In the work presented here, we prepared Ga-substituted NZTO (Na2-xZn2-xGaxTeO6, x = 0.00, 0.05, 0.10, 0.15, 0.20) layered materials with a soft chemical, citric acid-based synthesis method and characterized these by means of X-ray diffraction (XRD), 23Na and 125Te NMR, and by density functional theory (DFT) modeling. The influence of randomly distributed Ga cations on the 125Te NMR spectra confirms the successful synthesis. With DFT-based linear response computations, we show that the local distribution of Na ions in the two neighboring interlayers influences the 125Te chemical shift, consistent with observations. DFT modeling suggests that some of the Na sites are rarely occupied in pure NZTO but become favorable upon Ga substitution. There are clear indications that Ga substitution gives an uneven distribution of Na ions in neighboring interlayers and that the Na structure in one layer affects the adjacent layers.
In the work presented here, we prepared Ga-substituted NZTO (Na2-xZn2-xGaxTeO6, x = 0.00, 0.05, 0.10, 0.15, 0.20) layered materials with a soft chemical, citric acid-based synthesis method and characterized these by means of X-ray diffraction (XRD), 23Na and 125Te NMR, and by density functional theory (DFT) modeling. The influence of randomly distributed Ga cations on the 125Te NMR spectra confirms the successful synthesis. With DFT-based linear response computations, we show that the local distribution of Na ions in the two neighboring interlayers influences the 125Te chemical shift, consistent with observations. DFT modeling suggests that some of the Na sites are rarely occupied in pure NZTO but become favorable upon Ga substitution. There are clear indications that Ga substitution gives an uneven distribution of Na ions in neighboring interlayers and that the Na structure in one layer affects the adjacent layers.
Layered oxide materials
have been of interest for use in battery
technology since the introduction of LiCoO2 (LCO) as an early cathode material.[1] While Li-ion batteries are currently dominating, Na-based
technology is an interesting candidate for certain applications. This
can be attributed to Na’s greater global distribution[2] and the negligible weight difference in the larger
picture of all battery components. Layered oxides may exhibit a negligible
electronic conductivity while still having good ionic conductivity
and may thus be candidates as solid-state electrolytes (SSEs). SSEs
would replace the organic liquid electrolyte, which is highly flammable
and can emit toxic gases in the case of fires,[3] in addition to unwanted reactions with the electrodes.[4] SSE materials should exhibit high ionic conductivity,
low electron conductivity, and good stability[5] and can be amorphous, polymeric or crystalline-like NASICON-types,
certain sulfides, or Na-β-alumina.[6]A structural classification for AMO2 layered oxides was proposed by Delmas
et al., with A being an alkali cation and one or
several cations M located within (MO2) layers of edge-sharing octahedra.[7] Depending on the stacking of the MO2 layers, the intercalated
alkali ion may take octahedral (O) or prismatic (P) coordination.
Furthermore, a number in combination with O or P refers to the number
of distinct (MO2) layers in
the stacking sequence, with two prominent stacking variants being
the O3- and P2-types. An interesting family of quaternary layered
oxides Na2M2TeO6 (M = Ni, Co, Zn,
and Mg) was first described by Evstigneeva et al. in 2007[8] and further characterized by Berthelot et al.[9] These P2-type materials have 12 possible Na positions
available in face-sharing trigonal prisms in each unit cell, although
on average only four of them are filled with Na ions. The distance
between adjacent Na sites is 1.7 Å, which is too short for the
simultaneous occupation of Na ions. The M = Co, Ni members of Na2M2TeO6 are redox-active and are relevant
as cathode materials,[10] whereas M = Zn[11] and Mg[12] are candidates
for solid-state electrolytes. The focus of our work has been on the
Zn variant Na2Zn2TeO6 (NZTO) shown
in Figure , which
is in the space group P6322 and has an
alternating arrangement of the Te atoms across consecutive layers.[8]
Figure 1
(a) Perspective view of the P2-type NZTO structure and
space group P6322. Coordination polyhedra
of Te, Zn, and
Na are shown (bottom). (b) Crystallographic Na positions, labeled
as Wyckoff a-, f-, and g-sites. Note, on average, four out of 12 Na positions per unit cell
are filled, and two adjacent sites cannot be simultaneously occupied
due to distance constraints.
