3.1. XRD
The XRD analysis was conducted to find out how the coating process changes the structural properties of the synthesized cobalt ferrites. To compare bare nanomaterials and their coated counterparts, the results of XRD analysis from previous work is presented [
22].
Figure 2 shows 2 θ region from 34° to 38° of the normalized X diffractograms of the uncoated (bare) and starch-coated nanomaterials with (311) Bragg reflection. It can be clearly seen that the smaller nanoparticles US-CO, CO and MC-CO, with broader (311) reflections, underwent major changes during the starch coating process. Careful analysis of the diffractograms of coated nanoparticles provided quantitative data on the effect of the coating process itself on the starting nanomaterials.
The X-ray diffractograms of the starch-coated CoFe
2O
4 nanopowders are shown in
Figure 3, in the 2θ range from 15° to 90°. Starch-coated CoFe
2O
4 samples are labeled with an abbreviation indicating the synthesis method used (as for the bare samples), with the letter “s” for starch added in parentheses. All diffractograms were analyzed by Rietveld profile refinement using
FullProf Suite, Version: September 2020 OriginPro 2016.. The diffraction peaks were simulated with the
Pseudo-Voigt function. The same function is used to fit the strongest (311) Bragg peak with the aid of
OriginPro 2016,
Figure 3, left. The lattice constant
a311 is estimated using the well-known Laue–Bragg’s relation for cubic crystals:
The average nanoparticle size,
D311, is calculated by Debye–Scherrer relation:
where the instrumental FWHM (Si standard sample), w
i, for about 35.5°, is 0.07°.
With a higher starch content, a broad hump would be visible in the 10°–25° regions of the diffractograms [
25].
Figure 3 shows only well-crystallized CoFe
2O
4 with the space group
Fdm (No. 227).
Table 1 lists the structural parameters of the CoFe
2O
4 samples calculated from the diffractograms by Rietveld profile refinement and from the strongest peak (311). In the first row for each nanomaterial are values determined for bare CoFe
2O
4 samples [
22]. In the second row are the values for the starch-coated samples. The corresponding differences between coated and uncoated samples are given in brackets.
It is known that the refinement of the diffractogram according to Rietveld is not sufficiently sensitive for the inversion of cations whose atomic factors are of similar size. Therefore, XRD structure analysis was used to estimate more reliable values for cation inversion.
Figure 4 shows the results of the XRD structural analysis of the NP samples. The octahedral (
Roct) and tetrahedral (
Rtet) distances, as well as the cation inversion (
xstruct) are estimated via Equations (3)–(6), which relate the lattice parameters that were accurately ordered by the Rietveld profile analysis: Lattice constant (
aexp) and oxygen parameter (u) with known Shannon ionic radii [
26]. The effective radius of the Co
2+ cation with a high spin (
HS) electron arrangement in tetrahedral position is
r(Co
2+)
A = 0.58 Å, and in octahedral position the radius is
r(Co
2+)
B = 0.745 Å. For Fe
3+ in tetrahedral position the effective radius is
r(Fe
3+)
A = 0.485 Å (HS) and in octahedral position the radius is
r(Fe
3+)
B = 0.645 Å. The oxygen radius is
rO = 1.38 Å.
When the unit cell origin is B—vacancy (like in
FPSuite programme), ideal
= ¼ and the cation to anion distances are given by:
In
Figure 4a
Roct and
Rtet are presented as functions of
u, and in
Figure 4b the lattice constant is shown as a function of
xstruct. The migration of larger Co
2+ cations from B sites to A sites, i.e., the decrease in inversion, leads to an increase in the lattice constants (and all hopping distances, which depend only on
aexp). The obtained values of the cationic inversion,
xstruct, are listed in
Table 1.
The analysis of the XRD spectra,
Table 1, shows that the starch deposition process led to a decrease in the size of the magnetic CoFe
2O
4 nanoparticles of the US-CO(s) sample, a decrease in the cation inversion coefficient and an increase in the lattice constant. The reduction in the internal stress confirms the presence of a starch coating, which could lead to a reduction in the internal stress at least in the magnetic shell of the nanoparticles (and thus also to a reduction in the average stress).
