David Albinsson1, Sara Nilsson1, Tomasz J Antosiewicz2, Vladimir P Zhdanov1,3, Christoph Langhammer1. 1. Department of Physics, Chalmers University of Technology, 412 96 Göteborg, Sweden. 2. Faculty of Physics, University of Warsaw, Pasteura 5, 02-093 Warsaw, Poland. 3. Boreskov Institute of Catalysis, Russian Academy of Sciences, Novosibirsk 630090, Russia.
Abstract
The ability to study oxidation, reduction, and other chemical transformations of nanoparticles in real time and under realistic conditions is a nontrivial task due to their small dimensions and the often challenging environment in terms of temperature and pressure. For scrutinizing oxidation of metal nanoparticles, visible light optical spectroscopy based on the plasmonic properties of the metal has been established as a suitable method. However, directly relying on the plasmonic resonance of metal nanoparticles as a built-in probe to track oxidation has a number of drawbacks, including the loss of optical contrast in the late oxidation stages. To address these intrinsic limitations, we present a plasmonic heterodimer-based nanospectroscopy approach, which enables continuous self-referencing by using polarized light to eliminate parasitic signals and provides large optical contrast all the way to complete oxidation. Using Au-Cu heterodimers and combining experiments with finite-difference time-domain simulations, we quantitatively analyze the oxidation kinetics of ca. 30 nm sized Cu nanoparticles up to complete oxidation. Taking the Kirkendall effect into account, we extract the corresponding apparent Arrhenius parameters at various extents of oxidation and find that they exhibit a significant compensation effect, implying that changes in the oxidation mechanism occur as oxidation progresses and the structure of the formed oxide evolves. In a wider perspective, our work promotes the use of model-system-type in situ optical plasmonic spectroscopy experiments in combination with electrodynamics simulations to quantitatively analyze and mechanistically interpret oxidation of metal nanoparticles and the corresponding kinetics in demanding chemical environments, such as in heterogeneous catalysis.
The ability to study oxidation, reduction, and other chemical transformations of nanoparticles in real time and under realistic conditions is a nontrivial task due to their small dimensions and the often challenging environment in terms of temperature and pressure. For scrutinizing oxidation of metal nanoparticles, visible light optical spectroscopy based on the plasmonic properties of the metal has been established as a suitable method. However, directly relying on the plasmonic resonance of metal nanoparticles as a built-in probe to track oxidation has a number of drawbacks, including the loss of optical contrast in the late oxidation stages. To address these intrinsic limitations, we present a plasmonic heterodimer-based nanospectroscopy approach, which enables continuous self-referencing by using polarized light to eliminate parasitic signals and provides large optical contrast all the way to complete oxidation. Using Au-Cu heterodimers and combining experiments with finite-difference time-domain simulations, we quantitatively analyze the oxidation kinetics of ca. 30 nm sized Cu nanoparticles up to complete oxidation. Taking the Kirkendall effect into account, we extract the corresponding apparent Arrhenius parameters at various extents of oxidation and find that they exhibit a significant compensation effect, implying that changes in the oxidation mechanism occur as oxidation progresses and the structure of the formed oxide evolves. In a wider perspective, our work promotes the use of model-system-type in situ optical plasmonic spectroscopy experiments in combination with electrodynamics simulations to quantitatively analyze and mechanistically interpret oxidation of metal nanoparticles and the corresponding kinetics in demanding chemical environments, such as in heterogeneous catalysis.
In the presence of
oxygen, metals are susceptible to oxidation.
In particular, macroscopic surfaces are usually covered by a nanometer-sized
“native” oxide layer, preventing complete oxidation,
whereas nanoparticles can easily be converted into the fully oxidized
state. In this field, both experimental and theoretical studies of
oxidation have long been focused on macroscopic samples.[1] More recently, the oxidation of nanoparticles
and nanostructures has also received considerable attention due to
technological relevance for various areas including microelectronics
and heterogeneous catalysis (see, e.g., seminal articles[2−4] and more recent studies[5−10] and references therein). However, irrespective of the length scales
of the samples, the understanding of the mechanistic details governing
oxidation is still limited because it is typically influenced by a
subtle interplay of various factors including (i) the electric field
generated due to the charge located at the interface between the metal
and oxide, (ii) lattice strain arising due to the lattice expansion
during oxide formation, (iii) evolution of the oxide structure e.g.,
via grain growth, (iv) grain boundaries, and (v) generation of voids
in the metal (Kirkendall effect[2,6]) and/or cracks in the
oxide (see, e.g., ref (10) and references therein).Experimentally, the oxidation of
metal nanoparticles has been explored
by a wide range of techniques, including quartz crystal microbalance
(QCM),[11] in situ X-ray diffraction,[3] thermogravimetry (TG),[12,13] UV–vis spectroscopy,[9,14−16] X-ray photoelectron spectroscopy (XPS),[11] and transmission electron microscopy (TEM).[17,18] Despite the apparent abundance of different techniques, the accurate
monitoring of oxidation is still challenging because each of them
has its limitations. For example, techniques relying on high-energy
electrons (TEM, XPS) to probe or image a sample suffer from the need
of low operation pressures and tend to significantly influence the
oxidation process during (beam effects) as well as after imaging (due
to carbon contamination buildup), whereas gravimetric techniques (QCM,
TG) require relatively large samples and lack spatial resolution.