(a) Perspective view of the P2-type NZTO structure and
space group P6322. Coordination polyhedra
of Te, Zn, and
Na are shown (bottom). (b) Crystallographic Na positions, labeled
as Wyckoff a-, f-, and g-sites. Note, on average, four out of 12 Na positions per unit cell
are filled, and two adjacent sites cannot be simultaneously occupied
due to distance constraints.This structure has three different crystallographic
Na sites, with
a multiplicity of three, two, and one in the interlayer gallery and
below and above the layers of octahedrally coordinated Zn/Te. Hence,
the central atoms of the octahedra have several possible local configurations
with respect to the surrounding Na cations residing in the neighboring
interlayers.The three different Na prisms are differentiated
by their coordination
to the framework octahedra. A prism can either be positioned between
two octahedra, where it will face-share its two ends with the octahedra
on each side, or in the tetrahedral voids between the octahedra, where
it is edge-sharing with the surrounding octahedra. The latter of these
is the g-site, but the former is further differentiated
by the cations in the framework layer: The a-site
has a Zn octahedra on each side, and the f-site has
one Zn octahedra on one side and one Te on the other. These sites
are labeled using the symbols from the Wyckoff sites but omit the
multiplicity. Any number in combination with a, f, and g denotes the number of filled sites instead,
in line with our previous work on NZTO.[11,13]Na2Zn2TeO6 shows Na conductivity,
and by impedance spectroscopy, it has been reported to be 6.29 ×
10–4 S cm–1. By introducing Ga
at Zn sites, an increased conductivity of up to 1.1 × 10–3 S cm–1 has been reported.[14] This substitution is reported to reduce the
grain boundary resistance;[15] however, Sau
and Kumar et al. report that the main effect is decreased Na–Na
repulsion due to the increased Na vacancy concentration.[16−18] Karna et al. observed indications for Na ordering in a similar layered
Na2Ni2TeO6 based on Fourier maps
of synchrotron X-ray and neutron diffraction data.[19] On the other hand, ab initio molecular
dynamics studies of NZTO supported a disordered Na distribution.[13]Solid-state synthesis is the most common
synthesis method for the
abovementioned layered oxides.[9,11,20−22] This methodology is based on diffusion between and
inside reactant/product grains, which makes the homogeneous substitution
of elements in low concentrations challenging, as shown in previous
reports, which indicate that the amount of unknown secondary phases
increases with Ga substitution.[23] The synthesis
reaction pathway for the similar NaxCoO2 material
is complex and depends on several factors and was reported by Bianchini
et al. as an interplay between thermodynamically stable phases and
nonequilibrium kinetic phases, with a multistage, compositionally
unrestrained reaction pathway.[20] To ensure
homogeneous substitution, wet chemical sol–gel methods are
preferable as they shorten the diffusion paths and mix easily to form
a homogeneous distribution of precursors.In this article, we
present a detailed experimental and computational
study of Ga-substituted NZTO materials. The motivation behind the
work has been to investigate an alternative synthesis route, ensuring
homogeneous substitution, combined with a characterization method
for verification of the nominal substitution, which must also ensure
that no regions are unsubstituted. We have applied the citric acid
method, where all cations are presumably mixed at the atomic scale
in the form of complexes and precipitated in a homogeneous gel during
heat treatment. The substitution of Ga3+ for Zn2+, leading to Na2–Zn2–GaTeO6, modifies
the sodium content in the interlayer galleries and may, in turn, affect
the local Na substructure, within and between neighboring two-dimensional
(2D) intergalleries, thereby impacting the environment of Zn/Ga and
Te cations. Special attention is therefore given to Ga’s effect
on the average and local structure. For this, 23Na and 125Te magic angle spinning (MAS) solid-state NMR spectroscopy
was applied to obtain information on the local environment of Na and
Te and changes induced by Ga substitution. The energetics of different
interlayer Na configurations has been determined from structural optimization
calculations using density functional theory (DFT). Furthermore, DFT
linear response calculations of NMR chemical shifts are used to help
analyze and interpret NMR spectra. The results obtained on the basis
of high-quality samples made by the sol–gel method are discussed
in relation to the existing literature on NZTO and related 2D materials.
Materials and Methods
Synthesis
Samples of Na2–Zn2–GaTeO6 with x = 0.00, 0.05,
0.10, 0.15, and 0.20 were synthesized using sol–gel synthesis.
All precursors were added in relevant stoichiometric ratio, with the
exception of Na2CO3, which was added in 10%
excess to compensate for evaporation. The reactants ZnO (Sigma-Aldrich,
99.99%), Na2CO3 (Sigma-Aldrich, >99.5%),
and
TeO2 (Sigma-Aldrich, 99.995%) were dissolved by adding
nitric acid (Sigma-Aldrich, 65%) using a magnetic stirrer on a hot
plate at 50 °C until the solution became transparent. Subsequently,
Ga(NO3)3·xH2O (Sigma-Aldrich, 99.9%) was dissolved in water and added. The level
of hydration of the Ga-precursor was determined from thermogravimetric
analysis (TGA). Finally, citric acid (Sigma-Aldrich, 99.5%) was added
in a ratio of 5:1 with respect to the cations in the precursors.The solution was heated to 180 °C while stirring to allow NO gas to evaporate, and after gel formation,
the beaker was left overnight at 180 °C. The resulting powder
was then heated to 450 °C for 12 h. The powder was ball-milled
at 600 rpm for 20 min and pressed into pellets prior to final sintering
reactions. The samples with x = 0–0.10 were
sintered at 900 °C, while x = 0.15 and 0.20
at 800 °C, both using a heating/cooling rate of 5 °C. The
top and bottom of the pellet were covered with the parent powder before
sintering.
X-ray Diffraction (XRD)
Powder X-ray
diffraction (XRD) data were measured on a Bruker D8-A25 diffractometer,
using a Cu Kα1 radiation source and a Ge(111) Johansson
monochromator and a Lynxeye detector. Data were collected for the
2θ range between 10 and 128°, using a step size of 0.005°,
and samples were packed in a capillary for reducing preferred orientation.
Rietveld refinement against the collected data was performed using
Topas v6,[24] and the background was fitted
with a 10-term Chebychev polynomial.
Nuclear Magnetic Resonance (NMR) Spectroscopy
23Na (I = 3/2) and 125Te
(I = 1/2) MAS NMR single transient spectra were collected
at 11.74 T with a Bruker Avance AV III spectrometer using a 4 mm double-channel
probe head at 295 K and at a MAS frequency of 10 kHz. The applied 23Na resonance frequency was 132.29 MHz, and 400 free induction
decays (FIDs) after short pulses were accumulated for each spectrum.
For the 23Na experiments, we used 1.5 μs excitation
pulses at an RF-field of 33 kHz, calibrated using a 1 M NaCl(aq) solution.
