Open Access Article
Rita
Tóth
*a,
Roché M.
Walliser
b,
István
Lagzi
c,
Florent
Boudoire
ab,
Marcel
Düggelin
b,
Artur
Braun
a,
Catherine E.
Housecroft
b and
Edwin C.
Constable
b
aLaboratory for High Performance Ceramics, Empa, Swiss Federal Laboratories for Materials Science and Technology, 8600, Überlandstrasse 129, Dübendorf, Switzerland. E-mail: Rita.Toth@empa.ch; ritatoth1113@gmail.com
bDepartment of Chemistry, University of Basel, Spitalstrasse 51, 4056 Basel, Switzerland
cDepartment of Physics, Budapest University of Technology and Economics, 1111, Budafoki út 8, Budapest, Hungary
First published on 2nd September 2016
Periodic precipitation processes in gels can result in impressive micro- and nanostructured patterns known as periodic precipitation (or Liesegang bands). Under certain conditions, the silver nitrate–chromium(VI) system exhibits the coexistence of two kinds of Liesegang bands with different frequencies. We now present that the two kinds of bands form independently on different time scales and the pH-dependent chromate(VI)–dichromate(VI) equilibrium controls the formation of the precipitates. We determined the spatial distribution and constitution of the particles in the bands using focused ion beam-scanning electron microscopy (FIB-SEM) and scanning transmission X-ray spectromicroscopy (STXM) measurements. This provided the necessary empirical input data to formulate a model for the pattern formation; a model that quantitatively reproduces the experimental observations. Understanding the pattern-forming process at the molecular level enables us to tailor the size and the shape of the bands, which, in turn, can lead to new functional architectures for a range of applications.
We selected the AgNO3/K2Cr2O7/gelatin system because this is the oldest traditional Liesegang system. In addition, silver dichromate finds some application as an oxidation catalyst15 and we envisaged the potential for the self-assembly of electrocatalytic microreactors.
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| Fig. 1 SEM micrograph of a typical dual-frequency precipitate pattern in the AgNO3/K2Cr2O7/gelatin system. | ||
The focus of this paper is to understand why and how the two kinds of precipitate bands form in the classical AgNO3–K2Cr2O7 system. Since this is the prototypical Liesegang system, a deeper understanding of the dual-frequency pattern formation in this system will enable the design of these complex precipitate bands in other chemical systems.
To investigate the constitution of the bands, quantitative chemical information with a spatial resolution below 100 nm is required. Since the bands are composed of mesoscopic particles, XRD for phase analysis can be ruled out. We used scanning transmission X-ray spectromicroscopy (STXM), which provides detailed spectroscopic information at high spatial resolution. STXM can spatially map the electronic structure and the chemical state of the pattern by near-edge X-ray absorption fine structure (NEXAFS) spectroscopy.16–19
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| Fig. 2 Liesegang precipitation bands formed in a ∼500 nm thin gelatin film. In the middle: 3D laser scanning micrograph of the periodic bands and its surrounding area. Left side: STXM micrographs of the fine detail of bands (top: 125 nm pixels, bottom: 50 nm pixels). Right side: STXM micrographs of the fine detail of the area between two bands (top: 125 nm pixels, bottom: 50 nm pixels). The STXM micrographs were measured at 576.2 eV, corresponding to absorption by Cr. A–D shows the positions where STXM spectra were recorded (Fig. 3). | ||
Fig. 3 shows the average of 100 spectra (100 × 20 nm × 20 nm areas) at positions A, B, C and D of a dual-frequency pattern shown in Fig. 2, on a band of a pattern which contains only large bands (E), as well as the spectra of reference materials (gelatin, K2Cr2O7, K2CrO4, Cr2O3, Ag and AgNO3). The Cr L3,2 spectra present two sets of features in the L3 region (570–579 eV) and the L2 region (580–590 eV) (Fig. 3a). The strong similarity between spectra A, E and the reference Cr(VI) spectrum20 confirms that in the precipitation bands, chromium is present as Cr(VI). In spectra B and C, the L2 peak (∼584 eV) is shifted slightly to lower energy and resembles the Cr(III) reference spectrum20,21 indicating that the area between the large bands contains Cr(III). It is worth noting that the X-ray beam contains some spectral contamination from Cr(III), which is present in the synchrotron beamline optics. In addition, the gelatin could act as a reducing agent and generate some Cr(III). We conclude that the precipitate contains Cr(VI) but when very small amounts of precipitate are present, the signature of Cr(III) from the aforementioned source becomes spectrally prevalent.
