Christoph P Guntlin1,2, Stefan T Ochsenbein1,2, Michael Wörle1, Rolf Erni2, Kostiantyn V Kravchyk1,2, Maksym V Kovalenko1,2. 1. Laboratory for Inorganic Chemistry, Department of Chemistry and Applied Biosciences, ETH Zürich, Vladimir Prelog Weg 1, CH-8093 Zürich, Switzerland. 2. Laboratory for Thin Films and Photovoltaics and Electron Microscopy Center, EMPA-Swiss Federal Laboratories for Materials Science and Technology, Überlandstrasse 129, CH-8600 Dübendorf, Switzerland.
Abstract
Colloidal nanoparticles (NPs) with myriads of compositions and morphologies have been synthesized and characterized in recent years. For wüstite Fe x O, however, obtaining phase-pure NPs with homogeneous morphologies have remained challenging. Herein, we report the colloidal synthesis of phase-pure Fe x O (x ≈ 0.94) popcorn-shaped NPs by decomposition of a single-source precursor, [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH. The popcorn shape and multigrain structure had been reconstructed using high-angle annular dark-field scanning transmission electron micrograph (HAADF-STEM) tomography. This morphology offers a large surface area and internal channels and prevents further agglomeration and thermal tumbling of the subparticles. [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH behaves as an antiferromagnetic triangle whose magnetic frustration is mitigated by the low symmetry of the complex. The popcorn-shaped Fe x O NPs show the typical wüstite antiferromagnetic transition at approximately 200 K, but behave very differently to their bulk counterpart below 200 K. The magnetization curves show a clear, unsymmetrical hysteresis, which arises from a combined effect of the superparamagnetic behavior and exchange bias.
Colloidal nanoparticles (NPs) with myriads of compositions and morphologies have been synthesized and characterized in recent years. For wüstite Fe x O, however, obtaining phase-pure NPs with homogeneous morphologies have remained challenging. Herein, we report the colloidal synthesis of phase-pure Fe x O (x ≈ 0.94) popcorn-shaped NPs by decomposition of a single-source precursor, [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH. The popcorn shape and multigrain structure had been reconstructed using high-angle annular dark-field scanning transmission electron micrograph (HAADF-STEM) tomography. This morphology offers a large surface area and internal channels and prevents further agglomeration and thermal tumbling of the subparticles. [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH behaves as an antiferromagnetic triangle whose magnetic frustration is mitigated by the low symmetry of the complex. The popcorn-shaped Fe x O NPs show the typical wüstite antiferromagnetic transition at approximately 200 K, but behave very differently to their bulk counterpart below 200 K. The magnetization curves show a clear, unsymmetrical hysteresis, which arises from a combined effect of the superparamagnetic behavior and exchange bias.
Broadening the toolbox
for the rational synthesis of nanomaterials
is currently one of the most important objectives in inorganic chemistry.
Nanosized materials such as NPs, have shown properties (optical, magnetic,
and electronic) and possess attributes (colloidal state, tunable surface
chemistry, etc.) that can benefit fields including bioimaging,[1] radiation detection,[2] light emission,[3] electrochemical energy
storage,[4] photovoltaics,[5] and many more. State-of-the-art synthetic methods set high
standards in the uniformity of the size, shape, and composition of
NPs in a colloidal ensemble.Wüstite FeO (in general x = 0.84–0.95), an antiferromagnetic
compound, crystallizes
in a NaCl-type defective crystal structure. The stoichiometric composition
(FeO) does not exist at ambient pressure and room temperature (RT).
All obtained substoichiometric wüstite phases have a deficiency
of iron, and hence the mixed valency (Fe2+/3+) is necessary
to maintain charge balance. Fe3+ cations move to unoccupied
tetrahedral sites in FeO, leaving behind
vacancies on octahedral sites.[6] According
to the phase diagram, bulk FeO disproportionates
into Fe3O4 and Fe below 570 °C. However,
this disproportionation reaction becomes immeasurably slow below 300
°C.[7] Thus, FeO exists as a metastable phase at room temperature.[6,8] Yin and ÒBrien[9] showed that colloidal
wüstite NPs can be synthesized at 320 °C due to the already
strongly reduced rate of redox disproportionation close to 300 °C.
