Open Access Article
Oscar F.
Odio
a,
Giuseppina
Tommasini
bh,
F. J.
Teran
cd,
Jesus G.
Ovejero
e,
Javier
Rubín
f,
María
Moros
*bg and
Susel
Del Sol-Fernández‡
*b
aSECIHTI-Instituto Politécnico Nacional, Laboratorio Nacional de Conversión y Almacenamiento de Energía, CICATA-Legaria, 11500 Mexico City, Mexico
bInstituto de Nanociencia y Materiales de Aragón, INMA (CSIC-Universidad de Zaragoza), C/ Pedro Cerbuna 12, 50009, Zaragoza, Spain. E-mail: m.moros@csic.es
ciMdea Nanociencia, Campus Universitario de Cantoblanco, 28049 Madrid, Spain
dUnidad de Nanomateriales Avanzados, iMdea Nanociencia, Unidad Asociada al CSIC, Madrid, Spain
eInstituto de Ciencia de Materiales de Madrid, ICMM (CSIC), Sor Juana Inés de la Cruz 3, 28049 Madrid, Spain
fDept. Materials Science and Metallurgy, Escuela de Ingeniería y Arquitectura (EINA), Universidad de Zaragoza, María de Luna 3, 50018 Zaragoza, Spain
gCentro de Investigación Biomédica en Red de Bioingeniería, Biomateriales y Nanomedicina (CIBER-BBN), Madrid, Spain
hIstituto di Science Applicate e Sistemi Intelligenti “E. Caianiello”, Consiglio Nazionale delle Richerche, Via Campi Flegrei 34, Pozzuoli, 80078, Italy
First published on 23rd July 2025
Composition is a key parameter to effectively tune the magnetic anisotropy of magnetic nanoparticles, which in turn can modulate their structural–magnetic properties and final applications. The Mn2+ content of manganese ferrite nanoparticles (MnxFe3−xO4) deeply impacts their structure, anisotropy, magnetism, and their heating capacity. However, a direct correlation between Mn2+ content, magnetic properties and heating efficiency is not yet clear. Herein, we report the synthesis of a wide range of MnxFe3−xO4 with x = 0.14 to 1.40, with similar polyhedral morphologies and sizes (13 to 15 nm). By varying the Mn2+ content (in the range of x = 0.0 up to 0.70), we successfully tuned the effective anisotropy while maintaining saturation magnetization nearly constant. Highest Mn2+ levels (x = 1.40) lead to structural changes and strain defects reflected in their poor saturation magnetization. Mn2+ substitution is not uniform, instead promotes a compositional gradient across the MNPs, with the surface layers having a higher concentration of Mn2+ than the core. The Mn2+-rich surface likely exhibits superparamagnetic (SPM) relaxation, while the core remains predominantly ferrimagnetic (FiM). Water transference results in cation leaching, promoting vacancies and changes in the local ferrite structure but with a minor impact on the magnetic properties compared with initial MNPs. We obtained the optimal Mn2+ content that maximizes anisotropy toward improved specific loss power (SLP) values. The Néel relaxation mechanism is warranted regarding variable composition when sizes and shapes are maintained. Our detailed analysis provides a better understanding of the effect of Mn2+ substitution on the heating efficiency through anisotropy modulation and straightforward guidance on optimizing MNP design for magnetic hyperthermia.
New conceptsWe present a successful strategy to tune the heating efficiency of manganese ferrite nanoparticles (MnxFe3−xO4) by systematically varying the Mn2+ content, while maintaining consistent the size and shape. This approach uncovers a direct correlation between the Mn2+ content, effective anisotropy, and heating performance – key parameters for optimizing magnetic hyperthermia agents. A key discovery is that Mn2+ incorporation is not uniform – it begins on the nanoparticle surface, creating a compositional gradient. This gradient leads to superparamagnetic relaxation on the Mn-rich surface and ferrimagnetic behavior in the core. We identify an optimal Mn2+ content (x ≈ 0.60–0.70) that maximizes effective anisotropy and SLP, while preserving biocompatibility (>90% cell viability after 24 h). In contrast, high Mn2+ levels (x ≈ 1.40) lead to structural defects, Mn3+ species, and reduced magnetization. Despite ion leaching during water transfer via PMAO coating, key magnetic properties are retained. This work provides critical new insight into how compositional control – independent of morphology and size – affects magnetic relaxation and heating performance, offering a rational framework for the design of stable, efficient, and safe magnetic nanoparticles for application in nanomedicine. |
These discrepancies across reports are also reflected in the optimal conditions for effective heat dissipation under an alternating magnetic field (AMF). For instance, similar specific loss power (SLP) under an AMF has been observed in samples with markedly different composition,14,15 whereas samples with similar composition produced significant differences in terms of heat generation depending on their internal structural defects.3 The optimal Mn2+ content needed to efficiently dissipate heat under similar AMF conditions is not yet clear.4,16
Therefore, further studies are necessary to better understand how composition can affect all these properties. More importantly, in many cases, these studies are performed exclusively in organic solvents, overlooking the impact that the water transference protocols can have on the final composition and the magnetic properties, potentially leading to partial or misleading interpretations. Soriano et al. reported Mn2+ leaching, and consequently, composition changes after water transference by using meso-2,3-dimercaptosuccinic acid (DMSA) and dopamine (DOPA) ligands.16 This leaching could alter the crystal structure of the MNPs, significantly affecting their magnetic properties.