For 23Na, we measured, using the saturation recovery method,
a T1 relaxation time constant of ca. 500
μs, and the recycle delay was set to 0.5 s. The applied 125Te resonance frequency was 157.79 MHz, and 2000 FIDs (NS)
were accumulated for each spectrum using 90° pulses calibrated
using a 1 M Te(OH)6 (aq) solution. Tests with variable
recycle delays showed that the maximum intensity in the 125Te spectra were reached using a recycle delay of about 25 s. In addition,
we measured with the saturation recovery method a T1 relaxation time constant of ca. 7 s for 125Te, and the recycle delay was set to 30 s. There were no observable
differences between the various 125Te components in the
spectra regarding relaxation rates.The samples have been mainly
stored in an Ar/desiccator after preparation/XRD analyses but have
been some time in air since we have not worked in a completely inert
atmosphere. 1H NMR was carried out to check hydroxyl groups
and water level, and the samples showed a small broad peak that can
be attributed to water that is slightly above the probe background
level. The amount of hydroxyl groups was also only slightly above
background levels. 23Na experiments with high-power proton
decoupling gave identical spectra as those without decoupling. Hence,
based on these data, we anticipate very small effects of water/OH
groups on the samples, both in regard to structure, ion dynamics,
and relaxation times. We also note that studies of water’s
effect on similar materials show that the interlayer distance (c-axis) should increase with the intercalation of water.[25,26] We do not see any sign of this in our XRD data, and hence we are
confident that the water present is not of significance. Based on
these points, we have decided not to work in a completely inert atmosphere
with our materials.The magnetic field was adjusted by setting
the high-frequency peak
of Adamantane to 38.48 ppm. In addition to the references 1 M NaCl
(aq) for 23Na and Te(OH)6 (aq) for 125Te spectra, TeO2 (s) was used for comparison with chemical
shifts calculated from DFT (vide infra). The shift
values for aqueous 23Na and 125Te are set to
0 ppm. Before Fourier transform of the averaged FIDs, zero filling
and apodization were applied to improve the line shape definitions
and signal-to-noise ratio. The apodization was done by multiplying
the FIDs with a decaying exponential window function with a processing
line broadening (LB) factor of 250 Hz (23Na) and 50 Hz
(125Te).All NMR spectra were adjusted by proper
signal phasing and baseline
corrections. Curve fitting was performed using DMfit.[27]
Density Functional Theory Modeling
The DFT calculations were performed using the Vienna Ab initio Simulation
package (VASP, version 5.4.4).[28−31] The simulations build upon results and configurations
obtained in our previous work[13] and can
be divided into two categories: (i) accurate calculations on a relatively
small system to compute the Te chemical shift from linear response
theory and (ii) AIMD simulations to compute the structural properties
under Ga substitution. Structural optimization calculations were carried
out to obtain reliable starting configurations compatible with the
simulation parameters. All computations make use of the conjugate
gradient algorithm.The chemical shift for Te was evaluated
by means of linear response theory using the method developed by Yates,
Pickard, and Mauri.[32,33] The shift was computed with respect
to TeO2, which was then referenced back to Te(OH)6. Exchange and correlation were treated using the strongly constrained
and appropriately normed (SCAN) semilocal density functional.[34] The projector augmented wave (PAW) method was
used to model core states. Additional technical details can be found
in Section S1 in the Supporting Information
(SI).The Ga-substituted systems were modeled using a supercell
structure
of the configuration reported as the most stable in our previous work.[13] A 3 × 2 × 1 supercell system (16.03
× 18.48 × 11.37 Å3) of said configuration
was constructed, large enough to render the interactions between point
defects and their periodic images negligible and to perform molecular
dynamics simulation. The system contains 24 formula units (264 atoms).The AIMD calculations were performed on the supercell model of
the original NZTO structure and the two most stable substituted configurations.
The stoichiometry of the systems is Na48Zn48Te24O144, Na46Zn46Ga2O144, and Na44Zn44Ga4O144. For brevity, the Ga-substituted systems are
labeled as 2Ga and 4Ga, respectively. All AIMD simulations used a
calculation setup similar to the one chosen to construct the initial
configurations, with some minor modifications, as reported in Section S1.AIMD simulations were performed
both within the canonical (NVT)
and the microcanonical (NVE) ensemble: the former for thermalization
of the system and the latter for production. In both cases, we used
the same parameters described in Section S1. Calculations within the canonical ensemble were modeled using the
Nosé thermostat for controlling temperature oscillations.[35−37] The Nosé mass parameter was set so that the period associated
with these fluctuations was 40 fs. A time-step of 1 fs was found to
be sufficiently small to avoid sudden jumps in the total energy of
the system during the simulation. This setting was used to thermalize
the system using the procedure described in Section S1.Production calculations, performed in the microcanonical
ensemble,
compute 50 ps of dynamics. The analysis of the trajectories relies
on three packages: MDANSE,[38] the atomic
simulation environment (ASE),[39,40] and quippy, the python
interface of QUIP.[41] Additional software
used in this work includes VESTA[42] for
the rendering of ball-and-stick and coordination polyhedra.We would like to make some comments on the choice of methods when
it comes to calculating 125Te NMR parameters from first-principles.
Garaga et al. computed chemical shielding of various forms of TeO2[43] using the methodology developed
by Yates, Pickard, and Mauri.[32,33] This work shows that
meaningful results can be obtained already at the generalized gradient
approximations (GGA) level using the Perdew–Burke–Ernzerhof
(PBE) functional. Lizion et al. computed the NMR shift of Ge—Te
structures including vacancies.[44] As the
large size of the systems considered and the presence of crystal defects
render first-principles calculations particularly challenging, the
authors opted for the Virtual Crystal Approximation, a less-demanding
approach neglecting the distortion of the lattice due to vacancies
and only considering one average site for the entire structure. Albeit
not accurate, this approach allowed the identification of a large
number of vacancies, which is correlated with higher chemical shift
values. Furthermore, Alkan et al. showed that for 125Te,
it is important to include relativistic effects.[45] They used cluster models and showed that methods that included
relativistic corrections had to be applied for accurately modeling
the magnetic-shielding principal components of 125Te in
a range of different compounds. This work also offers a comparison
between results from different functionals, showing that, while hybrid
functionals are required to obtain accurate results, GGA-level functionals
do provide satisfactory results. Since Alkan et al. studied a range
of different compounds and bonding types around Te, it was important
to adopt methods that captured the essential parts of electronic structure
and energies and magnetic and relativistic effects for heavy nuclei.