Thus, FeO is kinetically stable at RT
in bulk and as NPs.[10] FeO NPs are expected to be faster oxidized in air as compared
to the bulk due to their larger surface area. However, fast oxidation
is generally not observed, and the oxidation rates strongly depend
on the capping ligands and the particle sizes/morphology. Thus, oxidation
can be slow and occurs mostly on the surface, leading to a ferromagnetic
shell covering the antiferromagnetic wüstite core.[11−13] Previously, FeO NPs with shapes such
as spheres, cubes, octapods, and truncated octahedra[9,14−18] were synthesized. Typically, single-source precursors such as iron(II)
acetate,[9,14,18] or Fe(acac)2–3,[14,15] or long-chain carboxylates[16,17] are decomposed in high boiling solvents or by selective oxidation
of Fe(CO)5 with pyridine N-oxide.[14] Another approach is to decompose Fe-oleates, leading to a wide variety
of NP shapes[16,17] and allowing the synthesis of
heterostructures such as wüstite/spinel[19] or wüstite/ferrite[20,21] core–shell
NPs. However, a clean wüstite phase has scarcely been obtained
at NP sizes below ∼20 nm because of the aforementioned surface
oxidation of FeO and the limitations
of these precursors in producing only Fe2+ species.In this report, we present a synthesis of novel, popcorn-shaped
FeO (x ≈ 0.94)
NPs (Figure ), with
high structural and size uniformity. The synthesis decomposes an iron(III)
oxo-trifluoroacetate single-source precursor (denoted as “Fe3OTFA”) in squalane as an inert solvent together with
trioctylphosphine (TOP) as a mild reductant and capping agent and
oleic acid (OA) and hexadecylamine (HDA) as capping ligands. The composition
of the FeO NPs with x ≈ 0.94 was elucidated by a Rietveld refinement of a powder
XRD pattern and by elemental mapping on the atomic scale using analytical
electron microscopy. We also detail the crystal structures of the
main precursor and three additional iron trifluoroacetate complexes
discovered in this work. Additionally, the magnetic properties of
the synthesized FeO NPs and their precursor
are presented and discussed.
Figure 1
Structural characterization of popcorn-shaped
FeO NPs (x ≈
0.94): (a, b) overview TEM
images, (c) slice through the reconstructed HAADF-STEM tomogram, (d)
reaction scheme for the NP synthesis, and (e) powder XRD (Cu Kα1, 1.540598 Å); inset: SAED spectrum of FeO NPs. (f) 3D tomography image reconstructed by tilt-series
of HAADF-STEM images.
Structural characterization of popcorn-shaped
FeO NPs (x ≈
0.94): (a, b) overview TEM
images, (c) slice through the reconstructed HAADF-STEM tomogram, (d)
reaction scheme for the NP synthesis, and (e) powder XRD (Cu Kα1, 1.540598 Å); inset: SAED spectrum of FeO NPs. (f) 3D tomography image reconstructed by tilt-series
of HAADF-STEM images.
Experimental Section
Synthesis of “Fe3OTFA” Precursor
Ten grams (62 mmol) of FeCl3 (Alfa Aeser, 98%) were
mixed with trifluoroacetic acid (100 mL, 1.3 mol, TFA, Fischer) in
a 250 mL two-neck round-bottom flask under N2 flow and
degassed three times by applying vacuum. Subsequently, the reaction
mixture was heated to 86 °C and left stirring for 2 h until a
homogeneous yellow suspension was obtained. Then 1 mL of deionized
water was injected, quickly turning the color of suspension into a
dark red. The solution was left stirring for additional 24 h at 86
°C. After cooling, TFA excess was distillated off under vacuum.