In this work, we present a detailed and systematic study of MnxFe3−xO4 MNPs (xEmpiric = 0.14–1.40) with similar sizes and shapes, synthesized by a one-step thermal decomposition method, with the aim of investigating Mn2+ substitution effects on the structural, anisotropy, magnetic behaviour and heating properties of MnxFe3−xO4 MNPs. To achieve this, we synthesized seven MNP samples by varying critical synthetic parameters, including the ratio of metallic precursors, final solvent volume, and the surfactant-to-metallic precursor ratio. A detailed investigation into the manganese oxidation state and allocation of cations among the samples revealed, for the first time, that the incorporation of manganese ions into the ferrite structure begins at the outermost layers and progressively extends toward the MNP core. We concluded that Mn2+ substitution is not uniform: instead, a concentration gradient is observed, with a higher Mn2+ fraction on the surface. The Mn2+-rich surface dictated the preferential magnetic relaxation of the MNPs, as seen by Mössbauer spectroscopy. Finally, we investigated the impact of a polymer coating on the final compositions of the MnxFe3−xO4 MNPs, their crystal structure and magnetic properties. This work provides valuable insights into how tailoring Mn2+ content can be used to effectively tune anisotropy and heating efficiency, thus advancing the understanding and optimization of MHT.
000–50
000 Da), N-(3-dimethylaminopropyl)-N-ethylcarbodiimide hydrochloride (EDC), 4-aminophenyl β-D-glucopyranoside and 3-(4,5-dimethylthiazol-2-yl)-2,5-diphenyltetrazolium (MTT) were purchased from Sigma-Aldrich. Tetramethylrhodamine 5-(and -6)-carboxamide cadaverine (TAMRA) was purchased from Anaspec. All solvents were of analytical grade and used as received. Dulbecco's modified Eagle's medium (DMEM), fetal bovine serum (FBS), glutaMAX, and antibiotic penicillin–streptomycin (10
000 U mL−1) were obtained from Gibco, and 4′,6-diamidino-2-phenylindole dilactate (DAPI) and Prolong Diamond were obtained from Invitrogen. Phalloidin Alexa Fluor 488 was purchased from ThermoFisher Scientific. Glass 4-well chamber slides were obtained from Nunc™ Lab-Tek.
000 rpm for 2 h four times and finally the MNPs were redispersed in milliQ water for further use.
The crystal structure of the samples was identified by XRD powder patterns recorded using a Bruker D8 ADVANCE diffractometer working with CuKα (λ = 1.5406 Å) radiation. The patterns were collected between 10° and 70° in the 2θ range. Crystallite size and lattice strain were determined using the Scherrer formula:
d = kλ/β cos(θ) | (1) |
![]() | (2) |
cos
θ on the y axis against 4
sin
θ on the x axis, and their consequent linearly fitting, we get the strain component from the slope (ε = slope) and the crystallite size from the intercept (i = kλ/DW–H).20
The elemental analysis was performed using an inductively coupled plasma optical emission spectrometry (ICP-OES) instrument (PerkinElmer mod. OPTIMA 2100 DV). Typically, 25 μL of the MnxFe3−xO4 MNPs suspension were digested in 1 mL of aqua regia in a volumetric flask at 60 °C overnight. Afterward, the flask was filled up with deionized water.
The surface chemistry was elucidated from FT-IR spectra recorded using a PerkinElmer Spectrum Two spectrometer in the range of 400–4000 cm−1. Samples were lyophilized 24 hours before use.
Thermogravimetric analysis (TGA) of the metal precursors was performed in a PerkinElmer TGAQ5000 instrument from 40 to 500 °C at a rate of 10 °C min−1 and under a N2 flow rate of 25 mL min−1. Likewise, the MNP organic contents were determined by TGA using a Universal V4.5A TA instrument; the N2 flow rate was 50 mL min−1 and the heating rate was set at 10 °C min−1 until a final temperature of 800 °C. MNPs in organic solvents were dried in air, while MNPs in water were lyophilized before measured.
The hydrodynamic diameters and zeta potential of the MNPs were measured using dynamic light scattering measurements (Malvern Zetasizer Nano) at room temperature. Samples were prepared at a concentration of 0.05 mgFe per mL in Milli-Q water and sonicated 10 s before measurement.
X-ray photoelectron spectra were recorded with a Kratos AXIS Supra spectrometer equipped with a monochromatic source of Al Kα (1486.7 eV) working at 120 W with a base pressure of 10−9 Torr; the survey spectra were recorded at a pass energy of 160 eV with a step size of 1000 meV, while the high resolution spectra were registered with a step size of 100 meV at pass energies of 20 and 40 eV for metal 2p and 3s regions, respectively. Due to the magnetic nature of the ferrite samples, the magnetic lenses were disabled, and it was operated in the electrostatic-slot mode, setting an analysis area of ca. 2 mm × 1 mm. The powdered samples were measured without any treatment, and the charge neutralizer mode was kept on during the measurements. All spectra were analyzed with the Thermo Avantage software package. The background was described with a Shirley-type equation. Relative atomic contents from the metal 2p region were computed from the Scofield sensitivity factors and the energy compensation factors obtained using the TPP-2M method. The high-resolution spectra in the metal 3s region were fitted with Voight profiles obtained from a mixture of Gaussian and Lorentzian functions (80/20); details concerning the calculation of the relative atomic concentrations after the fitting procedure are provided in the ESI.†
Mössbauer spectra were collected using a constant acceleration spectrometer equipped with a 5 mCi Co57/Rh source. The velocity scale was calibrated with α-Fe foil and analysed using the MossWinn 4.0 software. Isomer shift values are given with respect to α-Fe.
:
1 HCl
:
HNO3) at 60 °C for 15 min. Then, the samples were diluted up to 300 μL with miliQ water. At this point, 50 μL (in triplicate) were used for the iron quantification by mixing the digested samples with 60 μL of 0.25 M 1,2-dihydroxybenzene-3,5-disulfonic acid (Tiron). This molecule forms a coloured complex with iron, and it can be investigated by spectrophotometry at λ = 480 nm using a microplate spectrophotometer (BioTek Synergy H1 UV/VIS, Agilent Technologies, Santa Clara, CA, USA) and the results obtained were compared with standard calibration curve results obtained with solutions of known iron concentrations (0–1000 μg Fe per mL). This protocol was performed after each glucose functionalization.