However, in our case, we investigate very similar compounds and compare
configurations that are quite similar both in structure and properties;
hence, cancellation of errors is expected to occur. Even with the
Ga incorporation, the closest Te surroundings are quite similar and
only modulated slightly by the Na ions, and as long as we have found
a functional that gives parameters close to experimental findings,
other complicating effects will typically be canceled when making
comparisons.
Results and Discussion
Crystal Structure
The diffraction
data of Na2–Zn2–GaTeO6 are
well described in the space group P6322,
which is consistent with other experiments.[11,14,15,22] Diffractograms
are shown in Figure a, with a more detailed Rietveld fit in Figure S1a and information in Table S1.
The variation in unit cell dimensions with composition is shown in Figure b. Atomic coordinates
and derived average bond lengths are listed in Tables S3, S4, respectively.
Figure 2
(a) Observed and calculated (Rietveld
refinement) X-ray diffractograms
of Na2–Zn2–GaTeO6, with
increasing Ga concentration x; wavelength λ
= 1.54 Å. (b) Variation in lattice parameters; space group P6322. Error bars are calculated as standard
error.
(a) Observed and calculated (Rietveld
refinement) X-ray diffractograms
of Na2–Zn2–GaTeO6, with
increasing Ga concentration x; wavelength λ
= 1.54 Å. (b) Variation in lattice parameters; space group P6322. Error bars are calculated as standard
error.The SEM image of NZTO particles in Figure S2 shows that the material crystallizes
as 1–2 μm thick
platelets of some 2–5 μm in lateral size and with well-developed
facets. This could give preferred orientation effects, even in the
capillary setup. If the crystallites have an anisotropy similar to
the particles, anisotropic size broadening could be expected, and
adding this to the refinement improves the fit of the intensities.
However, as shown in Table S2, either preferred
orientation or anisotropic size broadening provided very low improvement
in the Rwp. This will be further explored
in later work.The elevated background in the 2θ range
16–24°,
as shown in an inset in Figure S1b, has
previously been ascribed to stacking faults.[32] The two additional weak peaks indicated with blue arrows as x = 0.00 were earlier explained by the presence of an O’3
impurity,[22] which, however, is unlikely
for our samples owing to the lack of a shoulder/peak at 2θ =
16°. There is a small, unexplained peak at around 35° for
all of the samples, which is tentatively ascribed to the Na substructure.[11,46] A small ZnO impurity is fitted for sample x = 0.00
and may be 0.05, as shown in Figure S1c, but decreases for higher x-contents and is not
visible in the patterns for x = 0.10, 0.15, and 0.20.On increasing Ga substitution at the Zn site, the c-axis expands slightly. This may have different causes: cation repulsions
due to higher charged gallium and O–O repulsion due to fewer
Na cations or weaker Na–O bonding. The ab-plane
contracts, leading to a decrease in the unit cell volume. The average
bond lengths from the structure and the bond lengths from the DFT
calculations described in Section are listed in Table S4.
In the average structure, the octahedral O-distances increase upon
Ga insertion, but the DFT calculations confirm only the increase in
the O–O distance in the Zn octahedra and show that prismatic
O–O distances also increase instead of the expected decrease
in the average model.The x = 0.15 sample appears
to have an anomalously
short c-axis, with c and possibly a deviating from an otherwise clear trend. Repeated synthesis
and analysis confirmed this result. As discussed in Section , we could confirm that
the actual Ga/Zn ratio corresponds well to the nominal composition.
This suggests that the reason for the anomaly might be rooted in the
Na distribution, which has been reported to influence the interlayer
distance.[47] As discussed in Section , modeling reveals
a preference for inhomogeneous Na distribution across the layers at
high Ga substitution levels. Ga distribution was found to be homogeneous
(vide infra), suggesting that the Na distribution
alternates between layers to uphold charge neutrality. A series of
different Na fillings, and therefore different layer distances, could
sum up to different averages depending on the degree of filling and
the filling/stacking sequence.The previously reported Na site
occupancies for NZTO vary considerably,
especially with respect to the f/g ratio.[8,13,22] The currently
adopted site distribution is given in Table S3. Attempts to further refine the Na occupancies give no significant
improvement in Rwp, which probably reflects
disorder, mobility, and weak scattering contrast. Note that the actual
Ga distribution on Zn sites cannot be determined by XRD due to the
low contrast between these neighboring elements in the periodic table,
and hence nominal values are reported. To clarify aspects related
to local ordering and the effect of Ga substitution, a series of NMR
studies were conducted (see below).
23Na NMR Study
The 23Na MAS NMR spectra of the studied samples are shown in Figure . Curve fitting and
superimposed spectra are shown in Section S3. Ideally, the sodium a-, f-, and g-sites with slightly different coordination environments
should show up as closely positioned peaks, and one would expect that
the prismatic coordination of Na should give an asymmetric environment
with an appreciable electric field gradient (EFG) and hence peaks
with typical second-order quadrupolar shape. However, the main peaks
are quite similar for all samples (peak FWHM ∼ 2.3 kHz), and
there are no signs in the line shape of strong quadrupolar couplings.
