Figure 5

    Figure 5. Bar graph of STN film responses (see eqs 1 and 2) to 10 ppm of CO, H2, CH4, C2H4O, and C2H5OH and 1 ppm of NO2.

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