US-CO(s) is the only sample that showed a significant decrease (Δxstruct < 0) in the inversion coefficient, so a noticeable increase in magnetization can be expected.
The lattice constant of the coated nanomaterial ME(s) remains the same as that of the pristine material. The cation inversion coefficient also remains unchanged (Δxstruct ≈ 0), but the size of the nanoparticles increases slightly due to the coating process. The increase in nanoparticles and even a minimal island-like coating lead to a decrease in the internal stress.
In the case of the starch-coated CO(s), the average size of the nanoparticles is significantly smaller and consequently the internal stress is higher. As a result of the increase in internal stress, a contraction of the crystal lattice (Δa < 0) occurred.
At first glance, it appears that the MW-HT(s) sample was not affected by the starch coating process. But a slight decrease in particle size and a slight decrease in internal stress confirm that starch coating has taken place.
MC-CO(s) has an increase in lattice constant, Δxstruct ≈ 0, a small increase in particle size, but a significant decrease in internal stress, indicating a very good starch coating.
3.2. Magnetic Properties
The results of magnetic measurements of starch-coated cobalt ferrite nanoparticles obtained by various synthesis methods are shown in
Figure 5. To make it easier to see the changes that occurred during the starch coating process, along with the magnetic hysteresis of the starch-coated nanomaterials, the hysteresis loops of the pure counterparts are also given. The same was applied to the results of FC/ZFC magnetization measurements. The left insets of the graphs for certain nanomaterials show the magnetizations of both the pure and coated counterparts together. All data were recorded during heating from 0 to 300 K in a weak magnetic field,
H = 100 Oe. Magnetization FC (
MFC) was measured after cooling in the presence of the same field. Magnetization ZFC (
MZFC) was measured after previous cooling in the absence of a field. The separation magnetizations of FC and ZFC as well as their curvatures indicate that the blocking temperatures
TB are below 300 K, see ref. [
22]. This means that in all ensembles of the investigated CoFe
2O
4 nanopowders a larger proportion of superparamagnetic particles is present at a measurement temperature of
M = f(H). Due to the presence of a large number of SP nanoparticles, at higher fields, beyond the hysteresis region, all samples have an asymptotic value of magnetization. For magnetic measurements at 300 K, CoFe
2O
4 nanoparticles smaller than 8 nm are in the superparamagnetic state in a time interval of about 100 s [
27]. In
Figure 5, the samples are arranged in order of increasing coercivity and decreasing FC magnetization values.
The measured (in
H = ±90 kOe) and calculated magnetic characteristics of starch-coated monodomain CoFe
2O
4 nanopowders obtained by different synthesis methods are given in
Table 2. The coercivity,
Hc, in the case of single-domain nanoparticles increases significantly with the size of the magnetic nanoparticles. It can be seen that as the coercivity increases, the “squareness” also increases, i.e., the magnetization curves become steeper. This is an expected trend and we have already seen it with these nanomaterials before their coating with starch [
22].
What changed strikingly after starch coating was the increased values of the slope of the magnetization curves of the smallest CO(s) and US-CO(s) nanoparticles in the
H = 0 region. (Corresponding slopes for bare nanoparticles were 13% lower for CO (46.7 emu g
−1/kOe) and 18% lover for US-CO (43.7 emu g
−1/kOe), as reported in Ref. [
22]). The increase in the rate of tracking changes in the magnetic field indicates a decrease in the interaction between the particles. The reason for this could be a decrease in the average size of the nanoparticles (which was confirmed by XRD). This increases the proportion of the surface layer (shell), which has a lower magnetic order. With a decrease in the average size, the proportion of superparamagnetic particles in the ensemble may also increase. Another possible reason for the lower interaction between the particles is their coating with starch. Depending on the amount of adsorbed starch and the type of coating (complete or partial shielding of the magnetic core), the effects can be different. In the case of MC-CO(s) nanomaterials, the starch coating led to a reduction in the influence of the magnetic field on the magnetic core of the nanoparticles. The decrease of the magnetization slope in the region close to the zero-field shows that the starch content in the MC-CO(s) nanopowders is significant. In general, starch coating leads to an increase in structural order in the magnetically depleted shell under the starch.