The remaining solid product, “Fe3OTFA”, was
dried at 60 °C under vacuum for at least 5 h, yielding a fine
red powder, which is directly useable without further workup. Despite
“Fe3OTFA” appearing stable under ambient
atmosphere, it was stored under vacuum until further use.
Synthesis of
Popcorn-Shaped FeO
(x ≈ 0.94) NPs
In a typical synthesis,
“Fe3OTFA” (337 mg, 0.3 mmol) was mixed with
HDA (1.304 g, 5.4 mmol, Aldrich, 90%), squalene (5 mL, Merck, ≥
99%), OA (3.6 mmol, 1.143 mL, Aldrich, 90%), TOP (5 mL, Strem, 15–6655,
> 97%) in a 25 mL three-neck round-bottom flask, forming a dark
solution.
This mixture was degassed by alternating between vacuum and N2 flow for 3 times at room temperature, followed by heating
under vacuum to 110 °C and left drying for another 1.5 h. Afterward,
the mixture was heated (19 °C/min) to 260 °C under N2. At ca. 210 °C, the solution changed color from black
to a clear, light yellow. Subsequent NC nucleation and growth processes
were visible as a color change from light yellow via brown to black
at 260 °C. After 20 min at 260 °C, the solution was rapidly
cooled to 110 °C and 20 mL of toluene were added, followed by
complete cooling. For purifying the particles, the reaction mixture
was mixed with 30 mL of ethanol as a nonsolvent and centrifuged (8000
rpm, 3 min), the supernatant was discarded and the precipitate was
dispersed in 10 mL of toluene.
Materials Characterization
Low and high resolution
transmission electron microscopy images (LRTEM/HRTEM) as well as selected
area electron diffraction (SAED) patterns were obtained with a JEOL
JEM-2200FS microscope operating at 200 kV. NCs were deposited onto
a carbon-coated Cu grids (Ted-Pella). A tomographic tilt-series from
−76 to 72° (2° steps) were recorded on an STEM-aberration-corrected
FEI Titan Themis operated at 300 kV with a probe semiconvergence angle
of 18 mrad (beam current 70 pA). The limits of the angular tilt-range
were given by shadowing of the Cu grid. The tomogram was reconstructed
based on high-angle annular dark-field scanning transmission electron
micrographs using FEI’s Inspect3D, and visualized using Amira
software. For element mapping using high-angle annular dark-field
scanning transmission (HAADF-STEM) electron microscopy, combined with
energy dispersive X-ray spectroscopy (EDX), a beam current of 6 nA
(no difference with 1 or 3 nA) and detection with a SuperEDX system
(4 detectors) were used. Powder X-ray diffraction (XRD) patterns were
obtained on a Stoe STADI P powder X-ray diffractometer (Cu Kα1 radiation, λ = 1.540598 Å, germanium monochromator).
The powders were measured on a transmission sample holder or in a
capillary (0.5 mm, Hilgenberg). For single-crystal measurements, a
suitable crystal was selected and tip-mounted either on a Bruker SMART
platform with an Apex I-detector diffractometer for “Fe3OTFA” at 250 K or on a Bruker D8 SMART platform equipped
with an Apex II detector for the other structures at 100 or 250 K
using graphite-monochromated Mo Kα radiation (λ = 0.71073
Å). Using Olex2,[22] the structure was
solved with the ShelXD[23] structure solution
program using Dual Space or with the Superflip[24−26] structure solution
program using charge flipping and refined with the ShelXL[27] refinement package using least-squares minimization.
Thermogravimetric analysis (TGA) coupled to mass spectrometry (MS)
was performed using a Netzsch simultaneous thermal analyzer (STA 449
F5 Jupiter) coupled (tubes at 200 °C) with a quadrupole mass
spectrometer (QMS 403 D Aëolos). “Fe3OTFA”
(13.1 mg) was placed in an aluminum crucible and heated under Ar gas
flow (40 mL min–1) to 500 °C (5 °C min–1). Fourier transform infrared spectroscopy (FTIR)
was measured on a Thermo Scientific Nicolet iS5 with an iD5 ATR accessory
(diamond). The device is located in an argon glovebox (O2 < 0.1 ppm, H2O < 0.1 ppm).