Among the above mentioned approaches, visible light optical spectroscopy,
and plasmonic spectroscopy in particular, is attractive because of
its remote readout compatible with ambient pressures and elevated
temperatures, combined with its generally noninvasive nature due to
the low irradiance of the employed visible photons.In general,
plasmonic spectroscopy relies on measuring the spectral
characteristics of the localized surface plasmon resonance (LSPR)
peak of (typically) metallic nanoparticles and how it responds due
to changes in and around the particle(s). This effect gives rise to
a large and conveniently measurable optical contrast upon oxide formation
because the LSPR frequency changes with the transition from the metallic
state supporting LSPR to a dielectric state that is plasmonically
inactive and thus exhibits a much smaller optical cross section. Nevertheless,
relying entirely on the intrinsic LSPR of the metallic nanoparticles
as a probe of oxidation has a number of drawbacks. First, the essentially
complete loss of well-defined optical contrast in the later stages
of the oxidation process, when most of the metal has been converted
to the oxide phase, makes its study challenging using LSPR. Second,
along the same lines, also the study of small particles is less effective
due to their smaller optical cross sections. Finally, the change in
the LSPR is not only selectively sensitive to the oxidation process
alone but also to other potentially simultaneously occurring effects
like temperature change,[19,20] desorption of species
from the nanoparticle/oxide surface,[21] and
chemical/dielectric changes occurring in the support.[22] To address these limitations, we apply here a plasmonic
heterodimer-based nanospectroscopy approach, which enables continuous
self-referencing by using polarized light to eliminate unwanted signal
contributions and drift,[23] and provides
high optical contrast all the way to complete oxidation.Focusing
on the oxidation of Cu, we note that this process is generic
in the field under consideration and that Cu exhibits excellent plasmonic
properties.[24] Mechanistically, oxidation
is usually considered to be controlled primarily by diffusion of Cu+ toward the oxide–gas interface and partly by diffusion
of O2–-species toward the oxide–metal interface.[1] In macroscopic, polycrystalline samples, with
increasing temperature (from 200 to 700 K), the oxide thickness has
been reported to increase from ∼10 to 1000 nm and the corresponding
kinetics were observed to follow logarithmic, inverse-logarithmic,
cubic, linear, and parabolic laws.[25] In
the case of single-crystal (111), (100), and (110) surfaces, with
increasing temperature from 300 to 450 K, the oxide film thickness
was measured to increase from a few nanometers to ∼100 nm and
the oxide growth was logarithmic for thicknesses under 5 nm and of
the power law type with exponents of 1/3 and 1/2 in the range of 5–25
nm and above 25 nm, respectively.[26] Furthermore,
the available oxidation studies focused on Cu nanoparticles indicate
that they, in analogy with other metals,[2,6,27,28] often exhibit the so-called
nanoscale Kirkendall effect (NKE), as a result of Cu-ions diffusing
faster in the oxide compared with O-ions.[4,9,14,29,30] This results in the formation of a characteristic
hollow oxide shell, with the amount of hollowness depending on the
ratio between the diffusion rates of Cu- and O-ions, as well as on
the oxide structure.In nanoparticles at relatively low temperatures,
in analogy with
bulk systems, preferential formation of Cu2O (over CuO)
is typically observed[9,12,13] and the reported activation energies cover a wide range.[9,12,14] In the corresponding studies,
the measured oxidation kinetics are typically explained by assuming
a single set of Arrhenius parameters and to the best of our knowledge
no one has investigated the correctness of this assumption or quantified
the change of these parameters with increasing extent of oxidation.
Hence, in this study we utilize the plasmonic heterodimer concept
to track the oxidation of ∼30 nm sized Cu nanoparticles all
the way to complete oxidation. We observe NKE from transmission electron
microscope (TEM) images and by combining optical experiments with
finite-difference time-domain (FDTD) simulations, we find that the
Arrhenius parameters for oxidation significantly depend on the extent
of oxidation and exhibit a distinct compensation effect between the
apparent activation energy and the pre-exponential factor.
Methods
Au–Cu
Heterodimer Nanofabrication
To make the
structures, a hole-mask with 100 nm circular holes was prepared.[34] As the first deposition step to grow the heterodimers,
40 nm Au was electron-beam evaporated through the mask at a 2.5°
angle off-normal. As the second step, a 5 nm Al2O3 layer was evaporated through the mask at normal incidence. Then,
to shrink the holes in the mask and to tune the size of the Cu nanoparticles
to be grown in the last step, the sample was tilted by 40° and
100 nm Al2O3 was evaporated while rotating the
sample at 5 rpm. In this way, according to the shrinking-hole colloidal
lithography (SHCL) concept, the evaporated Al2O3 is exclusively deposited on the walls of the mask without being
deposited on the substrate, enabling it to be removed completely in
the final lift-off. In the next step, 20 nm Cu was deposited through
the same holes in the mask (now shrunk to diameters of ca. 30 nm)
at an angle of 8° off-normal and in the opposite direction to
the Au deposition. In the last step, the mask and all other material
layers were removed by lift-off in acetone. All evaporations were
performed at a rate of 2 Å/s and a chamber base pressure of 5 ×
10–7 Torr.
LSPR Measurements in Flow Reactor
Glass samples were
mounted in a temperature-controlled quartz tube flow reactor with
optical access (Insplorion X1, Insplorion AB, Göteborg Sweden),
using Ar as the carrier gas. The gas flow rate was kept constant at
100 mL min–1 and the gas composition was regulated
by mass flow controllers (Bronkhorst ΔP). The sample temperature
was measured by a thermocouple mounted on the sample surface, and
a PID controller (Eurotherm 3216) connected to a power supply was
used to heat a coil surrounding the tube reactor. The sample inside
the flow reactor was illuminated by white light (AvaLight-Hal, Avantes)
through an optical fiber equipped with a collimating lens. To enable
simultaneous probing of the heterodimer with light polarized along
and perpendicular to its long axis, a polarizing beam splitter (Thorlabs
CM1-PBS251) was placed between the sample and two fiber-coupled fixed-grating
spectrometers (AvaSpec-1024, Avantes).
FDTD Simulations
The finite-difference time-domain
(FDTD) simulation, performed using commercial software FDTD Solutions
(Lumerical), was used to evaluate the optical response of the plasmonic
heterodimer structure. The Au sensor element in the dimer was simulated
as a truncated cone (81 nm bottom diameter, 66 nm top diameter, and
42 nm thickness) with rounded corners (r = 20 nm
top and r = 2 nm bottom). The neighboring Cu particle
was simulated as a half sphere with an original radius of 22 nm placed
8 nm from the Au element. The substrate was simulated as SiO2 (refractive index of 1.46) and the surrounding gas as a material
with the refractive index n = 1. The Au dielectric
function was taken from Johnson and Christy,[31] the one for Cu from McPeak et al.,[32] and
the one for Cu2O from Tahir et al.[33] For the various porous Cu cores, the dielectric functions were calculated
using eq S1. To correctly resolve the field
close to the Cu particle, a mesh overlay with a step size of 0.3 nm
was used around it. Light was introduced as a linearly polarized plane
wave via a total-field/scattered-field source, and the scattering
and absorption spectra were obtained in all directions by integrating
the Poynting vector of the field.