![]() | (3) |
water = 4.18 J g−1 °C−1) or water with different glycerol fractions from 0 to 50%, considering Cd
glycerol = 2.43 J g−1 °C−1 and for mixed water–glycerol Cd
mix = 3.30 J g−1 °C−1. The sample volume employed for the experiment was 1 mL.
Dynamical conditions: AC magnetometry measurements of the studied magnetic suspensions (mFe+Mn = 5 mg) were carried out using commercial inductive magnetometers (Advance AC Hyster Series; Nanotech Solutions, Spain) at 150 kHz and 300 kHz and field intensities up to 24 kA m−1. Each magnetization cycle is obtained out of three repetitions, resulting in the averaged magnetization cycle, related magnetic parameters (HC, MR, Area) and magnetic losses. SAR values were determined using the expression.22
| SAR = Af | (4) |
To elucidate the influence of the surfactant concentration on the overall composition, two MnxFe3−xO4 MNPs were synthesized using the same Fe(acac)3/Mn(acac)2 ratio (6.5) and a final solvent volume (50 mL), while slightly varying the OA/metallic precursor ratio from 2.6 to 3 (see Table S2 in the ESI†). The empirical x value, determined by ICP-OES, remained unchanged for both samples (xEmpiric = 0.18), indicating that under these synthetic conditions Mn2+ incorporation was insensitive to slight variations in the amount of surfactant. However, the sample synthesized using lower OA/metallic precursor ratios exhibited more irregular shapes (Fig. S1 in the ESI†). A plausible explanation is that limited OA availability leads to a preferential growth of the initial seeds along certain crystal directions (particularly those normal to the facets {111} and {110}, which are poorly stabilized by the OA, resulting in more irregular shapes. In contrast, sufficient OA during the nanocrystal growth ensures well-capped and stabilized crystal facets, leading to MNPs with controlled faceted shapes.24,25
The overall composition of the MNPs was then varied by changing the metallic precursor ratio and final solvent volume. Two series of MnxFe3−xO4 MNPs were synthesized: A Series (large-scale synthesis), where the MNPs were prepared in 150 mL of BzE, and B Series (small-scale synthesis) obtained using 50 mL of BzE. The Mn2+ content in both series was adjusted by changing the initial Fe(acac)3/Mn(acac)2 ratios, corresponding to theoretical x values of 0.40, 0.75, and 1.0 (Table S1 in the ESI†). In all cases, Mn2+ incorporated into the final MNPs was much lower than the theoretical values, based on the amount of Mn2+ added as initial precursor. This effect has already been described and is likely due to various factors, such as differences in the decomposition temperatures of the two precursors (most of the Mn(acac)2 decomposes at temperature of approximately 60 °C higher than that of Fe(acac)3, see Fig. S6 left panel in the ESI†) and/or the ionic radii differences between Mn2+ and Fe2+.16,26 However, this effect was not observed in other studies when using the same metallic precursors3,13 or oleates.2 Nevertheless, in the latter, octadecene was used as the synthetic solvent instead of BzE, making a direct comparison difficult. Moreover, it should be noted that in both series of MNP samples (A and B), the higher the molar concentration of the Mn2+ precursor used in the synthesis, the higher the Mn content in the final ferrite stoichiometry (Table 1). This tendency, determined by ICP-OES, was further confirmed by EDX for samples belonging to A Series (Fig. S2 in the ESI†).
| Samples | Fe/Mn precursors’ molar ratio in synthesis | x Theo value | x Empiric value | Measured formula | D TEM (nm) ± SD | (311) peak pos. (2θ°) | D XRD (nm) ± SD | D W–H (nm) ± SD |
|---|---|---|---|---|---|---|---|---|
| a Calculated using the Scherrer method. b Calculated using the Williamson–Hall method. | ||||||||
| A Series (150 mL) | 6.5 | 0.40 | 0.14 | Mn0.14Fe2.86O4 | 14 ± 3 | 35.43 | 12 ± 1 | 12 ± 1 |
| 3 | 0.75 | 0.23 | Mn0.23Fe2.77O4 | 13 ± 3 | 35.40 | 13 ± 1 | 18 ± 2 | |
| 2 | 1.0 | 0.37 | Mn0.37Fe2.63O4 | 15 ± 2 | 35.39 | 14 ± 2 | 15 ± 1 | |
| B Series (50 mL) | 6.5 | 0.40 | 0.18 | Mn0.18Fe2.82O4 | 13 ± 2 | 35.42 | 14 ± 1 | 15 ± 1 |
| 3 | 0.75 | 0.47 | Mn0.47Fe2.53O4 | 15 ± 1 | 35.39 | 13 ± 1 | 16 ± 2 | |
| 2 | 1.0 | 0.70 | Mn0.70Fe2.30O4 | 14 ± 2 | 35.35 | 13 ± 1 | 16 ± 1 | |
| 1 | 1.5 | 1.40 | Mn1.40Fe1.60O4 | 14 ± 1 | 35.26 | 13 ± 1 | 15 ± 2 | |
Additionally, the solvent volume influenced the incorporation of Mn2+ into the spinel structure (Fig. S3 in the ESI†). When the same Fe(acac)3/Mn(acac)2 ratio was used, the amount of Mn2+ incorporated into the spinel structure was consistently higher in the B Series (smaller volume of solvent) than in A Series (larger solvent volume) (Table 1). One hypothesis is that the use of a smaller solvent volume facilitates higher and more uniform temperatures throughout the mixture, improving the decomposition of the Mn(acac)2 precursor and thereby reducing the critical gap between the decomposition of metallic precursors and the saturation limit for particle nucleation.27 To further increase the Mn2+ content in the final MNPs, an additional synthesis was performed only for Serie B, as was the one incorporating more Mn2+ in the final structure (xTheo = 1.5, Mn1.50Fe1.50O4). The empirical x value was similar to the theoretical one (xEmpiric = 1.40, Mn1.40Fe1.60O4).