Magnetic Measurements
The magnetic properties were
measured on a Quantum Design PPMS-9. The magnetic susceptibility data
of “Fe3OTFA” were measured in an applied
magnetic field of 0.1 T between 2 and 300 K after cooling the sample
in zero field. The temperature-dependence of the magnetization of
FeO NPs was measured between 2 and 300
K in a field of 0.1 T after cooling without an applied field (zero-field
cooled, ZFC) and after cooling in a magnetic field of 0.1 T (field
cooled, FC). The field-dependence of the magnetization of FeO NPs was measured at 2 K after cooling in zero-field,
and at 2, 10, 50, 100, 200, and 300 K after cooling to 2 K in a field
of 1 T.
Results and Discussion
A direct
and reproducible synthesis of a single-source precursor
is the backbone of a successful nanoparticle synthesis method. For
the presented synthesis of wüstite NPs, the precursor quality
has a direct influence on the phase purity, size and shape of the
FeO NPs. A compound obtained by reacting
FeCl3 with TFA under reflux yields has been used as a catalyst
in several organic syntheses.[28−35] Our investigation of this reaction identified a mixture of several
products (Figures S1–S4, Tables S1–S8). Instead, [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH as a single product was obtained in this
work when the synthesis was modified by adding a defined amount of
water at a later stage of the reaction. The phase-pure precursor was
synthesized by reacting commercial FeCl3 and TFA at 86
°C for 26 h with the injection of water after 2 h. After evaporation
of the residual TFA, the precursor was obtained as a red, air-stable
powder and used for the synthesis of wüstite NPs without further
purification. We hypothesize that water ensures sufficient level of
hydrolysis of the preformed, suspended Fe(TFA)3. Instead
of adding water, FeCl3·6H2O as a starting
reagent also yields an identical precursor. However, the wüstite
NPs obtained from a precursor produced by water-assisted synthesis
were substantially more uniform and reproducible. The crystal structure
of our precursor, denoted as “Fe3OTFA”, was
determined using single-crystal XRD (see Figure a and the Supporting Information for all the crystallographic details) and has an
overall composition of [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH (Figure a and Figure S1 and Tables S1 and S2). The powder XRD pattern indicates phase purity (Figure b). “Fe3OTFA” crystallizes in the monoclinic space group P21/n. Three Fe3+ ions are arranged in a triangle around a central oxygen atom. Each
side of the triangle comprises two bridging trifluoroacetates. Trans
to the central oxygen atom, the sixth coordination site of the octahedral
coordinated Fe3+ ions is occupied either by H2O (2x) or by a trifluoroacetate. This trifluoroacetate group forms
a hydrogen bond to a TFA molecule. This “Fe3OTFA”
and another earlier published structure[36] are the only known compounds with exclusively Fe3+ ions
in the triangular core unit. Typically, this unit has only been observed
with mixed (Fe2+/3+) valency.[37−39] “Fe3OTFA” is isostructural to [Cr3(μ3-O)(CF3COO)6(H2O)2(CF3COO)]·CF3COOH.[38] To elucidate the decomposition of “Fe3OTFA”, a TGA-MS analysis was conducted (Figure S5). In addition to the structure of “Fe3OTFA”, three additional crystal structures were obtained
by varying the growth conditions of the single-crystal or by reducing
the synthesis temperature. All three structures and the crystallographic
details are presented in the Figures S2–S4 and Tables S3–S8. In this report, we focus exclusively
on “Fe3OTFA” as a precursor for the synthesis
of wüstite NPs, because this compound can be obtained in high
yield without further purification.
Figure 2
Structural analysis of the precursor:
(a) the crystal structure
of [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH as obtained from the single-crystal XRD and (b) simulated
and experimentally measured powder XRD patterns of this compound indicating
the excellent phase purity of the precursor.
