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Mixed-Metal Monophosphate Tungsten Bronzes Containing
Rhodium and Iridium
Alexander Karbstein,[a] Markus Weber,[a] Dominic Lahr,[a] Jörg Daniels,[a]
Wilfried Assenmacher,[a] Werner Mader,[a] Frank Rosowski,[b] Stephan A. Schunk,[c] and
Robert Glaum*[a]
Solution combustion synthesis followed by annealing in air led
to the MPTB-related phosphates (Rh1/6W5/6O3)8(PO2)4, (Ir1/6W5/
6O3)8(PO2)4(a=5.258(2) Å, b=6.538(3) Å, c=17.322(8) Å), (Rh1/
9W8/9O3)12(PO2)4and (Rh2/21W19/21O3)14(PO2)4. Single-crystals of the
mixed-metal (Rh,W)-MPTBs at m=4 and at m=7 were grown
by chemical vapor transport (CVT). Their crystal structures have
been refined from X-ray single-crystal data {(Rh,W)-MPTB at
m=4:P212121,Z=1, a=5.2232(3) Å, b=6.4966(3) Å, c=
17.3819(9) Å, R1=0.032, wR2=0.075 for 1714 unique reflections,
1524 with Fo>4σ(Fo), 66 variables, 1 constraint, composition
from refinement (Rh0.15W0.85O3)8(PO2)4;(Rh,W)-MPTB at m=7:
P21/n,Z=1, a=5.2510(4) Å, b=6.4949(5) Å, c=26.685(2) Å, β=
90.30(1)°,R1=0.060, wR2=0.163 for 2074 unique reflections,
1894 with Fo>4σ(Fo), 100 variables, comp. from ref.
(Rh0.07W0.93O3)14(PO2)4}. These structure refinements show un-
expected distribution of Rh and W over the available metal
sites. Further characterization (powder reflectance and mag-
netic measurements) of the (Rh,W)-MPTB at m=4 and at m=7
suggest for both phases a homogeneity range with respect to
the Rh/W ratio and the presence of small amounts of W5+
besides Rh3+and W6+. Results of the ligand field analysis for the
reference material Rh(PO3)3, which is containing the octahedral
chromophore [RhIIIO6], are reported (Δo=23200 cm1,B=
490 cm1).
Introduction
Thermodynamically metastable, multinary tungsten phosphates
with ReO3-like XRPD-pattern containing platinum group metals
have recently been identified as catalyst materials for the
formation of maleic anhydride via selective oxidation of n-
butane.[1] Annealing these catalyst materials at temperatures
above 900°C leads to phases with XRPD pattern resembling
those of phosphate tungsten bronzes (PTBs). These mixed-
metal PTBs are expected to contain platinum group metals
(PGM) in well-established chemical environments, which should
lead, following the reasoning of the concepts of single-site
catalysts and site isolation,[2] to even better catalyst perform-
ance than that observed for the disordered solids with ReO3-like
XRPD-pattern. Furthermore, up to now only a few anhydrous
phosphates of rhodium and iridium have been characterized
crystallographically (RhPO4and Rh(PO3)3,[3] Ir(PO3)3[4]). For this
reason further characterization of PGM-containing mixed-metal
MPTBs appeared of additional interest.
Since the discovery of the first tungsten bronze AxWO3(A:
Na, K) with yellow-golden color and metallic luster by Wöhler in
1825,[5] a wide range of bronzes containing transition metals
have been studied.[6] Their structures consist of corner-sharing
MO6octahedra arranged in a 3D-network, which can be
interpreted as a distorted ReO3-type structure. The interstitial
position can be occupied by a large cation Ato build a
perowskite-type structure, which leads to mixed-valency tung-
sten (V,VI) and, as a result, interesting physical properties (e.g.
electrical conductivity, antiferromagnetic ordering or super-
conductivity at low temperatures).[7,8]
Raveau et al. synthesized phosphate tungsten bronzes
(PTB), where ReO3-like slabs of WO6octahedra are separated by
phosphate (PO4) or diphosphate (P2O7) groups. These phos-
phates can be grouped into three classes of PTBs according to
their structural features: the monophosphate tungsten bronzes
with pentagonal tunnels (MPTBp) and the general formula
(WO3)2m(PO2)4with 2m14, the monophosphate tungsten
bronzes with hexagonal tunnels (MPTBh)Ax(PO2)4(WO3)2m (A: Na,
K, Pb) with 4m10 and the diphosphate tungsten bronzes
(DPTB) Ax(P2O4)2(WO3)2m (A: K, Rb, Ba, Tl) and 4m10.[9] Note,
that the A-site is not necessarily required to be occupied by a
cation. It can be empty, thus leading to pure mixed-valent
tungsten phosphates.