As shown in Fig. 1A and Table 1, all the synthesis yielded MNPs with similar polyhedral morphologies and sizes ranging from 13 to 15 nm, regardless of the metallic precursor's ratio or the solvent volume used. These results are in good agreement with previous works using the same precursors but different synthetic methods.13,16,28 Controlling the particle size and shape is crucial to isolate and accurately assess the influence of composition on the anisotropy and magnetic heating, while minimizing the influence of these parameters.
To investigate whether the tuned compositions could result in a single or core/shell MNP structure as previously reported,29,30 we carried out STEM-energy-dispersive X-ray spectroscopy analysis of selected MnxFe3−xO4 MNPs with the lowest, medium, and highest Mn2+ content (xEmpiric = 0.14, 0.70 and 1.40 respectively) (Fig. 1B). The chemical maps showed the presence of Mn and Fe signals along the magnetic cores and the absence of a marked core–shell structure, thus, confirming the successful synthesis of a unique MnxFe3−xO4 core in agreement with several reports.2,3,16
For further analysis, we selected samples with increasing Mn2+ content, that is, xEmpiric = 0.14, 0.23, 0.37, 0.47, 0.70, and 1.40. Fig. 2A shows the evolution of the XRD patterns of these MNPs together with the positions of the peaks corresponding to the MnFe2O4 spinel-type phase (PDF file 96-230-0619 in the ICDD powder diffraction file database). Interestingly, the presence of additional reflections (denoted with an asterisk) corresponding to the Fe1−xO phase (PDF file 96-101-1199) appeared for the samples with Mn2+ content x ≥ 0.70. The coexistence of both magnetic phases can have a high impact on the structural, magnetic, and heating properties of ferrite MNPs, as previously reported.3,31,32 As expected, we found a gradual shift toward lower angles while increasing the Mn2+ content from 35.43 (xEmpiric = 0.14) to 35.26 (xEmpiric = 1.40), taking as reference the reflection (311). This corresponds to an increase in the cubic unit cell parameter due to the substitution of smaller host ions (0.65 Å for Fe3+ and 0.78 Å for Fe2+) by a larger Mn2+ (0.83 Å),33 and to the appearance of strains inside the spinel structure.2,20 To further confirm this hypothesis, we calculated the strain (ε) component inside the spinel structure following the Williamson–Hall (W–H) method33 using XRD patterns and measuring the lattice distance for selected samples by HRTEM.33 As shown in the HRTEM images (Fig. 2B), the inverse FFT of the (220) plane distance increased from 0.286 nm (xEmpiric = 0.23) to 0.290 nm (xEmpiric = 0.37), in agreement with the XRD patterns. On the other hand, from the fitting of the W–H plot, we found that when the Mn2+ content increased from xEmpiric = 0.14 up to 1.40, the lattice strain increased from 0.20 × 10−3 to 2.12 × 10−3 (Table S3 in the ESI†), indicating a larger lattice spacing due to the introduction of Mn2+. This ultimately leads to the appearance of uniform tensile strain,20 which corresponds to the left shift shown in the XRD patterns (Fig. 2A). Although the lattice defects varied among the samples, the effect was more prominent for the sample with the highest content of Mn2+ (Mn1.40Fe1.60O4).
The average crystallite sizes calculated using Scherrer's formula (DXRD) and the W–H method (DW–H) ranged from 12 nm to 14 nm and from 12 nm to 18 nm, respectively (Table 1). In all cases, the mean MNP diameters obtained from TEM (DTEM) matched relatively well with the crystal sizes determined by XRD using both methods, indicating a single-crystal structure. No clear correlation between the Mn2+ content and the crystallite size was observed. Similar findings have been reported for MnxFe3−xO4 nanoparticles with homogeneous characteristics (∼6 nm in size, uniform shape, and oleic acid coating) in the range of x = 0.11 to 0.49.12 In contrast, other works have reported an increase of the crystallite size for MnxFe3−xO4 MNPs obtained by a similar synthetic procedure but using 1-octadecene as a solvent, or by co-precipitation in water using metallic chloride precursors.4,13 In contrast, a decrease in the crystallite size from 16.7 nm (x = 0) to 10.2 nm (x = 1) has been observed for Mn-doped CoFe2O4 ferrites.34 These discrepancies may be attributed to structural defects frequently associated with the increase of Mn2+ in the spinel structure, which could cause contraction of the crystal structure. In our case, the use of BzE as the solvent, rather than more reducing solvents like 1-octadecene, likely helped minimize the formation of such defects.3 Therefore, even when an increase in the Mn2+ content may have introduced some strain defects, these were insufficient to impact the final crystallite size of our MNPs.