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| Fig. 3 STXM spectra. (a) Cr L3,2 edges, (b) O K edge and (c) Ag M edge average spectra (blue curves) of 10 square areas of 20 nm × 20 nm on the fine structure of a large band (A), background between the fine structure in the band (B), on the fine structure between bands (C) and background where no precipitation occurred (D). Spectra E were taken on a band in a pattern which only contained the large bands. As references (red curves) for (a) we added Cr(III) and Cr(VI) spectra from ref. 20, for (b) we acquired K2Cr2O7, K2CrO4 and AgNO3 spectra and used Cr2O3 spectrum from ref. 21. For references for the silver edge spectra (c) we used AgNO3 in a gelatin film, our physical vapor deposited Ag film and a polycrystalline Ag sample.22 Structural properties of the chromate and dichromate anions were taken from ref. 23. | ||
This, however, does not yet reveal whether the bands contain chromate or dichromate ion. Both chromate and dichromate contain Cr(VI), but the bond lengths and angles about the Cr in the dichromate ion vary to a certain extent (Fig. 3). Fig. 3b shows the oxygen 1s spectra of the abovementioned regions. In spectra A, B and E, the two peaks suggest that the precipitate in the large bands contains dichromate. The peaks are narrower than in K2Cr2O7, possibly due to interaction with Ag+ ions. The peaks in spectra C and D are similar to the K2CrO4 reference spectrum, indicating that the high frequency thin bands between the large bands contain CrO42− ions. Smaller amounts of CrO42− ions are also found between these bands. Lastly, Fig. 3c shows the Ag M4,5 edge spectra; while the peaks corresponding to the M4,5 edges at 368 eV and 374 eV are clearly visible (arrows) on the Ag reference spectra,22 they are not observed in any of the precipitate spectra. The broad, flat peak in the range of the Ag M4,5 edges suggests that silver is present throughout the entire pattern, although a contribution from the nitrogen K edge peak at ∼405 eV is anticipated. Nitrogen is present in the gelatin, in the substrate (Si3N4 window) and in the outer electrolyte AgNO3.
As a conclusion of the NEXAFS results, the analysis of the Cr 2p multiplet spectra shows that the precipitates consist of Cr(VI). The O K pre-edge results reveal that the large bands contain Cr2O72− ions and the area between the large bands, including the high frequency thin bands, contains CrO42− ions. Since the Ag M edge spectra show that silver is present in the precipitate bands, we conclude that the precipitate in the large bands is Ag2Cr2O7 and in the small bands it is Ag2CrO4. It is noteworthy, that the Ag edge spectra also suggest the presence of Ag–N bonds in the high frequency bands causing the peak at 398 eV (see later discussion), while this peak is absent from the spectrum of the low frequency, large band when high frequency bands do not form (E).
:
chromium ratio of approximately 1
:
1.
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The higher the initial pH, the more the chromate–dichromate equilibrium is shifted towards the chromate side (see chemical equilibrium diagram in Fig. S2, ESI†). This is also apparent from the color change of the gelatin/K2Cr2O7/NH4OH solution; at higher pH the solution becomes yellow as opposed to the orange color of the solution without NH4OH. As a result, at higher pH fewer dichromate ions remain to form large bands. Therefore, with increasing pH, the number of the large bands decreases and consequently, the spacing coefficient increases. This is calculated from the spacing between consecutive bands using:
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| Fig. 7 The number of large bands decreases with increasing pH both in experiments (a) and model calculations (b). In (a) the red circles and the black rectangles correspond to gelatin films prepared with 500 rpm and 300 rpm spin coating speeds, respectively. The spacing of the bands increases with increasing pH both in experiments (c) and model calculations (d). We used the same parameter set in the numerical simulations as in Fig. 8. | ||
We also studied systems where the gelatin contained potassium chromate instead of potassium dichromate. The same pH dependence was observed with only a slight pH shift (blue and red curves in Fig. 6), due to the buffering effect of the gelatin. Without added gelatin and base we measured pH values of 4.22 and 8.66 for 0.01 M K2Cr2O7 and 0.01 M K2CrO4 solutions, respectively, but when 10% gelatin is added, the pH changes to 6.2 and 6.6. It shows that the type of the initial chromium(VI) species ions (chromate or dichromate) has only an insignificant effect on the pattern formation.