Structural analysis of the precursor:
(a) the crystal structure
of [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH as obtained from the single-crystal XRD and (b) simulated
and experimentally measured powder XRD patterns of this compound indicating
the excellent phase purity of the precursor.Popcorn-shaped FeO (x ≈ 0.94) NPs (Figure a–c,f) were synthesized in a colloidal heating-up
synthesis
method at 260 °C (heating rate: ∼19 °C/min) by decomposing
“Fe3OTFA” in TOP/squalane (1:1 by mass),
HDA and OA under N2. The starting solution had a dark-red
to black appearance. It turned into a clear, slightly yellowish solution
at approximately 210 °C. A subsequent color change to brown and
then to metallic black indicated the nucleation and growth of NPs,
respectively. The growth was finished when the solution turned shiny
black. A reaction temperature of 260 °C for 20 min and a 12:18:1
OA:HDA:“Fe3OTFA” molar ratio yielded the
best size homogeneity. The size of the popcorn FeO NP clusters is slightly tunable by varying the precursor
amount between 0.3 and 0.4 mmol (Figure S6). Higher precursor amounts led to inhomogeneous size distributions.
For the synthesis of popcorn-shaped FeO NPs, obtaining the correct HDA/OA molar ratio and molar quantity
is crucial. The molar ratio has to be between 1.3 and 2 (HDA/OA),
and at least a 6-fold molar excess of OA to “Fe3OTFA” is needed. When the HDA amount is increased to a 22-fold
excess, the resulting FeO NPs are separated,
and no popcorn clusters are built (Figure S7). The growth mechanism of such polycrystalline popcorn-shaped NPs
might first involve the formation of small (sub-10 nm) nuclei, which
then aggregate into polycrystalline NPs. Such aggregation might be
caused by the reduced solubility of NPs as they grow. The temperature
at which the process occurs is presumably too low to cause efficient
fusion of these crystalline domains.The surface of the isolated
FeO NPs
appears to be covered exclusively by oleates, according to FTIR (Figure S8). TOP is known as an efficient phosphor
source[40] and hence might contaminate the
oxide. This possibility had been ruled-out by high-resolution elemental
mapping of FeO NP using EDX measurements
in HAADF-STEM mode (Figure ). A very small phosphide signal indicates no distinct P surface
shell, but at most a minute residual contamination. The growth of
the popcorn shape may be influenced by three ligands: OA, HDA and
an amide. The formation of the latter might be catalyzed in situ by
Fe3+ ions.[41,42] When adding “Fe3OTFA” only after the drying step (110 °C, 1.5 h, Figure S9), no popcorn-shaped FeO NPs are obtained, which supports the assertion
that Fe3+-catalyzed amide formation is crucial to obtaining
the popcorn-shape. The role of such a NP-yielding side reaction, whether
by the amide as a ligand or a fluorine radical trap or by inducing
a structural change in “Fe3OTFA”, remains
uncertain. To obtain the wüstite phase, all four reactants
(HDA, OA, TOP, and squalene) are needed, which was verified by excluding
them one by one. The decomposition of “Fe3OTFA”
in HDA/OA or HDA/TOP/squalene produces Fe3O4 NPs, indicating that the combination of OA with TOP/squalane reduces
Fe3+ to Fe2+. Interestingly, in addition to
the popcorn-shaped FeO, a second phase
of highly monodisperse wüstite NPs appears when using slightly
increased amounts of OA/HDA and synthesis time (Figure S10). Herein, we focused on the synthesis of popcorn-shaped
NPs as this novel structure offers a unique morphology by combining
approximately 14 nm large subparticles into clusters measuring up
to 60 nm. The individual crystallite size was determined by Rietveld
refinement (Figure S11) using a Si standard
reference (NBS, no. 640, PDF 027–1402) to deconvolute the instrumental
broadening. Such clusters, unlike completely fused nanocrystals, still
provide a large surface area, but further agglomeration seems inhibited.