All spectra were successfully fitted with two sets of doublets and a minor contribution at higher binding energy (BE). The doublet with the lower BEs (80–90 eV) corresponds to Mn cations, and the one with higher BEs (90–100 eV) is attributed to Fe cations. The occurrence of these doublets is primarily due to the multiplet splitting of the ionic final-state configuration 3s13dn, arising from the exchange interactions between the remaining 3s core-electron and the unpaired electrons in the valence 3d shell of the transition metals.35–37 This interaction gives rise to high spin (lower BE) and low spin (higher BE) final-state configurations, where the electron spins in the 3s and 3d shells are coupled either parallel or anti-parallel, respectively. Since the magnitude of the resulting energy splitting (ΔBE) is proportional to the total spin density of the 3d shell, this value has been used to identify the oxidation state of the ion,38,39 especially for compounds with high degree of ionicity. In addition, as the ΔBE is also proportional to the exchange integral between the 3s and 3d shells, it could be sensitive to covalent and ligand field effects.40,41
Fig. 2C shows the behavior of the computed ΔBE values after spectral fitting. Remarkably, a close correlation between the energy splittings of both Mn 3s and Fe 3s doublets is apparent. For the samples with xEmpiric ≤ 0.37, the splitting of the Mn 3s doublet is higher than 6.2 eV, which strongly suggests that the manganese ions are preferentially in the divalent state, with no evidence of oxidized species.39,42 These values are consistent with the results reported elsewhere for several manganese ferrites.43,44 At these low Mn2+ levels (xEmpiric ≤ 0.37), the recorded values of ΔBE for the Fe 3s doublet around 6.2–6.3 eV suggest the coexistence of Fe2+ and Fe3+ cations due to the partial substitution of Mn2+ in the ferrite structure.36,37,40,41 It is worth noting that, as the Mn2+ content in the ferrites increases (e.g., in samples with xEmpiric = 0.47 and 0.70), a gradual decrease in ΔBE of the Mn 3s doublet is observed. Such behavior could be related to either the appearance of a small fraction of Mn in a higher oxidation state (xEmpiric ≥ 0.70) or a less ionic environment of the Mn2+ ions in the spinel structure,45,46 which could suggest: (i) a gradual occupancy of tetrahedral sites by Mn2+ or (ii) a higher probability of –Mn2+–O–Mn2+– sequences at the expense of –Mn2+–O–Fe3+– sequences. At the same time, the splitting of the Fe 3s doublet increases, which is consistent with the progressive substitution of Fe2+ cations by Mn2+ in the spinel structure. In the case of the sample with the highest Mn2+ content (xEmpiric = 1.40), the further reduction of the Mn 3s ΔBE to 5.9 eV may indicate the coexistence of a Mn3+ fraction forming oxidized species. Meanwhile, the high value for the Fe 3s ΔBE (7.2 eV) indicates the predominant presence of Fe3+ cations inside the oxygen lattice consistent with a highly ionic environment.36,40,41,47 This observation suggests a preferential occupancy of the octahedral sites (B) by Fe3+.45,46 Additionally, the likely absence of Fe2+ ions is consistent with a massive substitution of Mn in the ferrite structure.
The recorded XPS spectra also provided a conclusive clue on the heterogeneity of the samples by analyzing the 2p and 3s signals of the cations. We have computed the Mn/Fe atomic ratios from the spectral fittings of the 3s region (Section S1 in the ESI†) and the direct integration of the corresponding 2p high-resolution spectra (see Fig. S4 in the ESI†). Using the TPP-2 formula previously reported,48 it is possible to estimate the inelastic mean free path (IMFP) of the photoelectrons coming from both spectral regions, which is a function of the photoelectron kinetic energy. For the Mn and Fe 3s photoelectrons with kinetic energy around 1400 eV, the IMFP is roughly 2.1 nm; in the case of the Mn and Fe 2p photoelectrons with kinetic energy about 800 eV, the IMFP is roughly 1.4 nm. Therefore, the information depth (3 times the IMFP) derived from the 2p and 3s signals covers the outermost 4 nm (2p) and the topmost 6 nm (3s) of the ferrite MNPs, respectively. The comparison between the computed Mn/Fe atomic ratios is displayed graphically in Fig. 2D, where both data sets derived from XPS are plotted against the Mn/Fe ratios obtained by ICP quantification. The dashed line with a unitary slope represents the ideal case where the surface composition computed by XPS agrees with the overall composition of the MNPs (ICP). From the graph, it is apparent that for the samples with xEmpiric ≤ 1.40, the estimated cation composition along the outermost 6 nm of the MNP (3s) is similar to the composition from the ICP data, which is consistent with the estimated average MNP diameters of 13–15 nm from TEM and DRX measurements. The fact that the 3s data are slightly biased toward higher Mn content in all samples could suggest that the Mn ions entering the ferrite structure do not reach the very core of the MNPs. On the other hand, by comparing the data sets from the 2p and 3s signals, it is noticeable that for xEmpiric ≤ 1.40 the Mn/Fe atomic ratio is systematically higher in the first 4 nm than if it is computed extending the probed depth for other 2 nm inside the MNP core. In other words, the nanoparticle's surface is enriched in the Mn2+ content with respect to the deeper zones near the core. This fact could indicate that the incorporation of Mn into the ferrite structure starts in the most superficial layers and then extends toward the interior of the MNPs.
Previous works50–52 on doped ferrites have also reported this surface enrichment of the doping element, which seems to be related to differing onsets of the nucleation process: when the nucleation step of the doping-containing monomers occurs late compared to the nucleation of the matrix-containing monomers, the doping element is initially out of the core of the resulting particle, and can develop a gradient concentration as a function of its diffusivity across the particle. This phenomenon is triggered by the aforementioned 60 °C difference in the decomposition temperature between Mn2+ and Fe3+ acetylacetonates, which produces monomers at different stages of the reactions that nucleate inhomogeneously. A thorough understanding of the magnitude of Mn gradient along the nanoparticle structure as a function of ferrite stoichiometry requires more in-depth studies using STEM–EELS and XPS combined with Ar ion cluster sputtering, which will be the subject of future work.