In the high field range,
H⟶90 kOe, the slopes of magnetization of US-CO(s) and MC-CO(s) have drastically decreased. For the bare US-CO nanoparticles the slope of magnetization was 0.037 (about 40% higher) and for MC-CO it was 0.035 emu g
−1/kOe (24% higher) [
22]. This clearly indicates a better structural order and a reduction in the number of canting spins due to the thickness coating. The magnetization slopes of larger nanoparticles did not show such correlated and significant changes.
A brief discussion of the results of magnetic measurements of pure cobalt ferrite nano materials [
22] and their starch-coated counterparts, in light of the outcomes of the XRD analysis, is presented in
Table 3 and
Figure 6.
Since the coercivity (
Hc) of single-domain CoFe
2O
4 nanoparticles is approximately proportional to the size of the magnetic particles [
22], it can be assumed that in cases where the particle size decreases during the starch deposition process (Δ
D < 0), a decrease in coercivity (Δ
Hc < 0) also occurs, and vice versa.
For well-coated NPs, a reduction in magnetization proportional to the amount of capping material is expected [
25]. For nanoparticles where TGA has confirmed a significant amount of starch, such as US-CO (s) and MC-CO (s), a decrease in magnetization is expected. However, for the US-CO (s) sample with Δ
xstruct < 0, the increase in magnetization was not reduced by the deposited starch. It is greater and corresponds to
x = 0.81. This means that the starch is not uniformly deposited (it is probably island-like) and magnetic core of nanoparticles is not completely encapsulated.
The magnetization of the MC-CO(s) sample was significantly reduced, by up to 18%. This indicates a uniform deposition of starch in a fairly thick layer.
In the case of ME(s) with a much lower amount of starch, the reason for the reduction of
Ms could be the capping of the primary aggregates (not individual nanoparticles). In this case, a lower amount of starch would be sufficient. Aggregates of larger nanoparticles with stronger magnetic moments may be more resistant to disintegration by stirring in a starch solution. In general, the primary aggregates are disassembled (partially or completely) and different aggregates of nanoparticles are formed. The different agglomeration of the NPs could be the reason for higher values of magnetization
Ms in CO(s) and MW-HT(s) [
27].
The results of magnetic measurements of CoFe
2O
4 nanomaterials before and after functionalization with starch are illustrated in
Figure 6 as a function of structural parameters determined by Rietveld and XRD structural analysis. The saturation magnetization,
Ms, is given as a function of the coefficient of cation inversion
xstruct (obtained from XRD structural analysis),
Figure 6a. The coercivity measured at 300 K and magnetization
MFC at 5 K (obtained from FC/ZFC measurements) are shown as a function of the size of the nanoparticles (estimated from the Williams–Hall plot) in
Figure 6b,c, respectively.
In
Figure 6a are shown saturation magnetizations of bare and starch-coated CoFe
2O
4 nanomaterials.
Ms of bare nanoparticles regularly decreases with increasing of cation inversion and the dashed line corresponds to the linear fit of
Ms =
f(
x) for bare nanomaterials (
μFe = 3.25
μB and
μCo = 2.5
μB) [
22]. Magnetization of small NP-s dominantly depends on the cation inversion, but at the same time,
Ms depends on the size of nanoparticles. As can be seen, larger ME nanoparticles with better structure, have higher
Ms than is expected for their coefficient of the cation inversion.