Results and Discussion
Au–Cu
Heterodimer Nanostructures
Au–Cu
heterodimer arrays were fabricated on a 1 cm2 glass substrate
using shrinking-hole colloidal lithography (SHCL)[34,35] by growing a ca. 30 × 20 nm2 Cu nanoparticle next
to a larger Au disk nanoantenna (100 × 40 nm2) acting
as the sensor. The gap between the two was defined by a 5 nm thin
Al2O3 layer grown in between the dimer elements
to inhibit alloy formation between Au and Cu during heating (see the Methods section for details). Scanning electron
microscopy (SEM) images of the structures are presented in Figure b together with the
Cu particle size distribution measured from the SEM images (Figure c). Higher resolution
images (Figure c,d)
indicate that initially there are tiny Au particles near the Au nanoantennas,
which then almost completely disappear after heating the sample, most
likely by coalescing with the large nanoantenna.
Figure 1
(a) Polarization-dependent
optical extinction spectra of a heterodimer
array with the Cu nanoparticles in the metallic (solid lines) and
oxidized (dashed lines) states, respectively. The color code indicates
the linear polarization direction with respect to the dimer axis,
as depicted in the inset. Note the essentially identical optical signature
for perpendicular polarization, whereas a spectral blue shift occurs
upon Cu oxidation for the parallel polarization. The inset shows a
schematic depiction of the Au–Cu heterodimer arrangement comprising
a Au nanoantenna sensor adjacent to a much smaller Cu nanoparticle
that is oxidized upon exposure to O2. The red and blue
arrows indicate the simultaneously used perpendicular linear polarization
directions for drift-free optical sensing of the Cu oxidation process
by means of a beam splitter. (b) Top-view and side-view SEM images
of a nanofabricated Au–Cu heterodimer array. (c) Size distribution
of the Cu nanoparticles from SEM image analysis. A total of 169 particles
were analyzed.
Figure 2
(a) Temperature ramps
from 323 to 523 K in different O2 concentrations in Ar
carrier gas, as indicated by the red shaded
areas. The white shaded areas correspond to cooling cycles back to
323 K in 4% H2 in Ar carrier gas to induce reduction of
the Cu nanoparticles. (b) Corresponding LSPR centroid position shift,
Δλcent., of a Au–Cu heterodimer array
for light polarized parallel (Δλ∥) and
perpendicular (Δλ⊥) to the dimer axis,
as well as for the difference between the two (Δλ∥ – Δλ⊥). Note
how the subtraction of the two polarizations effectively eliminates
drift, as well as the temperature-induced optical response of the
dimer. (c, d) SEM images of a representative heterodimer taken before
and after, respectively, the experimental sequence outlined in (a).
(e) Time derivative of the drift-corrected Δλcent. response plotted as a function of temperature. The color code corresponds
to the one in (a) and depicts the O2 concentration in the
feed during the oxidation cycle. While the first oxidation cycle exhibits
a distinctly different response with an oxidation temperature of ca.
423 K (defined as the minimum in the derivative), a very similar oxidation
behavior with oxidation temperature of ca. 383 K is observed for all
other O2 concentration cycles.
(a) Polarization-dependent
optical extinction spectra of a heterodimer
array with the Cu nanoparticles in the metallic (solid lines) and
oxidized (dashed lines) states, respectively. The color code indicates
the linear polarization direction with respect to the dimer axis,
as depicted in the inset. Note the essentially identical optical signature
for perpendicular polarization, whereas a spectral blue shift occurs
upon Cu oxidation for the parallel polarization. The inset shows a
schematic depiction of the Au–Cu heterodimer arrangement comprising
a Au nanoantenna sensor adjacent to a much smaller Cu nanoparticle
that is oxidized upon exposure to O2. The red and blue
arrows indicate the simultaneously used perpendicular linear polarization
directions for drift-free optical sensing of the Cu oxidation process
by means of a beam splitter. (b) Top-view and side-view SEM images
of a nanofabricated Au–Cu heterodimer array. (c) Size distribution
of the Cu nanoparticles from SEM image analysis. A total of 169 particles
were analyzed.(a) Temperature ramps
from 323 to 523 K in different O2 concentrations in Ar
carrier gas, as indicated by the red shaded
areas. The white shaded areas correspond to cooling cycles back to
323 K in 4% H2 in Ar carrier gas to induce reduction of
the Cu nanoparticles. (b) Corresponding LSPR centroid position shift,
Δλcent., of a Au–Cu heterodimer array
for light polarized parallel (Δλ∥) and
perpendicular (Δλ⊥) to the dimer axis,
as well as for the difference between the two (Δλ∥ – Δλ⊥). Note
how the subtraction of the two polarizations effectively eliminates
drift, as well as the temperature-induced optical response of the
dimer. (c, d) SEM images of a representative heterodimer taken before
and after, respectively, the experimental sequence outlined in (a).
(e) Time derivative of the drift-corrected Δλcent. response plotted as a function of temperature. The color code corresponds
to the one in (a) and depicts the O2 concentration in the
feed during the oxidation cycle. While the first oxidation cycle exhibits
a distinctly different response with an oxidation temperature of ca.
423 K (defined as the minimum in the derivative), a very similar oxidation
behavior with oxidation temperature of ca. 383 K is observed for all
other O2 concentration cycles.