With increasing Ga content, there is a slight shift of peaks to higher
ppm values, and the small peaks around 45 ppm decrease and finally
disappear. A small shift to higher frequencies may be due to a slight
decrease in quadrupolar couplings; however, the low-frequency side
(right side) does not change with increasing Ga content. The lack
of observed features is interesting and may originate from several
phenomena. Atomic disorder around the Na sites will result in a distribution
of the chemical environments; however, distributions of quadrupolar
couplings and/or chemical shifts will lead to an asymmetric peak shape
with a tailing toward lower frequencies, which is not very obvious
in our spectra.[48] However, since NZTO and
its Ga-substituted derivatives show Na ionic conductivity (vide supra),[14] the lack of peak
shape features could also indicate an exchange of Na cations at rates
comparable to, or larger, than the spectral peak widths one would
observe for a situation with completely rigid and static Na ions.
Increasingly faster jump rates between various sites of prismatic
coordination will average the quadrupolar couplings and chemical shift
differences until a single peak is observed. To observe such a development,
one would have to carry out variable temperature experiments cooling
down to such a low temperature that Na ion dynamics were absent and
compare with experiments at higher temperatures. The apparent symmetry
of the main peak in the stacked plot (Figure ), is slightly misleading. Fitting shows
that the peak cannot be decomposed into one Gaussian/Lorentzian peak
for any sample, and hence residual quadrupolar couplings likely remain.
For layered NaxCoO2, Carlier et al. found that
the 23Na signal was not fully averaged at room temperature
and could only be fitted as one single peak first at 475 K.[47]
Figure 3
23Na NMR signals recorded for Na2–Zn2–GaTeO6. A peak of unknown origin is
indicated with ▼. Spinning sidebands are denoted with *.
23Na NMR signals recorded for Na2–Zn2–GaTeO6. A peak of unknown origin is
indicated with ▼. Spinning sidebands are denoted with *.With increased Ga substitution, the peaks at 45
ppm disappear.
Since they are located at higher frequencies than the main peak, they
probably originate from Na at a lower coordination as this is typical
for 27Al and also indicated for 23Na.[48,49] The peaks around 45 ppm could be intrinsic to NZTO or due to a secondary
phase. From tabulated values of chemical shift values for Na compounds,
no obvious feature appears to explain the peaks.[49] However, upon heating to 200 °C (addressed in another
work to be published), the peak at 45 ppm disappears and the main
peak shifts slightly to the left. However, the peak reappears upon
cooling, suggesting some dynamic effects that exclude a secondary
phase.The integral of the 45 ppm peaks corresponds to about
3% of the
total peak areas for pure NZTO. Hence, it is unlikely that the peak
is due to the Na situated at a grain boundary, interface, or surface.
In these cases, a high surface-to-volume ratio is necessary; however,
this is not supported by any broadening of XRD peaks. We consider
it unlikely that the peak may emerge from a substitutional defect
of Na on either the Zn or Te position, due to the difference in charge
and size. Under all circumstances, such a defect is expected to have
a chemical shift to the right of the prismatically coordinated Na,
considering that Na on the Zn site will be octahedrally coordinated.
Due to the ambiguous decomposition of the 23Na MAS NMR
spectra, the changes in the Na sublattice from the Ga substitution
cannot be described in sufficient detail.
125Te NMR Studies
The
NZTO-based materials were further characterized by means of 125Te MAS NMR; see spectra in Figures and S4 for curve fittings.
The 125Te spectrum of the NZTO (x = 0.00,
black line, Figure ) shows one peak at 155 ppm with a distinct shoulder at approximately
145 ppm. The physical origin of this shoulder feature will be discussed
in Section . Integration
of this shoulder feature (145 ppm) in the samples x = 0.00 and 0.05 is counted as part of the main peak (150 ppm) in
this section. Furthermore, note that the spectrum cannot be unambiguously
decomposed, and at least three Gaussian peaks are needed for a good
peak shape description. As Te takes one single crystallographic site
(Wyckoff site 2c) and is a spin 1/2 nucleus, the
presence of multiple peaks must be due to different local structures
around Te atoms. Upon Ga substitution, additional peaks emerge in
the region below 140 ppm (Figure ). All Ga-substituted samples show a feature around
140 ppm, while x = 0.15 and 0.20 show a weaker peak
at about 125 ppm as well. Based on charge and size arguments, we claim
that Ga substitutes for Zn are in compliance with the intensities
of the XRD patterns. A Ga atom at a Zn site will therefore be within
the second coordination sphere of three Te atoms. By curve fitting
and integration, we estimated the relative amounts of the main peak
at 155 ppm and the two side peaks at 140 and 125 ppm (see Table below). The integration
shows that the theoretical estimate of the number of Te atoms with
different surroundings corresponds very well with the integrated ratio
of the observed peaks, assuming the peak at 140 ppm to reflect Te
atoms with one Ga neighbor and the 125 ppm peak to reflect two neighbors.
Figure 4
125Te MAS NMR spectra of Na2–Zn2–GaTeO6. Two peaks that appear at higher substitution
levels are marked with black arrows for x = 0.20.
Table 1
Integrated Peak Intensities and Percentage
of Te Atoms with at Least One Close Neighbor Ga Atom for Na2–Zn2–GaTeO6a
x
theoretical
Te with at least one Ga neighbor [%]
I (155 ppm) [%]
I (140 ppm) [%]
I (125 ppm) [%]
sum small
peaks [%]
0.00
0.0
100.0
0.0
0.0
0.0
0.05
7.5
86.4
11.1
0.0
11.1
0.10
15.0
83.9
16.1
0.0
16.1
0.15
22.5
75.0
22.4
2.6
25.0
0.20
30.0
71.2
22.3
6.6
28.9
For x = 0.20, 10%
of Zn atoms are replaced by Ga. Each Zn site has three Te neighbors,
implying that 30% of the Te atoms for x = 0.20 have
at least one Ga neighbor.