The STXM Ag M edge spectra showed an Ag–N bond signature peak at 398 eV in the high frequency bands, but this peak was absent from the spectrum of the low frequency, large band (Fig. 3c, curve E). At higher ammonia concentrations, diammine silver(I),27 (aqueous [Ag(NH3)2][NO3]), can form from AgNO3 and NH4OH. If [Ag(NH3)2]+ plays a crucial role in band formation, bands should not form when KOH is used instead of ammonia. As both kinds of bands formed in the system containing KOH, [Ag(NH3)2]+ formation does not have a role in band formation. The Ag–N bond signature may also originate from the amino groups in gelatin which coordinate Ag+ in an alkaline milieu.
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| δta = DΔa − k1ab1 − k2ab2 | (7) |
| δtb1 = DΔb1 − k1ab1 − κ1b1 + κ2b2 | (8) |
| δtb2 = DΔb2 − k2ab2 + κ1b1 − κ2b2 | (9) |
| δtm1 = −λ1Δ(ε1m1 − γm13 + σΔm1) + k1ab1 | (10) |
| δtm2 = −λ2Δ(ε2m2 − γm23 + σΔm2) + k2ab2 | (11) |
= (ch + cl)/2 and λ, ε, γ and σ are parameters of the Cahn–Hilliard equation.30,31Eqn (7)–(11) were solved numerically using the “method of lines” technique on a uniform 1D grid with appropriate boundary (no-flux boundary conditions for all species except for A at the junction point of the electrolytes), where for species A a Neumann-type boundary condition was applied: (a|x=0(t) = a0) and initial conditions (a(t = 0, x) = 0, b1(t = 0, x) = b10, b2(t = 0, x) = b20, m1(t = 0, x) = m2(t = 0, x) = 0). The equations were integrated in time by the forward Euler method. The grid spacing and the time step were 1.0 and 0.04, respectively.
The results of the model are in very good agreement with our experimental findings. Fig. 8 shows experimental and calculated profiles at two different pH values. At pH = 5.7 large, low frequency bands form, while at pH = 10.1 very thin, densely packed bands can be observed. Here the chromate–dichromate equilibrium (1) is shifted towards CrO42−, a trend accurately reproduced by the model calculation. When κ1 >κ2 in eqn (4), the equilibrium is shifted towards Cr2O72− and strong, low density bands form. However, when the equilibrium is shifted towards CrO42−, K = κ1/κ2 decreases and the high frequency bands coexist with the large, low frequency bands. The number of the bands can also be controlled by the pH in the theoretical model similarly to the experiments. Fig. 7 illustrates how the number of bands decreases and consequently, the spacing between them increases with decreasing K = κ1/κ2 in agreement with the experimental findings.
SEM-FIB images and EDX analysis revealed that the precipitate particles contain a high silver ratio core. We propose that the white precipitate in the propagation front seen in the video contains silver nanoparticles which are formed from the invading outer electrolyte on a different time scale (faster), before the precipitation reaction between the inner and outer electrolyte occurs. We reported previously8 that in a system containing the same AgNO3 invading electrolyte, however, only NH4OH (no chromate) in the gelatin film, similar high frequency small bands form at pH > 7.2 and the bands are composed of Ag/Ag2O particles. Fig. S5 (ESI†) clearly demonstrates that the morphological parameters of this highly periodic pattern and the high frequency bands found in the classical system are almost identical. We used the same experimental conditions, the only difference between the two systems was the lack of potassium dichromate in one of the gelatin films. In the silver nitrate/ammonium hydroxide/gelatin system (Fig. S5 left, ESI†) we determined an average band height of 40–90 nm, a FWHH of 2.0 μm and a spacing of 3.15 μm (measured from the maximum of one peak to the maximum of the neighbouring peak). In the propagation front of the classical Liesegang system containing dichromate ions (Fig. S5 right, ESI†) we found an average band height of 40–80 nm, a FWHH of 2.1 μm and a spacing of 3.4 μm. SEM-FIB cross sections, made at approximately the same distance (350 μm) from the stamping core, revealed that the size of the particles forming the bands is the same in the two systems.