The results of the fits are shown in Fig. 2E and summarized in Table S10 of the ESI.† For the sample with xEmpiric = 0.14, the spectrum was successfully fitted with three hyperfine sextets and a small quadrupolar doublet. The two sextets with higher HFs and IS values around 0.3 mm s−1 are attributed to Fe3+ ions; the one displaying the largest HF (S1) corresponds to the cations that occupy A sites, while the other sextet (S2) is assigned to the cations occupying the B sites. The third sextet (S3) with a lower HF (ca. 43 T) and an IS near 0.5 mm s−1 can be attributed to the fictitious intermediate state Fe2.5+ due to the fast electron hopping between adjacent Fe2+ and Fe3+ cations along the B sites of the cubic spinel, above the Verwey temperature. As can be seen, the emergence of S2 is due to the imbalance between Fe2+ and Fe3+ cations due to the partial substitution of Fe2+ by Mn2+ in the ferrite structure. For the other two measured samples (xEmpiric = 0.23 and 0.37), additional sextets (S4–S6) were required. S4 is attributed to Fe2.5+ states where the Fe2+ and Fe3+ cations have different local environments with respect to those in S3 due to the emergence of inequivalent sites for Fe cations, i.e., the gradual incorporation of Mn2+ ions modifies the nearest-neighbor surroundings of Fe cations along the ferrite lattice. In contrast, S5 and S6 have large peak widths and HFs below the threshold value (40 T) for FiM behavior, indicating that these contributions encompass a fraction of Fe3+ and Fe2.5+ sites where the effective magnetic moment is no longer in a blocked FiM state, but it begins to fluctuate at a frequency that is on the order of the inverse of the Mössbauer characteristic time.
The rest of the spectral area contains only a broad quadrupolar doublet D1 (for the sample with xEmpiric = 0.14), or a distribution of HF values Sn (for the samples with xEmpiric = 0.23 and 0.37); such distribution is similar in both samples, with IS values centered at 0.3 mm s−1, pointing to a dominant contribution from Fe3+ cations and consistent with high Mn2+ substitution. The relative area of D1 is small in the xEmpiric = 0.14 sample (below 6%), while for the samples with higher Mn2+ concentration the overall contribution from Sn plus S5 and S6 sextets drastically increases above 40%. As was mentioned before, these spectral features indicate the occurrence of SPM relaxation, which can be the result of either small MNPs or MNPs with low magnetic anisotropy. Since the three samples exhibit similar size distributions, it is likely that the differences between them mostly arise from anisotropy effects across the particles. Indeed, the fact that the SPM contribution is more important for the samples with higher Mn2+ content strongly suggests that substitution of Fe2+ by Mn2+ in the ferrite lattice induces a decrease of the superexchange interactions,51 that is reflected in lower values of the magnetic anisotropy54,55 (see the next section). Moreover, since the XPS results point to a gradient of concentration with a large [Mn]/[Fe] molar fraction on the outermost part of the MNPs, it is likely that such SPM relaxation occurs preferentially on the surface of the MNPs. Hence, it can be inferred that sextets S1–S4 are associated with the inner part of the MNPs, i.e. the MNP cores exhibit FiM behavior at room temperature. Such a finding is further confirmed by estimating the ferrite stoichiometry from the relative area of these four contributions: the [Mn]/[Fe] molar ratio is 0.08, 0.13 and 0.20 for xEmpiric = 0.14, 0.23 and 0.37, respectively; these values are very close to those obtained from the 3s XPS data (cf.Fig. 2D), which provide information on the inner part of the MNPs, as has been pointed out.
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| Fig. 3 (A) Static magnetization cycles recorded at 300 K for the MNPs and (B) low field region of the magnetization cycles. | ||
The enrichment of Mn2+ cations in the outer part of the MNPs (see Fig. 2D) could promote a configuration where the spins close to the surface are canted and barely contribute to the MS in the static regime, explaining the unalterable MS values with increasing Mn2+ content. The heterogeneous allocation of Mn2+ cations and the level of Mn2+ substitution could play a major role in reducing the average HC and MR. In fact, even when MS values remained nearly constant across all samples, a slight decrease in the coercivity value (HC) was observed while increasing the Mn2+ content until xEmpiric = 0.70; beyond this point, however, an opposite effect was seen for xEmpiric = 1.40. The reduction of HCvia increased Mn2+ substitution ultimately led to a decrease in the effective magnetic anisotropy (Keff)60 as also evidenced with Mössbauer measurement, indicating a transition of the MNPs towards soft magnetic behavior (Fig. 3B). An exception is the sample with the highest Mn2+ content (xEmpiric = 1.40), where the presence of structural defects, associated with the concomitance of a reduced phase and Mn3+ fraction, effectively impacts their magnetic properties.