Additionally, they have intrinsic channels that can be visualized
by TEM tomography (Figure c and Video S1).
Figure 3
Elemental mapping using
EDX measurements of FeO nanoparticle
in the HAADF-STEM mode. (a) STEM image of a
FeO nanoparticle. The yellow frame shows
the area #1, from where the integrated STEM EDX spectra (see f and
g) were extracted. The green line (integrated) shows the taken line
profiles of the background corrected peak intensities. (b) Line profiles
representing intensity distribution of Fe (red), O (green), P (blue),
and HAADF (black). The elemental maps of the FeO particle for (c) Fe, (d) O, and (e) P. (f) Integrated STEM
EDX spectrum taken from the yellow area #1 indicated in a. (g) Zoom
into the STEM EDX spectrum showing a minor peak of P, which is 200
times smaller than the Fe–Kα peak. Cu arises from the
sample holder (Cu grids) and the small Si peak from the detector.
Elemental mapping using
EDX measurements of FeO nanoparticle
in the HAADF-STEM mode. (a) STEM image of a
FeO nanoparticle. The yellow frame shows
the area #1, from where the integrated STEM EDX spectra (see f and
g) were extracted. The green line (integrated) shows the taken line
profiles of the background corrected peak intensities. (b) Line profiles
representing intensity distribution of Fe (red), O (green), P (blue),
and HAADF (black). The elemental maps of the FeO particle for (c) Fe, (d) O, and (e) P. (f) Integrated STEM
EDX spectrum taken from the yellow area #1 indicated in a. (g) Zoom
into the STEM EDX spectrum showing a minor peak of P, which is 200
times smaller than the Fe–Kα peak. Cu arises from the
sample holder (Cu grids) and the small Si peak from the detector.For magnetic iron oxide-based
NPs the combined effect of the granularity
and the coexistence of the antiferromagnetic wüstite and uncompensated
surface spins or surface oxides (γ-Fe2O3 and/or Fe3O4) can overcome the superparamagnetic
magnetic limit due to the exchange bias arising at the interface of
the oxides,[43] and by reducing the thermal
tumbling of small subparticles because the cluster holds them in place.
The phase composition of these FeO NPs
remained constant for weeks. To obtain more insights into the properties
of the wüstite NPs and the precursor (“Fe3OTFA”), we conducted magnetic measurements.Figure a shows
the magnetic susceptibility of the precursor “Fe3OTFA”, plotted as the χT product as
a function of the temperature. χT at 300 K
is 5.3 emu K mol–1, and it decreases to 0.45 emu
K mol–1 at 2 K. The room temperature value is lower
than expected for three uncoupled spins s = 5/2 of high- spin Fe3+ ions, χT = 13.125 emu K mol–1 (for g = 2). This lower-than-expected
value at RT and the steady decrease in χT with
decreasing temperature indicate strong antiferromagnetic interactions
between the high-spin Fe3+ ions. The magnetic properties
of a polynuclear spin-only complex can be modeled based on the spin
Hamiltonian, as shown in eq. :[44]where J are the exchange coupling constants, are the spin operators, g are the Landé factors, μ is the Bohr magneton and is the magnetic field
vector. Using PHI,[45] the data can be fit
based on eq with i,j = 1,2,3 enumerating the Fe3+ ions. The best
fit, shown as a solid black line (Figure a), was obtained with J12 = J13 = −28.7 cm–1, J23 = −43.2 cm–1, and g1 = g2 = g3 = 2.32, comparable
to a recently studied oxygen-centered Fe3+ triangle.[46] This fit represents an isosceles triangle. While
the symmetry of the “Fe3OTFA” core is low
enough that three different exchange coupling constants and three
different g-values could be used, such a model does
not improve the fit significantly but instead overparameterizes the
model. An argument can be made for an isosceles triangle based on
the coordination of the Fe3+ ions: one has a different
coordination than the other two (trifluoroacetates vs water trans to the central oxygen atom). Therefore, the complex
contains two interactions between dissimilar Fe3+ ions
and one between similar ones. Antiferromagnetic interactions in a
triangle cannot all be satisfied at the same time; they are in competition.