[a] A. Karbstein, M. Weber, D. Lahr, Dr. J. Daniels, Dr. W. Assenmacher,
Prof. Dr. W. Mader, Prof. Dr. R. Glaum
Institut für Anorganische Chemie
Rheinische Friedrich-Wilhelms-Universität Bonn
Gerhard-Domagk-Str. 1, D-53121 Bonn (Germany)
https://www.glaum.chemie.uni-bonn.de/arbeitsgruppe/mitarbeiter/
glaum
[b] Dr. F. Rosowski
BasCat - UniCat BASF JointLab, Technische Universität Berlin, 10623 Berlin,
Germany
https://www.bascat.tu-berlin.de/bascat/menue/about_us/scientific_dir-
ectors/
[c] Dr. S. A. Schunk
hte GmbH, Kurpfalzring 104, 69123 Heidelberg, Germany
https://www.hte-company.com/
Supporting information for this article is available on the WWW under
https://doi.org/10.1002/ejic.202100047
© 2021 The Authors. European Journal of Inorganic Chemistry published by
Wiley-VCH GmbH. This is an open access article under the terms of the
Creative Commons Attribution Non-Commercial License, which permits use,
distribution and reproduction in any medium, provided the original work is
properly cited and is not used for commercial purposes.
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In particular, the MPTBpphases with their electronic
structure are of interest, because they show phase transitions at
low temperatures, which may lead to superconductivity and
charge localization effects (charge density waves). An inves-
tigation of (WO3)14(PO2)4(m=7) shows two phase transitions at
T1=188 K and T2=60 K. These are related to Peierls distortions
leading to charge density wave states and superconductivity
below T<0.3 K.[8]
Substitution of tungsten(V) in the ReO3-like slabs by other
transition metals is possible. It is already known, that W5+can
be replaced by appropriate combinations of tungsten(VI) with
MIV or MIII according to M IV
1=2WVI
1=2and M III
1=3WVI
2=3, respectively. For
the MPTB (WO3)4(PO2)4(m=2) mixed-metal substitution variants
with M: VIII, IV, CrIII, FeIII, MoIII, IV and TiIV have been reported.[10] In
addition to the described MPTBs at m=2, for M: Sc, V, Cr, Fe,
Mo, Ru, Rh, In and Ir the ortho-pyrophosphates MIII-
(WO2)2(P2O7)(PO4) of identical sum formula (with respect to the
MPTBs) but different structure were obtained.[10]
In this paper we report on synthesis, thermal behavior and
characterization of several mixed-metal (Rh,W)- and (Ir,W)-
MPTBs. For characterization results from XRPD, SXRD, electron
microscopy, UV/vis-spectroscopy, and magnetic measurements
are presented.
Results and Discussion
Synthesis
The new mixed-metal (mm) MPTBs (Rh1/6W5/6O3)8(PO2)4, (Rh1/9W8/
9O3)12(PO2)4, (Rh2/21W19/21O3)14(PO2)4and (Ir1/6W5/6O3)8(PO2)4have
been obtained as single-phase, micro-crystalline powders
(XRPD) by solution combustion synthesis (SCS)[11] followed by
annealing of the combustion products in air. For SCS Rh(NO3)3
(Umicore, Hanau) or Ir(acac)3(Umicore, Hanau), (NH4)6W12O39-
(H2O)4.8 (Alfa Aesar, Karlsruhe), H3PO4(VWR, Darmstadt), and the
polydentate ligand glycine (Labochem International, Heidel-
berg) were dissolved in water (molar ratio metal : glycine=1:3).
Conc. HNO3(Fisher Scientific, Schwerte) in excess was added as
oxidant to the solution to prevent the reduction of rhodium or
iridium during the combustion. To our observation, formation
of the PGM metals is irreversible under the described reaction
conditions and has to be avoided. The solutions were
evaporated at temperatures #100°C and thereafter ignited in
a preheated furnace at #=400°C, where a self-propagating
combustion took place and yielded black, voluminous, amor-
phous (XRPD) powders. These intermediates were ground and
annealed in air with stepwise rising of the temperature up to
1000°C for (Rh1/6W5/6O3)8(PO2)4and (Ir1/6W5/6O3)8(PO2)4and up to
1100°C for (Rh1/9W8/9O3)12(PO2)4and (Rh2/21W19/21O3)14(PO2)4. Thus
obtained powders display a dark-green color for the rhodium
and black for the iridium compounds. XRPD pattern were
recorded after each annealing step to control the progress of
product formation until the thermodynamically stable mm-
MPTB phase was obtained single-phase (see XRPD pattern in
Figure 1 and Figures S1-S4). In case of (Rh1/9W8/9O3)12(PO2)4the
described procedure led always to (Rh2/21W19/21O3)14(PO2)4as
minor by-phase. We attribute this outcome to the close
proximity of chemical composition of the two compounds and
the rather small amounts of material used for synthesis, due to
the high cost of rhodium.