Cu Oxidation Experiments
To induce and study the oxidation
of the Cu nanoparticles under controlled conditions, the heterodimer
array samples were mounted in a temperature-controlled quartz tube
flow reactor with optical access. Simultaneous probing of the heterodimers
with light polarized along and perpendicular to its long axis was
enabled by a polarizing beam splitter (Thorlabs CM1-PBS251) that was
placed between the sample and two fiber-coupled fixed-grating spectrometers
(AvaSpec-1024, Avantes). The observed spectral red shift, as well
as the broadening of the LSPR extinction peak for the dimers excited
in parallel polarization is a clear indication of the anticipated
near-field coupling between the dimer elements[36] (Figure a).Upon exposing the sample to 0.2% oxygen at 523 K to induce
Cu nanoparticle oxidation (the Au remains metallic due to its chemical
inertness at these conditions[37]), a significant
spectral blue shift of the LSPR peak becomes apparent for parallel
polarization (blue dashed line in Figure a), whereas the perpendicular polarization
peak remains almost unchanged (red dashed line). This can be understood
as plasmonic coupling when both dimer elements are metallic[38,39] and as diminishing coupling when the Cu element is transformed into
oxide. At the same time, any isotropic changes taking place in the
Au element or in the underlying substrate will be captured in both
polarization directions symmetrically, enabling effective correction
for such unwanted (symmetric) effects by subtraction of the signals
obtained for the two polarization directions.[23]To illustrate this in the present case, we carried out an
experiment
where a heterodimer sample was exposed to seven consecutive heating
ramps from 323 to 523 K at a heating rate of 5 K/min in increasing
O2 concentration (0.2–2%) for each cycle. Ar was
used as the carrier gas, and prior to the first oxidation cycle, the
sample was heated to 576 K in 4% H2 in Ar for 60 min to
reduce any native oxide on the Cu surface, as well as to induce Au
and Cu recrystallization. This is necessary since, directly after
nanofabrication, evaporated nanoparticles exhibit a structure far
from thermodynamic equilibrium.[32,40] After each oxidation
cycle, the sample was reduced in 4% H2 in Ar at 523 K for
60 min while cooling back to room temperature (Figure a,b). The induced LSPR centroid shift for
both polarization directions, Δλcent., was
obtained by fitting a 20° polynomial to the LSPR peak in the
measured optical extinction spectra for the two polarization directions
and then by deriving the spectral position of the peak centroid.[41]In addition to the contribution related
to oxidation of Cu nanoparticles,
the observed LSPR signal may be influenced by other factors. First,
upon heating, we observe a spectral red shift that is proportional
to the temperature change in both polarizations. This is caused by
the intrinsic temperature dependence of the LSPR.[19] Second, there is a parasitic signal stemming most likely
from substrate effects via spill-over of, e.g., H-species to the glass
(SiO2) support,[22] occurring
when the surrounding atmosphere is changed from oxidizing to reducing
at high temperature, as manifested in a distinct and almost immediate
Δλ blue shift upon exposure to H2 for each
cycle at 523 K. Third, we also notice a more long-term and irreversible
drift occurring over the course of the entire experiment, which gradually
red-shifts the LSPR peaks for both polarization directions. These
can be ascribed to slow morphological changes such as recrystallization,
transformation to more Wulff-shape crystals,[42] and Ostwald ripening. By inspecting SEM images taken before and
after exposing a sample to elevated temperatures (Figure c,d, respectively), one can
clearly see a reduction in the number of tiny Au particles surrounding
the Au disk (Ostwald ripening) as well as transformation of the Au
nanoantenna toward a more Wulff-like shape. Predominantly, the changes
take place in the Au nanoantenna, in line with the drift essentially
being the same for both polarization directions.To account
for and eliminate these three undesirable contributions
to the optical signal, we subtracted the perpendicular polarization
trace from the parallel one (Figure b). In this way, we obtain the plasmonic Δλcent. signal stemming from the oxidation/reduction of the Cu
nanoparticle. As the key observations from this analysis, we find
that (i) the long-term drift has been eliminated from the data and
(ii) only a distinct spectral blue shift about one-third into the
temperature ramp is recorded for each oxidation cycle. Furthermore,
the inspection of a heterodimer before and after cycling reveals that
both the Au nanoantenna and Cu nanoparticle are apparently nearly
intact (Figure c,d).To further analyze these data, we plot the first derivative of
the Δλcent. signal versus temperature[23] (Figure e). In this way, we can identify the temperature at which
oxidation occurs for each O2 concentration in the gas feed,
in analogy to traditional temperature-programmed oxidation. This analysis
reveals, apart from the first oxidation cycle, a very similar oxidation
behavior for the screened range of different O2 concentrations.
This indicates that (i) our experimental approach is robust, (ii)
the Cu nanoparticles are insensitive to O2 concentration
in the range of 0.5–2% and, (iii) the very first oxidation
is mechanistically distinct from the subsequent ones, as reveled by
the significantly higher oxidation temperature. As a consequence,
we have excluded the first oxidation cycle from further analysis below.Having established our experimental approach, we now turn to a
second set of experiments combined with extensive FDTD simulations
to investigate in detail and in a quantitative manner the oxidation
process of the Cu nanoparticles. As the first step, we carried out
the controlled oxidation of a sample that had been pretreated with
a full oxidation–reduction cycle at 383 K in 0.5% O2. This temperature is high enough for oxidation to occur at a reasonable
time scale and low enough to predominantly form Cu2O, while
suppressing CuO,[9,12,13] as confirmed by XPS analysis [Figure S2 in the Supporting Information (SI)] and in agreement with previous
studies of Cu nanoparticle oxidation.[14,43] We make the
following initial observations from the experimental data. As oxidation
proceeds, the LSPR peak for parallel polarization blue-shifts and
shoulderlike features appear and evolve on the long-wavelength side
(Figure a). Inspecting
SEM images (Figure b,c) of the same sample together with TEM micrographs obtained before
and after identical oxidation treatment of a sample-analogue fabricated
on a TEM membrane (Figure b,c—insets and Figure S1) reveals the formation of a central Kirkendall void during oxidation
and a corresponding increase of the particle size (Figure S1), in good agreement with earlier observations of
the NKE.[4,9,14,30]
Figure 3
(a) Evolution of the LSPR peak during the oxidation of
the Cu elements
in an array of Au–Cu heterodimers measured at 383 K in 0.5%
O2 in Ar carrier gas in a parallel polarization configuration.