The magnetization of the starch-coated samples shows the effect of starch deposition and the consequences of the mixing process in the starch solution. Changes in the magnetization that are not accompanied by corresponding changes in Δx are the result of altered agglomeration of the magnetic nanoparticles. Therefore, only significantly reduced values of ΔM < 10% (which cannot be associated with an increase in x) undoubtedly confirm the success of the encapsulation process, i.e., that the nanoparticles or their agglomerates are completely coated with a layer of starch. A larger amount of starch results in a smaller contribution from the magnetic core and a lower total magnetization of the coated nanoparticles. Additionally, diamagnetic starch partially reduces the total magnetization of the coated nanoparticle because its own magnetization is oriented opposite to the external magnetic field.
The coercivity
Hc =
f(
D) is proportional to the size of the nanoparticles,
Figure 6b. For all coated samples,
Hc is less than 2–43%, except for ME(s) where it is 1% higher. The decrease in
Hc values for the starch-coated samples indicates less interaction between the particles (due to the presence of starch) and consequently easier realignment in an external magnetic field. In addition to the influence of starch, the
Hc value is also influenced by the size change that may have taken place during the starch deposition process. The increase in nanoparticle size due to the increased core/shell ratio leads to an improvement in the structure (on average), and thus to an increase in mutual interactions and a more difficult realignment of magnetic moments in an external magnetic field. The increase in ME(s) nanoparticles can be one reason for the increase in Hc. On the other hand, the CO(s) sample has the lowest
Hc value (43% lower than
Hc of pure CO). This decrease in
Hc confirms that the average size of the NPs in the CO(s) sample is significantly reduced.
The starch coating process has probably led to the partial dissolution of small nanoparticles due to the strong mixing of the solution. Then, Ostwald ripening can lead to the growth of larger nanoparticles at the expense of the reduction of smaller nanoparticles.
The decrease in
Hc, (which is barely perceptible on the broad scale of
Hc in
Figure 6b, despite the increase in NP size for some nanomaterials (except CO(s)), shows that even incomplete capping has reduced the dipole magnetic interaction in the NPs.
The value of the magnetization in a weak magnetic field,
H = 100 Oe, at 5 K (and the curvature of the magnetization
MFC =
f(
T)) depends on the magnetic anisotropy as
Hc. For pure samples,
MFC = Const. −
f(
D), (black dashed line) at
T = 5 K, i.e., the decrease in
MFC is proportional to the increase in particle size
D,
Figure 6c. The
MFC values of the starch-coated samples show the same trend as for the pure nanomaterials. There are no comparable changes to the magnetization measured at 300 K,
Figure 6a. A significantly larger value of the magnetic moments of the cations in the nanoparticles of CoFe
2O
4 at 5K (
μFe = 5
μB and
μCo = 3.36
μB) is observed compared to
μFe = 3.25
μB and
μCo = 2.5
μB at 300 K [
22], overcoming the influence of the covering starch layer at low temperatures. The graph in
Figure 6c shows the changes in size of the magnetic CoFe
2O
4 nanoparticles before and after the starch coating process, but without any visible effect of the starch itself on the values of
MFC.
To summarize, a relatively small amount of starch is bound to the NP-s, so the starch had no effect on reducing agglomeration. In TEM and SEM [
21], no starch is visible. Perhaps new aggregates of nanoparticles were formed due to the incomplete coating of starch.
The starch coating should reduce the surface tension and thus the internal tension to a certain degree. This effect was observed for all coated nanoparticles, except for CO(s), where a significant reduction in NP size caused an increase in internal tension. If the starch had completely covered the surfaces of the NPs, the effect would have been more pronounced, so that an increase in the lattice constants could have occurred, but an increase in aexp is only visible for US-CO(s) and MC-CO(s).
In the case of CO(s), aexp decreased. Partial dissolution of a large proportion of the small particles in CO(s) occurred, so that the average size in the ensemble decreased, the internal stress increased and the crystal lattice contracted.
In MC-CO(s), a sufficiently large amount of starch is registered on the surface of the nanoparticles, which leads to the obscured of the magnetic core and a significant decrease in the saturation magnetization, Ms.