125Te MAS NMR spectra of Na2–Zn2–GaTeO6. Two peaks that appear at higher substitution
levels are marked with black arrows for x = 0.20.For x = 0.20, 10%
of Zn atoms are replaced by Ga. Each Zn site has three Te neighbors,
implying that 30% of the Te atoms for x = 0.20 have
at least one Ga neighbor.The highest substitution level of x = 0.20 should
influence 30% of the Te atoms. The integration shows that the main
peak amounts to 71.2%, and the two smaller peaks sum up to 28.8%,
which is in good agreement with the expected value. An exception is x = 0.05, for which the integrated value is higher than
the theoretical value (11.1 vs 7.5, respectively), which can be attributed
to uncertainties in the integration of the weak peak at 140 ppm and
the high influence of variations during phasing. The increase in only
the two-neighbor peak (at 125 ppm) between x = 0.15
and 0.20 are indications that the Ga distribution is less random at
high substitution levels. We note a change in the peak shape also
for the main peak with increasing x. Hence, Te atoms
with no neighboring Ga atoms are also affected. The nature of the
changes is explored in Section . Note that there are no indications that any 23Na or 125Te peaks are due to significant amounts
of a secondary phase. Based on our NMR analyses, it is likely that
samples correspond to the nominal composition targeted in the synthesis,
except for maybe the material with x = 0.05. This
suggests that the deviation in the c-parameter for
the x = 0.15 sample is not due to aspects of Ga concentration.
Furthermore, the NMR data clearly indicate that the homogeneous substitution
of Ga is obtained upon sol–gel synthesis.
DFT Calculations of 125Te Chemical
Shifts
To progress further with analyses of the 125Te spectra, DFT calculations of chemical shifts were carried out
as we expected 125Te chemical shifts to be influenced by
the distribution of Na ions between the g-, f-, and a-sites due to its many electrons.
Out of these sites, Na atoms in the a-sites have
the largest separation from the Te site. Hence, for the NMR spectra,
focus was on the f- and g-sites.
We describe the Te environment with respect to interlayer Na cations
with the notation namb, where na and mb refer to two neighboring sodium layers; a, b denotes the type of Na site (f or g) and n, m describes the number of Na in the said type of site (0,
1, 2, 3). In the case of an f-site, only n, m = 0, 1 are possible. When n = 0 or m = 0, either na or mb is omitted for simplicity. Some possible
coordination environments for Te are shown in Figure .
Figure 5
Five Te environments, in addition to the 1f1f-environment. As noted, the 3g2g is not common but is included to calculate
the influence
of the number of Na neighbors to Te. Note: there are 12 distinct Te
configuration environments in total.
Five Te environments, in addition to the 1f1f-environment. As noted, the 3g2g is not common but is included to calculate
the influence
of the number of Na neighbors to Te. Note: there are 12 distinct Te
configuration environments in total.Calculations to benchmark various approaches were
performed on
the most stable configuration reported in our previous work.[13] This arrangement is a modification of the hexagonal
structure, with twice as many atoms in the unit cell to account for
a nonhexagonal reconstruction of the Na sublattice with Na ions equally
distributed across the g- and f-sites
and with a-sites unoccupied. In this model, all Te
atoms exhibit a 2g1f coordination
environment.Obtained benchmarking chemical shift data are reported
in Table and compared
with
experimental values. The GGA calculation correctly reproduces the
sign of the chemical shift and its order of magnitude but deviates
clearly from the experimental reference. It is hence tested whether
a different setup for the calculation would provide a chemical shift
closer to the measured values.
Table 2
Calculated Shifts According to Three
Methods for the 2g1f Environment
in NZTO. TeO2 is Used as a Reference in the Computations,
While Te(OH)6 is the Standard Used for Referring Te Shifts
and in Experiments
method
shift from
TeO2 [ppm]
shift from
Te(OH)6 [ppm]
GGA (standard setting)
–291
460
GGA + core states
–278
473
SCAN + core states
–609
142
experimental
span NZTO
–606
to −587
145–164
The most accurate set of PAW potential is adopted.
In this approach,
labeled as “GGA + core states” in Table , the most external full shells of p and
s electrons are treated as valence electrons, and the associated Kohn–Sham
equations are explicitly solved. This method did not provide a shift
value closer to the experiment. We note that the usage of hybrid functional
(i.e., approaches mixing PBE and Hartree–Fock results when
computing the exchange portion of the energy) is not viable due to
the size of the system (4 formula units, i.e., 44 atoms). A more suitable
option is the Meta-GGA functionals using the Laplacian of the density
or the kinetic energy on top of the density and its gradient considered
by GGA. Within this class of functionals, SCAN recently emerged as
an approach capable of an accurate description of bonding in various
cases, including oxides such BaTiO3, PbTiO3,
and BiFeO3,[50] while maintaining
a computational cost comparable to GGA. The reason for this improvement
in accuracy is, however, not obvious. While SCAN usually provides
more accurate interatomic distances than GGA, the computed values
are, in both cases, compatible with experimental data, as shown in Table S5.The SCAN-based description of
the chemical bonding, Table S6, is compatible
with the GGA reference
and shows a substantial ionic character in good agreement with expectations.
The calculated Te shift is fully compatible with experimental references.
For this reason, we use the SCAN method and proceed to a modified
Te environment to compute the effect on the chemical shift. These
environments are constructed to generate different Te coordination
environments and are explained in detail in Section S5.Due to the small size of the system, only a few configurations
can be explored. We have opted not to use a supercell system since
a large number of atoms in a linear response calculation of this kind
significantly increases the computational cost, and convergence of
the self-consistent field computation is hard to achieve. The number
of atoms is kept constant, and the Na distribution is rearranged to
obtain the most frequently observed coordination environments for
Te (computed by analysis of MD trajectories described in Section ). These coordination
environments are 1g1f, 2g1f, 2g1g, and 2g1g. The 3g2g environment, albeit rarely encountered, is also
considered to be better, influencing the number of Na ions in the
Te coordination environment. Figure below shows the calculated chemical shift values for
five different Te environments in NZTO.