The color code depicts the reaction coordinate between 0 (fully reduced
state) to 1 (fully oxidized state). We note the spectral blue shift
and the appearance of shoulderlike features on the long-wavelength
side of the peak, as oxidation of the Cu element progresses. SEM images
of a representative single dimer in the reduced (b) and fully oxidized
(c) state. The insets show the corresponding TEM images obtained before
and after identical oxidation treatment of a sample-analogue fabricated
on a TEM membrane. They reveal the formation of a central Kirkendall
hole during oxidation. (d–g) Experimentally determined temporal
evolution of the four peak descriptors, that is, (d) peak position
shift, Δλ, (e) peak centroid shift, Δλcent. (f) full-width-at-half-maximum change, ΔFWHM, and
(g) extinction at peak maximum change, ΔExt. The colored lines
indicate the position of the selected spectra shown in (a) along the
reaction coordinate. (h) Extinction spectra for different degrees
of oxidation of the Cu element in a single Au–Cu heterodimer
simulated by FDTD for parallel polarization. The color code depicts
the volumetric oxidation fraction, δ, of the Cu element. We
note the good qualitative agreement with the experimental spectra
in (a). (i) Schematic depiction of the FDTD model used to simulate
the Au–Cu heterodimers. (j) Schematic depiction of and geometric
descriptors used in the NKE-Cu oxidation model for the corresponding
FDTD simulations. (k–n) Same as (d)–(g) but with data
taken from the FDTD simulations and plotted versus the oxidation fraction,
δ.
(a) Evolution of the LSPR peak during the oxidation of
the Cu elements
in an array of Au–Cu heterodimers measured at 383 K in 0.5%
O2 in Ar carrier gas in a parallel polarization configuration.
The color code depicts the reaction coordinate between 0 (fully reduced
state) to 1 (fully oxidized state). We note the spectral blue shift
and the appearance of shoulderlike features on the long-wavelength
side of the peak, as oxidation of the Cu element progresses. SEM images
of a representative single dimer in the reduced (b) and fully oxidized
(c) state. The insets show the corresponding TEM images obtained before
and after identical oxidation treatment of a sample-analogue fabricated
on a TEM membrane. They reveal the formation of a central Kirkendall
hole during oxidation. (d–g) Experimentally determined temporal
evolution of the four peak descriptors, that is, (d) peak position
shift, Δλ, (e) peak centroid shift, Δλcent. (f) full-width-at-half-maximum change, ΔFWHM, and
(g) extinction at peak maximum change, ΔExt. The colored lines
indicate the position of the selected spectra shown in (a) along the
reaction coordinate. (h) Extinction spectra for different degrees
of oxidation of the Cu element in a single Au–Cu heterodimer
simulated by FDTD for parallel polarization. The color code depicts
the volumetric oxidation fraction, δ, of the Cu element. We
note the good qualitative agreement with the experimental spectra
in (a). (i) Schematic depiction of the FDTD model used to simulate
the Au–Cu heterodimers. (j) Schematic depiction of and geometric
descriptors used in the NKE-Cu oxidation model for the corresponding
FDTD simulations. (k–n) Same as (d)–(g) but with data
taken from the FDTD simulations and plotted versus the oxidation fraction,
δ.Turning back to the optical response
induced by the oxide shell
growth and Kirkendall void formation, we tracked four different peak
descriptors as a function of oxidation time, that is, the peak position
Δλ, the centroid position, Δλcent. (according to the definition by Dahlin et al.[41]) the change in peak full width at half-maximum (ΔFWHM),
and the change in extinction value at the peak wavelength (ΔExt)
and all are shown in Figure d–g. The Δλ time trace obtained after subtraction
of the corresponding perpendicular polarization trace nicely reproduces
the blue shift identified from the spectra but also reveals a slight
red shift before and after the blue-shifting period (Figure d). The evolution of the centroid
time trace is similar but exhibits a period of more pronounced spectral
red shift prior to blue-shifting (Figure e). Looking at the time traces of the remaining
two peak descriptors ΔFWHM and ΔExt reveals a significantly
different response, where a distinct maximum or minimum, respectively,
occurs during the second half of the Δλ blue shift period
(Figure f,g).
FDTD-NKE
Model Simulations
The four peak descriptors
introduced above allow us to quantify the optical response to oxidation
of Cu nanoparticles. However, to actually track the kinetics of oxidation,
we need a method to convert these descriptors to the extent of oxidation.
To enable this conversion, we employ electrodynamics simulations of
our structures at different stages of oxidation and extract the same
peak descriptors from the simulated optical response. Specifically,
we utilize the FDTD method due to its capability of simulating the
optical response of an arbitrarily shaped nanostructure, including
the structures of interest to us. In the FDTD model, the heterodimer
structures were represented as a truncated Au cone with rounded corners
located next to a hemispherical Cu particle (Figure i). Specifically, the Cu particles are described
using a conventional hemispherical core–shell model (Figure j; for oxidation
of Cu, this structural model has been successfully used earlier[9,16]). In particular, the Cu2O shell of volume Voxide is assumed to be structurally homogeneous. Due to
the NKE, the core volume Vcore is considered
to contain metal and voids. The net volume of metal (without voids)
and the volume of voids are designated as VCu and Vvoid, respectively. For these volumes,
we have four general balance equationswhere V0 is the
initial volume of the particle, δ is the fraction of Cu atoms
converted into the oxide state, Z = 1.68 is the Pilling–Bedworth
ratio for Cu2O formation,[44] and
θ is the relative extent of the void formation inside the core
compared to its maximum possible value (θ ≤ 1).Physically, θ = 0 corresponds to a situation where only O-ions
diffuse inwards and no internal void is formed, whereas at θ
= θmax = 1, only outward diffusion of Cu-ions occurs
and results in the full-scale formation of Kirkendall voids in the
core. Since in our case, the formation of a central Kirkendall hole
and the corresponding increase in the particle diameter in the oxide
state after complete oxidation are clearly observed, we further focus
on the full NKE and thus set θ = 1. With this condition, eq is reduced to Vcore = V0.The ingredients of the model introduced above are independent of
details describing the void distribution in the core. To account for
variation in the location and distribution of internal voids, we therefore
analyzed a few versions of our FDTD model to clarify the scale of
potential errors related to the uncertainties of the underlying assumptions
(Figures S6 and S7). Here, we describe
the version, which appears most reasonable and present the corresponding
results.To specify the description of voids, we notice that
in our case,
during the initial oxidation phase, a multitude of small voids is
expected to form simultaneously inside the metallic phase. We describe
them by assuming that they form isotopically throughout the metallic
phase and grow in number until a critical concentration is reached
when they coalesce into a larger void or hole in the center of the
nanoparticle. This assumption is reasonable for our particles because
they are rich in defects and grain boundaries, as a consequence of
the growth conditions during Cu evaporation. This heterogeneity then
provides multiple nucleation sites for the initial transient formation
of small voids that at the later oxidation stage coalesce into a single
large Kirkendall hole.[29] The presence of
small voids inside Cu can be described in terms of their integral
volume, Vsv, the integral volume of Cu
and small voids, VCu + Vsv, and the corresponding coefficient of porosity, defined
byBefore the
onset of the formation of a large
Kirkendall hole, we have Vsv = Vvoid = δV0. Substituting this expression and expression into 5 yields β
= δ. In our treatment, we consider that this regime occurs up
to reaching the critical value of β (or δ), i.e., at β
≤ β* = 0.3, and then the porosity remains
constant (this value of β* is physically reasonable
because at smaller β, large voids are usually not observed[9]). For the later stage of oxidation, eq remains applicable
but with β = β*. In particular, it can be rewritten as . Using the latter relation
and considering
that the full volume of pores is δV0 (see eq with θ
= 1), we obtain the expression for the hole volumeAs expected, Vhole = 0 at δ = β* and Vhole = V0 at δ = 1.Our FDTD simulations (Figure h,k–n) were performed for a hemispherical Cu
particle (22 nm in diameter) located next to (8 nm gap) a truncated
Au cone (81 nm bottom diameter, 66 nm top diameter, and 42 nm thickness).