In an equilateral triangle, i.e., where all three exchange coupling
parameters are the same, the molecule is spin frustrated with a doubly
degenerate S = 1/2 ground state, which is unstable
toward distortion or higher order exchange interactions (e.g., Dzyaloshinskii-Moriya
interactions). In “Fe3OTFA”, the degeneracy
is lifted by the unequal interactions in the triangle, leading to
a gap between the two lowest S = 1/2 states (inset
of Figure a).[46]
Figure 4
(a) Magnetic susceptibility (as the χT product)
of “Fe3OTFA” vs temperature. Solid line:
best fit to the Hamiltonian (eq ) with parameters g = 2.32, J12 = J13 = −28.7 cm–1, J23 = −43.2 cm–1. Inset: ground
state of an equilateral (frustrated) and an isosceles triangle. (b)
Magnetization vs temperature of popcorn-shaped FeO (x ≈ 0.94) NPs at 0.1 T, zero-field-cooled
(ZFC, black squares) and field-cooled (FC, red circles). (c) Magnetization
vs magnetic field of FeO NPs at 2 K after
zero-field cooling (ZFC, dotted black line) and after cooling in a
field of 1 T (FC, solid blue line); magnetization at 300 K (red dashed
line). Inset: expanded region around the origin.
(a) Magnetic susceptibility (as the χT product)
of “Fe3OTFA” vs temperature. Solid line:
best fit to the Hamiltonian (eq ) with parameters g = 2.32, J12 = J13 = −28.7 cm–1, J23 = −43.2 cm–1. Inset: ground
state of an equilateral (frustrated) and an isosceles triangle. (b)
Magnetization vs temperature of popcorn-shaped FeO (x ≈ 0.94) NPs at 0.1 T, zero-field-cooled
(ZFC, black squares) and field-cooled (FC, red circles). (c) Magnetization
vs magnetic field of FeO NPs at 2 K after
zero-field cooling (ZFC, dotted black line) and after cooling in a
field of 1 T (FC, solid blue line); magnetization at 300 K (red dashed
line). Inset: expanded region around the origin.The magnetic properties of FeO NPs
are presented in Figure b. Both the zero-field-cooled (ZFC) and field-cooled (FC) magnetization,
at a field of 0.1 T between 300 and 2 K, show a broad maximum at approximately
220 K and a decrease below 200 K, which is steeper in the ZFC curve.
The FC magnetization is almost flat between 150 and 25 K, after which
a relatively steep increase occurs with decreasing temperatures. The
ZFC magnetization is only flat down to 100 K, followed by a decrease
trending to zero. Below 25 K, however, an increase similar to that
in the FC magnetization is observed. The broad maxima at 220 K and
the sharp drop below 200 K are a clear indication of the antiferromagnetic
order known for wüstite, which has a Néel temperature
of ∼200 K. In bulk FeO, TN increases from 192.4 to 199.2 K between x = 0.95 and 0.929.[47,48] Therefore, TN ≈ 200 K for our FeO NPs is slightly higher than expected, possibly indicating
some nanosize effects. The divergence of the ZFC and FC magnetization
below the Néel temperature, however, is unexpected for an antiferromagnet
but indicative of superparamagnetism, ferromagnetism or spin-glass
freezing. The increase at low temperatures can probably be ascribed
to a paramagnetic impurity with a Curie or Curie–Weiss temperature-dependence
of the magnetization.The field-dependence of the magnetization
at 2 K shows a clear
opening around the origin, i.e., magnetic hysteresis. While the hysteresis
after ZFC is symmetrical around zero, it is shifted to negative fields
after cooling in a +1 T field. The coercive field of the 2 K ZFC magnetization
is ±0.2 T. The negative FC coercive field is −0.32 T,