Similar results were recently reported for cobalt ferrite CoxFe3–xO4 type MNPs, where increasing the cobalt content had little effect on MS across samples, but led to a significant increase of Keff.61 In summary, considering that all samples exhibited similar average particle and crystallite sizes, and morphologies, the tuneable Keff, the preference of Mn2+ for tetrahedral sites and the heterogeneous allocations of cations could be the key properties influencing the ultimate magnetic properties.56
| Samples | Empirical x value before PMAO | Empirical x value after PMAO | Measured formula | D TEM (nm ± σ) | D DLS (nm ± SD) | Z potential (mV ± SD) | Organic content (%) |
|---|---|---|---|---|---|---|---|
| Mnx@PMAO | 0.14 | 0.07 | Mn0.07Fe2.93O4 | 12.9 ± 1.9 | 51.1 ± 1.6 | −38.1 ± 7.2 | 39.9 |
| 0.23 | 0.20 | Mn0.20Fe2.80O4 | 13.9 ± 2.1 | 65.5 ± 0.7 | −37.7 ± 6.1 | 27.3 | |
| 0.37 | 0.30 | Mn0.30Fe2.70O4 | 14.6 ± 2.3 | 66.5 ± 1.9 | −31.2 ± 4.8 | 23.6 | |
| 0.47 | 0.40 | Mn0.40Fe2.60O4 | 14.3 ± 1.2 | 66.6 ± 0.4 | −39.6 ± 8.2 | 32.0 | |
| 0.70 | 0.60 | Mn0.60Fe2.40O4 | 14.4 ± 1.8 | 69.4 ± 2.3 | −34.3 ± 6.8 | 28.4 | |
| 1.40 | 1.10 | Mn1.10Fe1.90O4 | 13.6 ± 1.3 | 66.5 ± 1.8 | −32.3 ± 4.2 | 34.6 |
Surface modification can play a major role in the redistribution of cations, ultimately modifying the final composition of the spinel structure and its functionality.63,64 To study the influence of the PMAO coating on the composition and, thus, on the structural and magnetic properties, the samples were characterized after coating by ICP-OES, FT-IR and XRD. From the ICP-OES results, we confirmed that Mn2+ ions leached out from the MNPs after PMAO coating (Table 2), as previously reported after DMSA or dopamine coatings.16 Mn2+ losses ranged from 13.0 to 21.4% of the initially incorporated amount across samples, except for the sample containing the lowest content of Mn2+, which exhibited a loss of nearly 50% of its Mn2+ ions. This trend aligns with the XPS data (Fig. 2D).
The stability of cations occupying surface sites also depends on their interaction with the surface ligand and/or the solvent.56Fig. 4B shows the FT-IR spectra of the selected MNPs with the lowest (xEmpiric = 0.07) and the highest Mn2+ content (xEmpiric = 1.10) after PMAO coating. In region I, the signals of ν(C–H) stretching mode belonging to the OA anchored to the surface of MNPs dominate, being more intense for the sample with the highest percentage of OA (xEmpiric = 0.07), as also confirmed by TGA. Next, region II is dominated by two broad bands that correspond to νas(COO−) and νs(COO−) modes of metal carboxylates, indicating the successful polymer coating. The intense band that appears in region III is characteristic of lattice Fe–O vibrations in spinel ferrites. Interestingly, as the Mn2+ content increased, this band showed a left shift, indicating the modification of Fe–O bond lengths and the rearrangement of the oxygen sublattice to accommodate different cation distributions among the octahedral and tetrahedral sites, which was affected by PMAO coating.56 In agreement with this, a gradual shift in the mean peak (311) position can also be seen by comparing the XRD patterns of samples before and after polymer coating, while the spinel ferrite structure was maintained (Fig. 4C).
The effect of polymer coating on the magnetic properties was evaluated at 5 K and 300 K, with results summarized in Table 3. In agreement with initial oleic acid coated MNP behavior, both the HC and the MR decreased to near zero values at RT, indicating that the SPM regime was preserved after surface modification. The MS values were slightly higher (85.0–89.0 A m2 kgferrite−1) than those of initial MNPs (see Section 3.4 and Fig. 3) or Fe3O4 MNPs (82 A m2 kg−1) obtained under the same synthetic procedure at 300 K (Fig. 4D). Changes in the magnetic properties after surface modification have been previously reported when using different polymers such as triethyleneglycol (TEG) and polyethyleneglycol (PEG), attributed to the reduction of the spin canting effect.65,66 However, this does not fully apply in our case, as the PMAO polymer is not directly coordinated to the iron ions but rather intercalated in the OA chains; nevertheless, the PMAO coating could be associated with ion leaching and subsequent cation's redistribution on the MNP surface,60,67 which is relevant for applications dependent on the surface properties such as AC hysteresis and relaxometry.63
| Samples Mnx@PMAO | 300 K | 5 K | ||||||
|---|---|---|---|---|---|---|---|---|
| M S (A m2 kg−1) | H C (kA m−1) | M R (A m2 kg−1) | M S (A m2 kg−1) | H C (kA m−1) | M R (A m2 kg−1) | H K (kA m−1) | K eff (105 J m−3) | |
| a Determined as the field at which the magnetization of the magnetized and the demagnetized branches differs in 3% of MS.60 | ||||||||
| Mn0.07Fe2.93O4 | 85 | 2.6 | 16 | 100 | 22.9 | 40 | 100 | 3.9 |
| Mn0.30Fe2.70O4 | 86 | 2.6 | 16 | 101 | 20.5 | 39 | 80 | 3.2 |
| Mn0.40Fe2.60O4 | 87 | 2.6 | 17 | 102 | 19.4 | 37 | 72 | 2.9 |
| Mn0.60Fe2.40O4 | 89 | 2.6 | 17 | 107 | 16.6 | 44 | 64 | 2.7 |
| Mn1.10Fe1.60O4 | 66 | 2.6 | 5 | 85 | 24.1 | 18 | 100 | 3.3 |
| Fe3O4 | 82 | 2.6 | 12 | 92 | 22.9 | 34 | 80 | 2.9 |
The effective anisotropy constant (Keff) values of the different MNP@PMAO samples were estimated from the formula
, with MS and HK being measured at 5 K following the Stoner and Wohlfarth model.60,68 The obtained values (Table 3) confirmed a decrease in Keff from 3.9 to 2.7 × 105 J m−3 as the Mn2+ content increased up to xEmpiric = 0.60 and an increase for samples with x ≥ 0.60, confirming the direct correlation between HC and the Mn2+ content. Keff values are approximate due to assumptions of full saturation, negligible temperature variation between 0 and 5 K, and limited interparticle interaction effects at high fields. It is noticeable that Keff for Mn0.60Fe2.40O4 is close to the values reported for MnFe2O4 MNPs (1–2 × 105 J m−3),60,69,70 which highlights the crucial impact of the Mn2+ content on the effective anisotropy of the samples.