These dimensions are slightly different compared to the experimentally
measured ones. The difference is a consequence of tuning the simulated
spectra to match the resonance wavelength observed experimentally
to compensate for the characteristic stochastic intra-array coupling
present in our experimental system.[45] This
matching is important to ensure that the simulated plasmonic peak
“probes” the spectrally appropriate parts of the dispersive
refractive indices of Cu/Cu2O that are the same as in the
experiment. The dielectric functions of Cu, Cu with voids, and Cu2O are presented in the Methods section
and SI (in particular, we used the Maxwell-Garnett
approximation for Cu with small voids; at β ≤ β* = 0.3, this approximation is considered fairly accurate[46]).With the specification above, in good
agreement with the experiment
(cf. Figure h,a),
an initial spectral red shift, followed by a larger blue shift is
reproduced in the FDTD-simulated spectra, and shoulderlike features
emerge on the long-wavelength side of the peak, indicating that the
oxidation mechanism is captured very well by the model. The more distinct
nature of the long-wavelength features riding on top of the broad
LSPR peak is a consequence of the ensemble averaging in the experiment,
compared to the simulation, which is done for a single nanoparticle.
The obtained response captures all of the key features observed for
the different descriptors (Δλ, Δλcent., ΔFWHM, and ΔExt) (cf. Figure d–g,k–n). We also note that
simulating the same oxidation process with the incident field polarized
perpendicular to the dimer axis results in an essentially constant
optical signature, in agreement with the corresponding experimental
data (Figure S4).To evaluate the
robustness of the results presented above, we also
performed the calculations based on three other slightly different
versions of the model: (i) locating the Kirkendall hole off-center
of the particle to break symmetry (Figure S5), (ii) using the Maxwell-Garnett approximation up to 100% void inclusion
(Figure S6c), and (iii) nucleating the
Kirkendall void at a specific position of the metal–oxide interface
instead of in the center of the nanoparticle (Figure S6a). The corresponding results, presented in Figure S6, indicate that the main trends observed
experimentally in the evolution of the optical response are qualitatively
captured by all of the model versions but that the version introduced
above describes the experimental observations most accurately, corroborating
our choice to rely on it for the further interpretation of the experimentally
measured oxidation kinetics.
Cu Oxidation Kinetics
Having established
our FDTD-NKE
model and benchmarked it with the corresponding experimental data,
we can now apply it to quantify the oxidation process in detail. As
the first step, we utilize the simulations to assign an oxidation
fraction to the experimentally measured temporal evolution of the
LSPR peak descriptors. For this purpose, we carried out an experiment
where we obtained the optical response (using the same four peak descriptors
as above) of a heterodimer sample during eight isothermal oxidation
cycles in 0.5% O2 in Ar, carried out at temperatures ranging
between 363 and 423 K with 10 K increase, using parallel and perpendicular
polarizations (Figure a for experimental sequence and Figure b for a Δλcent. readout
example). After each oxidation cycle, we reduced the particles in
2% H2 in Ar carrier gas at 493 K. The specific oxidation
temperature range was again chosen to favor the formation of Cu2O over CuO.[9,12,13] The long-term drift in the Δλ∥ signal,
observed in Figure b, can be ascribed to minor changes of the structure of the Cu nanoparticles
after each completed oxidation–reduction cycle (e.g., due to
reshaping of the Cu particle), resulting in a gradual blue shift of
the signal.
Figure 4
(a) Schematic depiction of the experimental sequence for the cyclic
isothermal oxidation of Cu nanoparticles in 0.5% O2 (red
shaded areas) in Ar carrier gas, using a different temperature for
each cycle. After each oxidation, the Cu particles are reduced in
2% H2 (gray shaded areas) in Ar carrier gas at 493 K. (b)
Corresponding optical, Δλcent., response for
parallel (Δλ∥) and perpendicular (Δλ⊥) polarizations, as well as the latter subtracted from
the former. For clarity, the subtracted parallel–perpendicular
Δλcent. response is offset by −15 nm.
The areas shaded in color denote the O2 exposure pulses
at different temperatures and the light-gray shaded areas the reduction
cycles in 2% H2.
(a) Schematic depiction of the experimental sequence for the cyclic
isothermal oxidation of Cu nanoparticles in 0.5% O2 (red
shaded areas) in Ar carrier gas, using a different temperature for
each cycle. After each oxidation, the Cu particles are reduced in
2% H2 (gray shaded areas) in Ar carrier gas at 493 K. (b)
Corresponding optical, Δλcent., response for
parallel (Δλ∥) and perpendicular (Δλ⊥) polarizations, as well as the latter subtracted from
the former. For clarity, the subtracted parallel–perpendicular
Δλcent. response is offset by −15 nm.