and the positive side almost goes through the origin (0.02 T). Between
2 and 200 K, the FC coercivity narrows with increasing temperature
(Figures S12 and S13) and disappears by
300 K. The opening of a hysteresis at a low temperature supports superparamagnetism
as an explanation for the ZFC-FC divergence. The shift of the hysteresis
curve after field-cooling is reminiscent of exchange bias.[43,49] Put together, these observations indicate that the FeO NPs can be viewed as antiferromagnetic cores with
uncompensated surface spins. The surface spins lead to a net magnetic
moment in the NPs. Due to the coupling of the surface spins to the
antiferromagnetic core of the NPs, these surface spins have a preferred
orientation and can be frozen in that orientation below the Néel
temperature. That the hysteresis curves never saturate, not even at
9 T and 2 K, may also be attributed to the antiferromagnetic core
of the FeO NPs. Similar effects have
been observed in NiO and CuO NPs[50,51] but also in
FeO/Fe3O4 core–shell
NPs.[52−55] We cannot entirely rule out the partial oxidation of the FeO surface leading to a similar core–shell
structure, as in earlier publications.[52−55] In our case, however, any hypothetical
oxidized phase is below the detection limit of powder XRD and is invisible
in TEM. The presence of an exchange bias alone might not be a sufficient
evidence for the oxidation of the surface to form FeO/Fe3O4 core–shell NPs, as the
examples of NiO and CuO NPs indicate.[50,51]
Conclusions
A gram-scale synthesis of a phase-pure iron oxo-trifluoroacetic
precursor [Fe3(μ3-O)(CF3COO)(μ-CF3COO)6(H2O)2]·CF3COOH and its crystal structure are presented. Besides this
“Fe3OTFA” compound, three additional compounds
were obtained by slight variations of the reaction conditions or crystallization
procedure. “Fe3OTFA” had been then used as
a single-source precursor to obtain colloidal wüstite FeO NPs by decomposition in a high-boiling
solvent. These wüstite NPs show an unprecedented popcorn morphology
that offers large surface area and internal channels. A 3-D tomography
model created from HAADF-STEM images reveals the striking details
of these popcorn-shaped FeO NPs (see Video S1). Magnetic measurements of the FeO NPs show signs of the antiferromagnetic
order expected for wüstite but also shows a divergence of the
FC and ZFC magnetizations below TN, hysteretic
magnetization curves and exchange bias. The magnetism of the precursor,
“Fe3OTFA”, can be modeled by an isosceles
antiferromagnetic triangle.
Authors: Maryna I Bodnarchuk; Maksym V Kovalenko; Heiko Groiss; Roland Resel; Michael Reissner; Günter Hesser; Rainer T Lechner; Walter Steiner; Friedrich Schäffler; Wolfgang Heiss Journal: Small Date: 2009-10 Impact factor: 13.281
Authors: Maryna I Bodnarchuk; Maksym V Kovalenko; Stefan Pichler; Gerhard Fritz-Popovski; Günter Hesser; Wolfgang Heiss Journal: ACS Nano Date: 2010-01-26 Impact factor: 15.881
Authors: Nicholas F Chilton; Russell P Anderson; Lincoln D Turner; Alessandro Soncini; Keith S Murray Journal: J Comput Chem Date: 2013-02-05 Impact factor: 3.376
Authors: Kostiantyn Kravchyk; Loredana Protesescu; Maryna I Bodnarchuk; Frank Krumeich; Maksym Yarema; Marc Walter; Christoph Guntlin; Maksym V Kovalenko Journal: J Am Chem Soc Date: 2013-03-08 Impact factor: 15.419
Authors: Lyudmila M Bronstein; Jessie E Atkinson; Andrey G Malyutin; Faiz Kidwai; Barry D Stein; David G Morgan; John M Perry; Jonathan A Karty Journal: Langmuir Date: 2011-02-04 Impact factor: 3.882