The 10% decrease of Ms in ME(s) is difficult to explain due to the extremely low amount of adsorbed starch (if the coating of primary aggregates is excluded). At the same time, a slight increase in Hc and D was registered.
3.3. Raman Spectroscopy
As we have already seen, all analyzed CoFe
2O
4 samples showed a typical XRD pattern of
Fd-3m space group, i.e., macroscopically are cubic. The factor group analysis predicts 42 phonon modes for the normal cubic spinel structure: three acoustic of
T1u symmetry and 39 optic modes distributed among the following symmetries in the center of the Brillouin zone [
28,
29]:
Five of these phonon modes are Raman active, namely A1g, Eg and 3T2g; four are IR active, 4F1u, and remaining modes are silent.
Raman spectra are more sensitive to local symmetry and exhibit asymmetric or dissociated peaks characteristic of inverse and partially inverse spinel structures. For simplicity (as is usual), the Raman modes are assigned as for normal cubic spinel.
Figure 7 shows the Raman spectra of bare and starch-coated nanopowders with fully separated components of the
A1g mode typical for (Co
1-xFe
x)[Fe
2-xCo
x]O
4.
The spectra of the coated NPs do not clearly show the presence of starch, probably due to the low amount of starch and the poor quality of the spectra. The starch peaks around 480, 860 and 940 cm
−1 are not visible, but small bumps at 840 cm
−1 and 930 cm
−1 in some spectra, marked with an asterisk in
Figure 7b, could be a trace of starch [
25].
Raman spectra are fitted with seven (or eight) Lorentzians. The values of the wavenumbers are generally consistent with the literature [
30].
The
A1g mode is divided into an
A1g (1) component, which arises from the stretching vibrations of O
2- in tetrahedra with central cation Fe
3+ (Fe
3+-O4 bonds), and an
A1g(2) component, which arises from the stretching vibrations of O
2- in tetrahedra with cation Co
2+ (Co
2+–O4 bonds). The intensities of these modes are proportional to the number of corresponding cations in the A-site of the cubic spinel, so that the value of the inversion coefficient
xR can be roughly estimated from the ratio of the intensities:
Here,
r—stands for the relative oscillator strength of the Co
2+-O
4 bonds in relation to the Fe
3+-O
4 bonds and
IA1g(1,2) are the corresponding Lorentzian areas. The force constant
k, which determines the mode frequency
ω2 ∝
k/m, where m is the reduced mass of the ions, is directly proportional to the charges Z
A and Z
O the central cation or oxygen of the A site and inversely proportional to the cubic number of the associated bond length
rA-O, as
k ∝ Z
AZ
O/r
A-O3 [
31]. The ionic radii of the tetrahedral Co
2+ and Fe
3+ ions are 0.58 Å (high spin) and 0.49 Å (high spin), respectively, and the radius of the oxygen O
2- in the tetrahedra is 1.38 Å [
26]. Therefore, the relative oscillator strength of the Co
2+ bonds in relation to the Fe
3+ bonds in tetrahedra is:
The calculated Fe contents in the tetrahedral range,
xR, for various cobalt ferrite samples are shown in
Figure 7.
When compared with the inversion coefficients obtained on the basis of XRD structural analysis (stars) (
Figure 8), it can be seen that
xR (circles) follows the trend of change, i.e., it gives a fairly good picture of the redistribution of cations in the starch-coated nanomaterial.
Spectral intensities and Lorentzian widths in deconvoluted Raman spectra can be associated with structural disorder. In the spectra of starch-coated NPs, the weak F2g (3) mode is more clearly visible than in the spectra of bare NPs, regardless of whether their average size increased or decreased during the mixing process in the starch solution. It can be concluded that all coated nanopowders experienced some reduction in structural disorder.