The areas shaded in color denote the O2 exposure pulses
at different temperatures and the light-gray shaded areas the reduction
cycles in 2% H2.Similarly, extracting the time evolution for all four peak
descriptors
and plotting them together for each oxidation cycle temperature reveals
that extreme points (maxima or minima) occur at different times and
thus oxidation fractions for the different descriptors (Figure a–d). Furthermore, the
extreme points occur at different absolute times for different oxidation
temperatures. In the first step to quantify the oxidation process,
we can thus use the temperature dependence of these extreme points
(presented by symbols in Figure a–d) to analyze the kinetics of the oxidation
process. Specifically, we assume that at each extent of oxidation
the time needed to reach this extent can be represented in Arrhenius
formwhere τ0 and Ea are the apparent Arrhenius parameters
(i.e., pre-exponential
factor and activation energy), R is the gas constant,
and T is the temperature. By plotting ln(τ0) versus 1/T and then applying a linear fit,
we can extract Ea and τ0 from the slope and the intersection with the y-axis,
respectively. The corresponding Arrhenius plots, together with derived
apparent activation energies, Ea, for
Cu oxidation obtained using the different peak descriptors and their
respective used extreme point readouts, are summarized in Figure e–h. The found
values range from 36 to 53.4 kJ/mol, which are at the lower end of
the related range of literature values, which spans from 37 to 144
kJ/mol.[9,14]
Figure 5
Time evolution of the extracted peak descriptors:
(a) peak position
shift, Δλ, (b) centroid shift, Δλcent., (c) change in full-width-at-half-maximum, ΔFWHM, and (d)
change in extinction at peak maximum, ΔExt, during isothermal
oxidation in 0.5% O2 in Ar at seven different temperatures
ranging from 363 to 423 K. The symbols (◊, ×, □,
Δ, +, ∇, o) correspond
to the tracked extreme points in the respective descriptor temporal
evolution, at which characteristic oxidation times (τ) are extracted
for all temperatures. (e–h) Arrhenius plots based on extracted
times (τ) from (a)–(d) together with the derived apparent
activation energies, Ea.
Time evolution of the extracted peak descriptors:
(a) peak position
shift, Δλ, (b) centroid shift, Δλcent., (c) change in full-width-at-half-maximum, ΔFWHM, and (d)
change in extinction at peak maximum, ΔExt, during isothermal
oxidation in 0.5% O2 in Ar at seven different temperatures
ranging from 363 to 423 K. The symbols (◊, ×, □,
Δ, +, ∇, o) correspond
to the tracked extreme points in the respective descriptor temporal
evolution, at which characteristic oxidation times (τ) are extracted
for all temperatures. (e–h) Arrhenius plots based on extracted
times (τ) from (a)–(d) together with the derived apparent
activation energies, Ea.It is now interesting to analyze if Ea for the different peak descriptors depends on the oxidation
fraction
in a systematic way. For this purpose, we plot the obtained apparent
activation energies obtained from the different peak descriptors versus
the oxidation fraction, δ, derived from the FDTD simulations
for δ < 0.4 (symbols ◊, ×, □, Δ,
+ in Figure a). We
find that, to a first approximation, all of the extracted Ea values follow the same trend when plotted
against the oxidation fraction, δ, which has the following implications.
First, it corroborates the robustness of our approach and the interchangeability
of the four peak descriptors. This is an interesting result, in particular
in view of the quite different qualitative temporal evolution of the
respective peak descriptor signal. Second, it demonstrates that the
apparent activation energy is not constant but dynamically changes
as oxidation proceeds. To this end, low activation energies are often
attributed to grain boundary diffusion, whereas higher activation
barriers are explained by Cu ion diffusion through an amorphous Cu2O layer that forms at later oxidation stages and has been
found to eliminate grain boundaries.[47] Consequently,
it is now interesting to further evaluate the evolution of Ea even in the δ > 0.4 regime all the
way
to δ = 1, as enabled by our heterodimer sensing approach. For
this analysis, we employ the ΔExt peak descriptor since it exhibits
the largest optical contrast at the late oxidation stages. By finding
the times at which the ΔExt peak descriptor reaches certain
values (Figure S7), the kinetics of oxidation
can be extracted (Figure b). From this, we perform the same Arrhenius analysis as outlined
above (Figure S8), and as the main result,
we find that the apparent activation energy exhibits a sizable gradual
increase, whereas the pre-exponential factor significantly drops as
the oxidation progresses toward completion at δ = 1 (Figure a). In other words,
we observe a significant compensation effect.
Figure 6
Kinetics of Cu oxidation.
(a) Arrhenius parameters Ea and ln(τ0) for oxidation of the Cu
nanoparticles plotted as a function of oxidation fraction, δ,
derived from FDTD simulations. The open circles correspond to data
points extracted by using the ΔExt peak descriptor (see Figure S8 for the corresponding Arrhenius plots)
and the shaded areas depict the corresponding 95% confidence bounds
of the Arrhenius fit. The additional symbols (◊, ×, □,
Δ, +) correspond to the Ea values
derived and presented in Figure e–h using the other three peak descriptors.
(b) Oxidation fraction, δ, as a function of time for the different
considered temperatures.
Kinetics of Cu oxidation.
(a) Arrhenius parameters Ea and ln(τ0) for oxidation of the Cu
nanoparticles plotted as a function of oxidation fraction, δ,
derived from FDTD simulations. The open circles correspond to data
points extracted by using the ΔExt peak descriptor (see Figure S8 for the corresponding Arrhenius plots)
and the shaded areas depict the corresponding 95% confidence bounds
of the Arrhenius fit. The additional symbols (◊, ×, □,
Δ, +) correspond to the Ea values
derived and presented in Figure e–h using the other three peak descriptors.
(b) Oxidation fraction, δ, as a function of time for the different
considered temperatures.To illustrate the extent of compensation, we show τ
as a
function of δ at the average temperature ⟨T⟩ = 393 K (Figure a) and the normalized change of the apparent activation energies
together with the corresponding normalized pre-exponential factors
also as a function of δ (Figure b). The observed compensation between the two Arrhenius
parameters can mathematically be expressed aswhere k and m are constants (inset
of Figure b). In our case, m ≃ −0.26 (kJ/mol)−1 which is comparable to , indicating that the extent of compensation
is significant.