The SLP computed values for high and low-frequency regimes appear in Tables S6 and S7 in the ESI.† These SLP values, shown in Fig. 5A and B, were fitted with a power law SLP = φHn, with φ being the mass concentration of the MNPs in the colloid, H the amplitude of the applied field, and n the power exponent (between 1.99 and 1.09) within the linear response theory (LRT).73,74 As low-frequency measurements did not produce accurate fitting, values were not considered. However, under a fixed frequency of 763 kHz (Fig. 5B), the quadratic field dependence of the SLP is fulfilled under all the range of magnetic fields tested, and it is independent of the composition (Table S7 in the ESI†). From these data, we can conclude that the variation of the composition (maintaining a similar size and shape) with the amplitude of the magnetic field only affects the regime of dissipation of the MNPs if the incorporation of Mn2+ produces structural defects and/or concomitant with different Mn species like Mn3+. In contrast, even with a very different Mn2+ content but without any impact on the average structural–magnetic properties, the heat dissipation regimen is warranted within the SPM regime. Still, the SLP values can be successfully tuned with the Mn2+ increase.
The magnetic relaxation process of MNPs dispersed in liquids results from individual or combination of Néel and Brown relaxation mechanisms.73,75 To unveil between the predominance of Néel and Brown relaxation to produce heat over the anisotropy energy barrier, we tuned the viscosity of the medium containing the MNPs. Specifically, our best nanoheater (xEmpiric = 0.60) was dispersed in water with increasing final amounts (% v/v) of glycerol (2% and 50%, viscosity range up to ∼ 15 mPa s75) and measured by calorimetry at a field intensity of 16.8–28.8 kA m−1 and f = 763 kHz. We observed that the SLP values remained unaltered when the viscosity of the media was changed (see Fig. S8 in the ESI†), suggesting that the Néel relaxation process is the predominant mechanism.61,76 This finding aligns with other works reporting that Fe3O4 MNPs of 16 nm and 14 nm in water and in glycerol, respectively, are needed to maintain the predominance of Néel relaxation mechanism in a broad range of frequencies (100 kHz to 1 MHz).61,77 In contrast, for more advanced compositions such as cobalt ferrite, the Néel relaxation mechanism predominates only within a size range of 6–10 nm.61,78 In our case, the predominance of Néel relaxation across compositions and in the range of 13–15 nm just by controlling Keff is a crucial strategy for the design of soft ferrite MNPs as heat mediators in complex environments such as tumors, where MNPs tend to aggregate, potentially compromising their magnetic properties.79–83
Fig. 5E depicts the AC hysteresis loops at 300 kHz for samples with xEmpiric = 0.0, 0.07, and 0.60, also showing a dependence on the Mn2+ content. The sample with xEmpiric = 0.60 presented the largest opening of the AC hysteresis loops, and thus, a SAR value of about 510 W gFe+Mn−1, whereas Fe3O4 MNPs in a similar range of sizes showed a smaller area (SAR = 184 W gFe+Mn−1) under the same AMF conditions (300 kHz, 24 kA m−1) (Fig. 5F and Table S9 in the ESI†). Linear SAR(Hac) dependence was maintained as in the case of 150 kHz measurement with a plateau deviation with amplitude ≥20 kA m−1 (Fig. S10B in the ESI†).
Aiming to compare both methods, we selected very near low frequencies, 155 kHz for the calorimetric method and 150 kHz for AC magnetometry at a fixed H of 16.8 kA m−1. Considering our best nanoheater (xEmpiric = 0.60), we obtained a SLP = 67.3 W gFe+Mn−1 by calorimetry compared with SAR = 144.5 W gFe+Mn−1 by magnetometry. These differences could be attributed to the non-adiabatic conditions employed for calorimetry measurements, resulting in lower dT/dt depending on the thermal exchange of MNP suspension with the surrounding media.85 However, if we compare the results depicted in Fig. 5A and D it is evident that the heating capacity tendency as a function of the Mn2+ content is maintained in both methods, showing their complementarity.
Then, we assessed the internalization of MnxFe3−xO4 in the MIA PaCa-2 cell line by fluorescence microscopy. As can be seen in Fig. 6C, large amounts of both MnxFe3−xO4 MNPs appeared internalized inside the cells as red spots in comparison with the control (cells without MNPs), suggesting high cellular uptake after 24 h of treatment. This result is important for applications like classical magnetic hyperthermia where high internalization of iron is required to achieve therapeutic heat. To confirm that, the intracellular iron content was measured by ICP-OES. After 24 h of treatment, the amount of intracellular Fe was 8 and 15 pg per cell for Mn0.07Fe2.93O4 and Mn0.60Fe2.40O4 MNPs, respectively. The different uptake between samples could be attributed to a different amount of glucose functionalized on the MNP surface, or to a diverse stability in biological media. Further studies to elucidate the dependence between MNPs composition and cellular internalization are still needed.
Footnotes |
| † Electronic supplementary information (ESI) available: Experimental conditions employed for the synthesis of the two series of MNPs. TEM characterization of samples with equal compositions but varying ratios of OA/Fe-Mn, EDX spectra, lattice strain calculations, a section dedicated to curve fitting of the high-resolution spectra of Mn 3s and Fe 3s signals and proper quantification of Mn/Fe ratios, high resolution XPS spectra, TGA analysis, the magnetic properties of oleic acid coated MNPs at 300 K, heating curves under different frequencies, SAR evolution vs. glycerol content, and SAR values obtained from AC magnetometry. See DOI: https://doi.org/10.1039/d5nh00254k |
| ‡ Present adress: Instituto de Ciencias Físicas, Universidad Nacional Autónoma de México, Av. Universidad s/n, Col. Chamilpa, Cuernavaca, Morelos 62210, Mexico. E-mail: sdelsol@icf.unam.mx |
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