The disappearance of the A1g* mode also confirms that the coating leads to a reduction in structural disorder. Indeed, in order to match the spectra of the bare MW-HT and MC-CO samples, it was necessary to introduce the A1g* mode, which corresponds to the maghemite-like depleted surface layer. After the starch coating process, these peaks disappear in both materials, and the intensity of the spectra becomes higher. The intensity of the MW-HT(s) spectrum is higher than that of the bare NPs, although the average size of the coated NP-s is slightly reduced according to XRD.
The average size of nanoparticles in MC-CO(s) increases during the coating process. The size distribution becomes narrower, and the average size increases at the expense of the smallest nanoparticles. As the width of the blocking temperature (
TB) distribution is equivalent to the width of the size distribution, narowing of size distribution is confirmed in
Figure 9, which shows the results of fitting the
TB distribution for starch-coated and bare samples. The fitting model and procedure on the basis of the modified Stoner-Wohlfarth model [
32,
33] were applied in our previous work, Ref. [
22], for uncoated samples.
Based on the data from
Figure 9, a clear narrowing of the size distribution for the MC-CO(s) sample and a reduction in the Δ
max ∝
1/
Keff compared to bare MC-CO can be seen. Reduction of Δ
max in MC-CO(s) coincides with the increase of nanoparticle size. For the MW-HT(s) sample, with greater nanoparticles and an unchanged narrow size distribution, the changes in Δ
max are much smaller and accompanied by a slight decrease in nanoparticle size. The Raman spectra of these two samples show that the starch coating leads to a reduction in the magnetically depleted shell of the nanoparticles.
3.4. 57Fe-Mössbauer Spectroscopy
57Fe-Mössbauer spectroscopy is a perfect and efficient characterization technique to investigate the local structure of the Mössbauer-active element such as Fe. Spin behaviors of the bare, caped, core–shell iron oxide nanoparticles were discussed, based on the results of Mössbauer spectroscopy. In our previous work, the
57Fe-Mössbauer spectroscopy was used to investigate the pure CoFe
2O
4 nanoparticles prepared by different synthesis routes [
34]. In this work, we investigated the same samples that were afterwards additionally coated with starch. The aim is to determine in which way the process of starch coating and the presence of starch on the surface of nanoparticles impact the structure and magnetic properties of CoFe
2O
4. The Mössbauer spectra of pure nanomaterials and the same nanomaterials with a starch coating are presented together in
Figure 10 for easier comparison. The fitting results are shown in
Table 4 and
Table 5.
Mössbauer spectra shown in
Figure 10 are analyzed by Voigt-based fitting method (VBF) to describe arbitrarily-shaped hyperfine parameter distributions [
35]. The thickness corrections were performed and the results presented in
Table 4 and
Table 5 are for the thin-limit spectra. The relative peak areas (3:2:1:1:2:3) and the Lorentzian linewidth (HWHM = 0.097 mm s
−1) were fixed during the fitting procedure. The background was not allowed to float in the fits. In the case of starch-coated nanoparticles, a correction was made for the mass of starch obtained by TGA.
Each spectrum is fitted with two magnetic generalized sites (two broadened sextets depicted by the hyperfine field distributions, HFDs) corresponding to the main tetrahedral (A-site) and octahedral (B-site) Fe and one weak sextet corresponding to the disordered spins of Fe atoms present at the surface of the nanoparticles (in the magnetically depleted shell). For samples with smaller average size of nanoparticles, additional paramagnetic generalized site (broadened doublet depicted by the quadrupole splitting distribution, QSD) was necessary to describe some of the Fe atoms that are in superparamagnetic (SP) surrounding. Due to cation distribution, we used four Gaussian-components for describing distribution of the effective hyperfine magnetic field of octahedral Fe and two Gaussian-components for the field of less sensitive tetrahedral Fe [
36,
37,
38]. For the poorly defined weak sextet (HFD site 3), the quadrupole shift was set to zero as for the ideal cubic spinel [
39] and the isomer shift was set to 0.33 mms
−1 in the final fits. It was found that such a sextet best describes the part of each spectrum where the absorption lines strongly overlap.