Figure 7
Kinetic parameters for Cu oxidation. (a) Characteristic
times (τ)
at different levels of oxidation, δ, extracted at the average
experimental temperature ⟨T⟩ = 393
K. (b) Normalized change in activation energy, Ea – ⟨Ea⟩ (where
⟨Ea⟩ is the value of Ea at δ = 0.5), and logarithm of the pre-exponential
factors, , as a function of δ.
The inset shows
ln(τ0) as a function of Ea to illustrate the linear relationship between the Arrhenius parameters
[eq with m ≃ −0.26 1/(kJ/mol)].
Kinetic parameters for Cu oxidation. (a) Characteristic
times (τ)
at different levels of oxidation, δ, extracted at the average
experimental temperature ⟨T⟩ = 393
K. (b) Normalized change in activation energy, Ea – ⟨Ea⟩ (where
⟨Ea⟩ is the value of Ea at δ = 0.5), and logarithm of the pre-exponential
factors, , as a function of δ.
The inset shows
ln(τ0) as a function of Ea to illustrate the linear relationship between the Arrhenius parameters
[eq with m ≃ −0.26 1/(kJ/mol)].To articulate the difference between what we observe and
what one
might expect to see on the basis of conventional models of oxidation,
we consider the simplest core–shell model of oxidation with
diffusion of metal ions through the oxide shell and void formation
in the core. In such a case, the growth of the oxide layer thickness
can be described as , where D is the diffusion
coefficient, l is the oxide layer thickness, and A is a constant. The extent of oxidation, δ, can be
considered approximately proportional to l, and thus
the time corresponding to a given δ is given bywhere Ed is the
activation energy for diffusion. In this case, the activation energy
for oxidation is independent of δ and coincides with Ed, whereas τ0 increases with
increasing δ as τ0 ∝ δ2, which is the opposite of what we observe. Thus, the kinetics we
experimentally measure indicate a different and most likely more complex
oxidation mechanism.Historically, this type of compensation
effect has been observed
most prominently in heterogeneous catalysis at the level of complex
reactions[48−50] and also at the level of the dependence of the Arrhenius
parameters of elementary reaction steps on coverage.[51] Usually, this effect is attributed to a change of the reaction
mechanism with increasing temperature or to systematic errors in measurements
and/or interpretation[52] (the latter might
be the case if the interpretation includes a specific kinetic model
which does not correspond to reality). In our case, the systematic
errors might be related to the FDTD-NKE model simulations. The scale
of this error is, however, only about ±5 kJ/mol, as estimated
by using different versions of our model (see the corresponding section
in the SI and Figure S7), and it is small
compared to the observed amount of compensation. Hence, it does not
influence our conclusion and a change of the reaction mechanism with
increasing oxidation fraction appears to be the more likely cause
of the observed change in apparent Arrhenius parameters. For example,
at low extents of oxidation, the oxide layer is thin and oxidation
can occur via the Cabrera–Mott mechanism, where strong electric
fields at the metal–oxide interface can reduce the measured
activation energy. Additionally, the low Ea at the early oxidation stage can be a result of many small, disordered
grains forming in the oxide as a consequence of the local oxide phase
nucleation process on the surface of the metal. As the oxidation progresses,
the size of the oxide grains near the metal–oxide interface
increases due to recrystallization, and as a consequence, the effective
activation energy for diffusion jumps also increases since low energy
diffusion sites at grain boundaries become less abundant, giving rise
to the experimentally observed increase in the activation energy.The explanation of the decrease of τ0 with oxidation
extent is less obvious. One of the physically reasonable conjectures
here is that this is also related to the grain growth upon progression
of oxidation. As already noted, the grains near the oxide–metal
interface are expected to be small and highly disordered in the beginning,
as a consequence of oxide phase nucleation. Under such conditions,
the activation energy for diffusion steps near this interface is distributed
over a wide range, and the apparent activation for oxidation is determined
by the diffusion steps with the lowest activation energy. The absolute
number of available pathways for such steps is, however, low, and
accordingly τ0 is large in this case. With increasing
extent of oxidation, the grains formed near the oxide–metal
interface grow, the distribution of the activation energy of diffusion
steps narrows, the number of accessible pathways for the steps determining
the oxidation rate becomes high, and accordingly τ0 is smaller in this case, explaining the corresponding trend found
in our experiments, as well as the compensation effect of the Arrhenius
parameters.
Conclusions
In summary, we have
presented a method to experimentally investigate
metal nanoparticle oxidation in situ by means of plasmonic optical
spectroscopy. It employs a plasmonic heterodimer nanoarchitecture,
which enables continuous self-referencing using polarized light to
eliminate parasitic signals and to provide large optical contrast
all the way to complete oxidation. Using this approach in combination
with detailed FDTD electrodynamics simulations explicitly taking into
account the Kirkendall void formation observed by ex situ TEM analysis,
we have been able to quantitatively analyze the oxidation kinetics
of ca. 30 nm sized Cu nanoparticles all the way to complete oxidation.
We found a distinct dependence of the corresponding Arrhenius parameters
(Ea and τ0) on the extent
of oxidation with, as the general trend, increasing apparent activation
energy Ea for progressing oxidation, and
for the initial oxidation stages, absolute values in good agreement
with the available literature. Additionally, we observed a significant
kinetic compensation effect where the pre-exponential factor (τ0) decreases as the apparent activation energy (Ea) increases during progressing oxidation. We attribute
these sizable changes in the Arrhenius parameters to changes in the
oxidation mechanism mainly dictated by the evolution of the grain
structure in the growing oxide, emphasizing the complex nature of
oxidation processes in nanoparticles. In a wider perspective, our
work demonstrates the usefulness of combining experiments, based on
nanoarchitectures tailored for in situ optical plasmonic spectroscopy,
with mechanistic FDTD electrodynamics simulations, as a tool to quantitatively
analyze and mechanistically interpret oxidation processes of metal
nanoparticles and the corresponding kinetics. Hence, it also opens
the door to noninvasive in situ investigations of metal nanoparticle
oxidation during, for example, a catalytic reaction or in a corrosive
environment.