Figure 6
Calculated chemical shift
values for five Te environments in NZTO
that are produced by four different Na configurations as explained
in more detail in Section S5.
Calculated chemical shift
values for five Te environments in NZTO
that are produced by four different Na configurations as explained
in more detail in Section S5.There are two noticeable trends for the Te chemical
shifts seen
in Figure . Te atoms
with a larger number of Na neighbors are more shielded and therefore
shifted to a lower frequency compared to Te atoms with fewer Na neighbors.
A comparison of the 2g1f and 2g1g environments is the only instance where
the difference between the f- and g-sites can be determined, as one set of neighbors (2g) is the same for both, while the second is either f or g. In this situation, the edge-sharing g-position provides better shielding than the face-sharing f-site. Overall, the trend in chemical shifts can be summed
up as follows:Less shielding of Te is provided by
fewer Na neighbors, which shifts the spectra to higher frequencies/ppm
values.Less shielding
of Te is provided by
Na atoms in the f-position (face-sharing) than those
in the g-position (edge-sharing). This shifts the
spectra to higher frequencies/ppm values.On one side of a Te atom, there can be one, two, or
three Na ions
in g-sites or only one in an f-site.
Hence, the 1st point is only relevant for environments involving g-sites.We observe that for a given Te environment,
the calculated shift
is different depending on the Na configuration, i.e., it is influenced
by Na positions beyond those that are directly face- or edge-sharing
to the given Te atom. Since relatively small periodic systems are
used for these computations, the Na distribution exerts certain distortions
on the lattice, expectedly to be a feature of the simulations.Based on these trends, we expect that Ga3+ substitution
at the Zn2+ sites, which in turn will lower the amount
of Na+, will result in a change in the peak intensities
in the 125Te MAS NMR spectra toward higher frequencies,
which is exactly what is observed in Figure . The main peak (Te with zero close Ga neighbors)
shifts to the left with increasing substitution, consistent with a
lower Na content.Albeit we observe just a moderate shift of
2 ppm in the peak position,
the width of the main peak broadens on Ga substitution. This may be
due to increased dipolar couplings of Te with substituted Ga, as all
Ga atoms have nuclei with magnetic moments, and only about 4% of Zn
atoms have nuclear magnetic moments. The Te–Ga interactions,
in addition to the already in place Te–Na interactions, and
the relative strengths may be discussed by considering the magnetogyro
ratios of 125Te, 69,71Ga, and 23Na
(all are quite similar) and distances from Te to these elements (see
details in SI9). The Te–Na and Te–Zn/Ga
distances from the average structure from XRD are 2.81 and 3.05 Å,
respectively. Hence, by increasing the Ga content, one could expect
a relative increase in nuclear dipole–dipole couplings of Te,
albeit complicated due to Ga’s relaxation rates. Furthermore,
Na is known to be dynamic at room temperature in these materials,
and Na’s interactions with Te are therefore decreased relative
to a static case. The result is that when Ga is substituted into the
material, one could expect a broadening of Te peaks due to the increase
in dipole–dipole couplings of Te and nearby nuclei.
Ab Initio MD Simulations:
Na Distribution and Te Environments
It is not possible to
break down 125Te spectra into an unambiguous decomposition,
and DFT simulations are performed to gain some insight into the Te
coordination environments. Three compositions of Na2–Zn2–GaTeO6 type with x = 0 (NZTO), 0.083 (2Ga), and 0.167 (4Ga) were explored with ab initio MD simulation, the latter two with, respectively,
2 and 4 Ga3+ ions in a supercell with 24 formula units.
The construction of the systems is explained in Section S7. For each composition x, we consider
two simulation temperatures, 750 and 1000 K. As demonstrated in Section S7, the 4Ga system exhibits a clear preference
for an uneven Na distribution when comparing Na layers. In this case,
a 23:21 distribution of the 44 Na ions has an energy gain of 0.2 eV
with respect to a system with an even (22:22) distribution. The layer
with a larger vacancy concentration exhibits an increased occupancy
of the a-site.The average occupation of the
Na sites is computed from the AIMD trajectories using an ad
hoc procedure described in S8 and
reported in Table S7. When examining these
data, it is important to keep in mind the multiplicity of the three
sites: if the occupancy of all of the available sites were equal,
the sum of the g-sites would be three times as populous
as that of the a-site. At 750 K, we note that an
increased amount of Ga corresponds to a more favorable occupation
of the a-sites. At 1000 K, the Na site population
of all systems is compatible, and it is impossible to identify any
effect of Ga substitution. Using the described labeling of the occupied
Na sites, we can determine the coordination environments of Te from
the AIMD trajectories and compute their abundance using an extension
to the algorithm described in Section S8. The resulting population for 750 K is shown in Figure a. At this temperature, the
Ga substitution influences the Na distribution.
Figure 7
Te environments from
50 ps MD at 750 K. The number of Na neighbors
around Te is marked as gray and white areas as a guide to the eye.
(a) Relative percentages of each Te environment; (b) cumulative distribution,
where amounts of each environment are added in the order of calculated
shielding from Section . The average of two 4Ga runs is plotted, with the two individual
runs indicated by gray dotted lines.
Te environments from
50 ps MD at 750 K. The number of Na neighbors
around Te is marked as gray and white areas as a guide to the eye.
(a) Relative percentages of each Te environment; (b) cumulative distribution,
where amounts of each environment are added in the order of calculated
shielding from Section . The average of two 4Ga runs is plotted, with the two individual
runs indicated by gray dotted lines.For the pure NZTO, the more populous environments
are 1g1f, 2g1f, 2g1g, and, to a minor
extent,
2g2g, whereas the 1f1f is not populated at all. As the f-site has an expected high occupancy, this may then indicate that
the Na layers are not independent but that the Na in one layer influences
the structure in adjacent layers. In 4Ga, it is interesting to note
that the 1f environment becomes very populated as
the f- and a-sites become more favorable.