The paramagnetic contribution to the magnetic measurements is visible in all samples, but for the Mössbauer experiment the critical diameter of the SP particles is much smaller:
Dsp < 3.3–5.4 nm.
Dsp can be calculated based on the data [
22], for the anisotropy constant
Keff(300K) ≈ 5 J/m
3 and by the Néel–Arrhenius law [
40]:
τm =
τo exp (
Keff·v/(
kB·
T)), where the measurement time for the Mössbauer experiment is
τm = 10
−8 s and the characteristic relaxation time is τ
o ~10
−9–10
−12 s. For magnetic measurements,
Dsp is < 8 nm when
τm = 100 s [
41]. Due to the much shorter measurement time, there are more blocked nanoparticles and a lower contribution from SP in Mössbauer measurements.
Assuming that the recoilless factors of the
57Fe nuclei located at different crystallographic sites are the same, the relative area (
S) of the corresponding Mössbauer partial spectra is equal to the relative site population (Pop.):
SA/
SB = PopA/PopB. Therefore, the relative proportion of Fe at the site is:
SA/
SB =
x/2 −
x. The coefficient of cation inversion can now be estimated as follows:
We first fitted the spectrum of the ME sample whose A- and B- sextets are not completely overlapped. The inversion coefficient calculated based on the population values of A and B sites (Equation (10)) agrees quite well with the inversion coefficient determined by XRD (within the margin of error of xXRD). In the preliminary fits of other samples, we started from ME values as fixed hyperfine parameters, only the areas of the generalized sites were to float. After this preliminary adjustment to the individual spectrum was done, we lifted some of the constraints. Finally, from the various accepted fits, we choose the ones that were in overall agreement with each other regarding physical meaning.
Table 4 shows that the maximum values of the average hyperfine magnetic field, <|
Bhf|>, were obtained for the ME and MW-HT samples with the largest nanoparticles. Samples with smaller nanoparticles, obtained by coprecipitation methods: CO, US-CO and MC-CO, show lower values of <|
Bhf|>. Thereby, the values of <|
Bhf|> for
57Fe B-site in both groups increase with the increase of the inversion coefficient. It is expected considering the increase of the superexchange interaction, J
AB due to increase in the number of Fe ions in A-site with stronger superexchange interaction: J(Fe
B-O-Fe
A) > J(Fe
B-O-Co
A) [
37]. The values of <|
Bhf|> for the A-site show no clear dependence. This is also to be expected for relatively small nanoparticles, as the total J
AB of tetrahedral
57Fe changes significantly less with a change in the degree of inversion.
The CO and MW-HT samples exhibit the largest deviations between the degrees of inversion determined by Mössbauer analysis (xMoss) and those obtained from XRD analysis (xXRD). For the other samples, the differences are smaller. As mentioned above, the sextet overlap prevents a more accurate determination of the inversion coefficient.
The relative areas of the doublets in the Mössbauer spectra of the samples with the -smallest nanoparticles are very small (≈0.9–3.1%). It can be concluded that among the samples with visible doublets in the spectra, the US-CO nanoparticles have the narrowest size distribution, and the MC-CO nanoparticles have the broadest size distribution.
All samples had to be fitted with an additional, poorly defined sextet (HFD-site 3), which is obviously related to the magnetically disordered surface layer of the nanoparticles. The contribution of HDF-site 3 is significant in the spectra of the samples with smaller particles, while its relative area is minimal in ME sample. The volume percentages of the disturbed, magnetically depleted layers estimated for pure CoFe
2O
4 samples in our previous paper (Ref. [
22],
Table 5), are significantly higher than the effective area of HFD-site 3. As a reminder, the influence of the less magnetically disordered parts of the surface layers of the nanoparticles, the “shell”, is taken into account in the fitting of the Mössbauer spectra via additional Gaussian components for the distribution of the effective hyperfine magnetic fields of the A and B sites.