Remarkably, it was also found that the cores of the particles in the bands of the classical system (Fig. 10b and d) are almost identical in shape and size as the nanoparticles found in the silver nitrate/ammonium hydroxide/gelatin system (Fig. 10a and c). As the core structures were found in both the large and small bands formed in the classical dichromate Liesegang system, it is rational to assume that the silver containing nanoparticles formed in the reaction front serve as nucleation sites for the Ag2Cr2O7 and Ag2CrO4 precipitates at high pH. As the Ag2CrO4 precipitate is less soluble than Ag2Cr2O7 (eqn (2) and (3)), first this nucleates on the silver particles in the small bands, and later Ag2Cr2O7 builds upon them forming the large bands. For this reason, much larger particles are observed in close proximity to the peak of the large bands in the SEM-FIB cross-section micrographs. This also explains why the STXM measurements show mainly Ag2Cr2O7 precipitate in the large bands even when they are split into small bands and in contrast, the small bands between the large bands appear to contain Ag2CrO4 precipitate. The two precipitates can form consecutively and both of them can be present at the same time due to their different solubilities.
It has already been suggested by Holba32 and Ramaiah33 that secondary (small) precipitation band formation precedes the primary (large) band growth, but it was thought that the latter is a result of the coarsening and strengthening of the secondary bands. However, from our results it is clear that the chemical composition of the two types of precipitation bands is different; therefore they must form independently from each other. We assume that the white precipitate forming first at the reaction front creates the fundamental structure for the two kinds of bands, before silver chromate/dichromate grow around the silver containing core particles. Similar coexistence of larger and finer bands was observed by Karam et al.13 in the Pb(NO3)2/K2CrO4/agar system. However, this system follows a reverted spacing law, i.e. the spacing between large bands decreases with the distance from the contact area of the two electrolytes, as opposed to the classical Ag2Cr2O7 system we used, where the spacing increases as we get further from the contact area. This difference implies a different formation mechanism which is, according to the authors, related to the light sensitivity of the PbCrO4 precipitate.
With the gained knowledge from our investigations of the “classical” Liesegang system, we are now able to understand the formation of the bands. This helps us to control the formation as well as the size and the shape of the bands. Now we can tailor the system for potential low cost structures adapted to a wide range of applications e.g. production of nanowires/bands, surface enhancement of catalytically active materials, as well as diffraction gratings.
SEM (scanning electron microscopy), SEM-FIB (scanning electron microscopy-focused ion beam) and EDX (energy-dispersive X-ray spectroscopy) measurements were performed on a FEI Helios Nano Lab 650 at ZMB (Zentrum Mikroskopie der Universität Basel, Basel Switzerland) on the same samples, which have been analyzed before by STXM. The STXM sample holder was mounted onto a SEM sample holder. The whole setup was then sputter-coated with a 30 nm platinum layer to increase conductivity.
STXM (scanning transmission X-ray spectro-microscopy) measurements were performed on the PolLux beamline of the Swiss Light Source, Paul Scherrer Institute (Villigen, Switzerland).17–19 The images and spectra were acquired at photon energies covering the chromium L-edge (565 eV to 800 eV), the oxygen K-edge (500 eV to 600 eV) and the silver M-edge (340 eV to 420 eV). The silver energy range also contains the nitrogen K edge (395 eV to 403 eV), which presents some interference due to the nitrogen present in the gelatin and the silicon nitride membranes supporting the samples and the Fresnel zone-plate focusing optic of the STXM instrument. We also recorded spectra of several reference materials, such as K2Cr2O7, K2CrO4, Ag and AgNO3. An empty hole of the sample holder and a pure gelatin film were also scanned as a background for the sample and reference materials measurements. Background subtraction, normalizations and absorbance calculations for the STXM data were performed using custom Matlab procedures.
Footnote |
| † Electronic supplementary information (ESI) available: EDX spectra, video monitoring setup, comparison of AgNO3/NH4OH/gelatin and the classical AgNO3/K2Cr2O7/NH4OH/gelatin Liesegang systems, chemical equilibrium diagram for chromate–dichromate equilibrium. See DOI: 10.1039/c6sm01564f |
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