As shown in Figure b, we further note that the 2g1g environment becomes highly populated for 2Ga.With the limited
size of the supercell, the amount of each environment
is quite low, and the exact number is therefore quite uncertain. Instead,
one can look at the general trends, which are clearer when looking
at the cumulative distribution of Te environments in Figure b, plotted in the order of
the shielding calculated in Section . This plot demonstrates that the samples
with the high level of Ga substitution have more of the Te environments
with a low number of Na neighbors, while the unsubstituted material
has more of Te environments with a high number of Na neighbors. This
is fully in line with the interpretation of the 125Te NMR
data: the spectra will gain more intensity in the high-frequency region
(left part) upon Ga substitution due to an increase of Te environments
with fewer Na neighbors. It should be noted that this is not a peak
shift but a relative change in the peak intensity ratios for different
environments. This could be the explanation for the disappearance
of the shoulder peak at 145 ppm, which is due to Te environments with
a high number of Na neighbors for the materials with a lower amount
of Na. This is also consistent with the observed features in the Te
spectra, where the environments do not vary linearly with composition x. The peak maxima shift minimally, but the edges of the
peak shift to a larger extent. The shift of the high-frequency edge
is well in line with the increased population of the 1f environment, which is expected to be at a higher frequency than
any environment in the pure NZTO. Furthermore, it is very likely that
the 125Te NMR spectra consist of multiple overlapping peaks,
which are not resolved.
Comments on Ion Conductivities Based on New
Synthesis Protocol: Comparison and Discussion
The homogeneity
of Ga in the Ga-substituted materials is likely not to have a large
direct influence on the total ionic conductivity as measured by, e.g.,
impedance measurements. The synthesis method we have reported is employed
to control the stoichiometry, ensuring that no region has a lower
degree of substitution, which in turn might give a local decrease
in ionic conductivity. The bulk (interlayer) conduction is based on
the large number of vacancies relative to the Na number, which should
be comparable if samples are stoichiometric. A comparison between
the 23Na NMR for NZTO synthesized with sol–gel and
solid-state synthesis is shown in Section S10, which demonstrates the same local environment. This suggests that
the different synthesis methods have very little influence on the
local structure, which would result in a relatively similar bulk conductivity.
However, there are other influences on the total ion conductivity
where the synthesis method is believed to have a greater influence.
One is the grain boundary conductivity, which was demonstrated by
Wu et al. to be 2 orders of magnitude lower than that of the bulk,
greatly limiting the total conductivity.[15] The temperature program used in this work has a shorter heating
time than previous studies, which would yield smaller particles, resulting
in more grain boundaries and thus might reduce total ionic conduction.
Material preparation aiming for high ion conductivity might therefore
have to be further optimized to give large particles and dense samples,
which should be possible as the sol–gel synthesis method can
tailor particle size and morphology.
Conclusions
In this work, we have described
sol–gel synthesis and structural
characterization of layered NZTO and its Ga-substituted derivatives
(Na2–Zn2–GaTeO6, x = 0.00, 0.05, 0.10, 0.15, 0.20) by means of XRD, MAS NMR, and DFT
methods.The sol–gel synthesis protocol we applied provided
samples
with a high level of purity and with a homogeneous distribution of
Ga. This is essential for the manufacturing and for the detailed characterization
of a solid-state electrolyte candidate material, in particular when
it comes to relationships between composition (substituents) and structure
(sites).The NMR data, with the support of DFT modeling, suggest
a uniform
Ga substitution; hence, we can claim that Ga atoms take the position
of the Zn atoms with a concomitant reduction of the Na content. The
introduction of heterovalent Ga atoms influences the Na substructure,
in a way that the various Wyckoff sites become more energetically
similar. The DFT modeling also suggests an inhomogeneous Na distribution
between the neighboring layers for higher substitutions, in addition
to an influence on the Na distribution in one layer from the Na structure
in the adjacent layers.The 125Te NMR chemical shift
values are influenced by
both Na and Ga. The effect created by the Na distributions in the
two neighboring interlayers was analyzed by DFT calculations. We found
that linear response calculation using the SCAN functional gave values
for the chemical shifts within the experimental range. The Ga-containing
samples showed additional peaks in the 125Te NMR spectra
in quantities as expected for a uniform substitution mechanism.
Authors: Ask Hjorth Larsen; Jens Jørgen Mortensen; Jakob Blomqvist; Ivano E Castelli; Rune Christensen; Marcin Dułak; Jesper Friis; Michael N Groves; Bjørk Hammer; Cory Hargus; Eric D Hermes; Paul C Jennings; Peter Bjerre Jensen; James Kermode; John R Kitchin; Esben Leonhard Kolsbjerg; Joseph Kubal; Kristen Kaasbjerg; Steen Lysgaard; Jón Bergmann Maronsson; Tristan Maxson; Thomas Olsen; Lars Pastewka; Andrew Peterson; Carsten Rostgaard; Jakob Schiøtz; Ole Schütt; Mikkel Strange; Kristian S Thygesen; Tejs Vegge; Lasse Vilhelmsen; Michael Walter; Zhenhua Zeng; Karsten W Jacobsen Journal: J Phys Condens Matter Date: 2017-03-21 Impact factor: 2.333
Authors: J Lizion; A Piarristeguy; R Laskowski; P Blaha; R Escalier; M Ménétrier; A Pradel; G Silly Journal: Solid State Nucl Magn Reson Date: 2021-07-27 Impact factor: 2.293