The
57Fe-Mössbauer spectra of the investigated starch-coated CoFe
2O
4 samples are shown in
Figure 10 and the fitting parameters are listed in
Table 5. The comparison of the raw data for the starch-coated and untreated CoFe
2O
4 samples shows that the spectra are basically very similar. Only slight changes in the parameter values could be recognized. In the coated nanoparticles, the electrostatic interaction of the polar starch molecules with the surface of the nanoparticles leads to a decrease in Fe spin disorder. The consequences, such as the decrease in line broadening and the increase in the strength of the HF fields, are as expected.
In the fits of all starch-coated CoFe2O4 samples, we started from the corresponding “non-coated” CoFe2O4 values as fixed 57Fe-Mössbauer parameters. As the first fitting step, only the areas of the generalized sites were allowed to float. After this adjustment to the individual starch-coated spectrum, we allowed some of the parameters to float. The first parameters that were lifted are related to the surface and shell of the nanoparticles, under the assumption that the starch may dominantly influence the outer part of nanoparticle. We have used the information from the XRD determined degree of inversion for the individual sample to constrain some of the Mössbauer parameters. Finally, from the various accepted fits, we choose the ones that were in overall agreement with each other regarding physical meaning. The presented fits due to the overlap of the central components are not unique.
Table 5 shows that the hyperfine parameters for the starch-coated samples are comparable to those of the uncoated samples. Changes are observed in the values of HF field parameters and in the area populations, especially in the area population of the doublets. The reduction of the doublet area, i.e., the SP site population (from 0.9%, 1.37% and 3.1% in the uncoated US-CO, CO and MC-CO samples to 0.35%, 1.13% and 2.8% in the coated counterparts, respectively) suggests that the strong mixing in the starch solution led to the dissolution of the smallest nanoparticles and to the narrowing of the size distribution of the nanoparticles.
In US-CO(s), the decrease of the measured effective magnetic
57Fe hyperfine fields and the increase of their standard deviation are observed, which is related to the decrease of the local magnetic order. These changes indicate the decrease in the average size of the nanoparticles after starch coating.
Figure 10 clearly shows the broadened sextet peaks in US-CO(s) compared to the bare US-CO sample. The decrease in
D was confirmed by XRD and magnetic measurements. It is possible that the effects of nanoparticle reduction somewhat offset the potential effects of starch coating. The decrease in the inversion coefficient is consistent with ∆
xXRD.
The reduction in the standard deviation of the measured effective 57Fe HF magnetic fields in the ME(s) sample shows some increase in local magnetic order compared to ME.
In the case of CO(s), XRD and magnetic measurements confirmed that there was a reduction in nanoparticle size during the starch deposition process. Despite the size reduction, the decrease in the standard deviation of the HF field and the increase in all HF magnetic fields are registered in the CO(s) sample. These are exactly the changes in the fitting parameters of the Mössbauer spectrum that are expected when the starch is successfully deposited.
The fitting parameters of the MW-HT(s) spectra have changed slightly compared to the parameters of the bare counterpart MW-HT. The strength of the HF magnetic field in the surface layer increases significantly, i.e., the disorder decreases, and the coefficient of cation inversion decreases (which is accompanied by a slight increase in magnetization).
For the MC-CO(s) sample, the increase in the standard deviations σ(|Bhf|) with decreasing HF fields in the A-site and the surface layer as well as the increase in the effective area of the HFD-site 3 indicate a decrease in the size of the coated nanoparticles. However, the increase in the HF field at the B-site does not fit into the picture of a decrease in particle size.
Such inconsistent changes in the parameters of coated and uncoated nanoparticles are the result of different methods of nanoparticle production. Differences in surface quality, shape, nanoparticle size, size distribution, internal stress, etc. can lead to very different results under identical conditions of the starch coating process.
Mössbauer spectroscopy confirmed the influence of starch coating on increasing the magnetic order and decreasing the internal stress by cross-referencing the data obtained by XRD and magnetic measurements.