Experiments aiming at “(Rh2/9W7/9O3)6(PO2)4 (m=3), “(Rh2/
15W13/15O3)10(PO2)4 (m=5) or “(Rh1/12W11/12O3)16(PO2)4 (m=8) led
to the neighboring MPTB phases. In case of iridium only (Ir1/6W5/
6O3)8(PO2)4was formed. The mixed-metal MPTBs (M1/3W2/
3O3)4(PO2)4(m=2) with M=Rh, Ir were never observed. Instead,
formation of M(WO2)2(P2O7)(PO4)2(M=Rh, Ir) did occur, as
previously described by Roy et al.[12]
Lattice parameters of the MPTBs were determined using the
program SOS[13] and α-SiO2(Merck, Darmstadt) as internal
standard (see Table 1). Interestingly, the lattice parameters a
and bwhich are parallel to the ReO3-type slabs of the (Rh,W)-
MPTBs are smaller compared to the pure tungsten MPTBs,
whereas the parameter c(perpendicular to the ReO3-type slabs)
is enlarged (Table 1).
Figure 1. XRPD pattern (IP Guinier technique, Cu-Kα1) of (Rh1/6W5/6O3)8(PO2)4
(top) and (Rh2/21W19/21O3)14(PO2)4(bottom) with simulations based on SXRD
data. (Ir1/6W5/6O3)8(PO2)4and (Rh1/9W8/9O3)12(PO2)4(middle) with a simulation
based on (Rh2/21W19/21O3)14(PO2)4(grey) and (WO3)8(PO2)4[14] or (WO3)12(PO2)4[15]
(black) with an even distribution of rhodium/iridium over all three tungsten
sites.
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Progress of phase formation and thermal decomposition
For (Rh2/21W19/21O3)14(PO2)4, the (Rh,W)-MPTB at m=7, as
representative example, the progress of phase formation
starting from the amorphous intermediate obtained by SCS is
summarized in Figure 2. It shows, rather unexpectedly, strong
kinetic effects during phase formation. After SCS (400°C ignition
temperature; hot spot temperature up to 900°C for a few
seconds) the intermediate exhibits a diffraction pattern typical
of an amorphous solid. Heating to 750°C leads to less
“amorphous background” and development of rather broad
Bragg peaks indicating the formation of a thermodynamically
metastable phase with a ReO3-related pattern. The chemical
composition of this phase, (Rh2/21W19/21O3)14(PO2)4, can be re-
written as (RhIII2/27WVI19/27PV6/27)(O25/9&2/9) to emphasize its rela-
tion to ReO3and to show the oxygen-deficiency as a
consequence of the average oxidation state of the cations. This
and related ReO3-like phases are obtained with high reproduci-
bility by the described protocol and they show remarkable
thermal stability against transformation into the thermodynami-
cally stable equilibrium phases. However, without SCS and
initial annealing temperatures too high these phases were
never obtained.
Surprisingly, transformation (equilibration) of the single-
phase homogenous ReO3-like phase to the microcrystalline
powder of (Rh2/21W19/21O3)14(PO2)4(m=7) does not occur
directly, but via the apparently kinetically favorable formation
of the (Rh,W)-MPTB at m=4 (depleted in WO3with respect to
the starting composition) and a WO3-rich phase with ReO3-
related XRPD pattern. Thus, as can be taken from Figure 2,
above 800°C a pattern similar to (WO3)8(PO2)4(MPTB at m=4)
begins to emerge from the amorphous background. Simulta-
neously, the lattice parameter aof the ReO3-like phase shrinks
slightly from 3.79 Å to 3.71 Å (see Table 2) and is thus
approaching the value given in literature for cubic WO3.[17] We
are therefore relating this change to a depletion of the ReO3-
like phase of rhodium and phosphorus and an enrichment by
WO3. The powder obtained after annealing at 1000°C (Figure 2)
clearly shows, according to its XRPD pattern, an off-equilibrium
mixture of three phases. The presence of the WO3-rich, ReO3-
like phase (~16%wt) and of the intermediate (Rh,W)-MPTB (m=
4; ~47%wt), which has a higher content of rhodium and
phosphorus than the starting mixture is apparently kinetically
controlled. The equilibrium phase (Rh2/21W19/21O3)14(PO2)4(m=7)
is already present in the mixture at ~37%wt. Eventually, after
annealing at 1100°C the targeted (Rh,W)-MPTB at m=7 is
obtained as single-phase powder. Further heating up to 1200°C
of this (Rh,W)-MPTB in air leads to decomposition to P4O10
vapor, WO3(monoclinic after quenching to ambient temper-
Table 1. Lattice parameters from XRPD data of (Rh,W)- and (Ir,W)-MPTBs in comparison to the pure tungsten phosphates.
Compound a[Å] b[Å] c[Å] β[°]
m=4 (orthorhombic)
(WO3)8(PO2)4[14] 5.285(2) 6.569(1) 17.351(3)
(Rh1/6W5/6O3)8(PO2)45.223(1) 6.513(2) 17.356(6)
(Rh0.15W0.85O3)8(PO2)4[a] 5.2232(3) 6.4966(3) 17.3819(9)
(Ir1/6W5/6O3)8(PO2)45.258(2) 6.538(3) 17.332(8)
m=6 (orthorhombic)
(WO3)12(PO2)4[15][a] 5.2927(7) 6.5604(7) 23.549(3)
(Rh1/9W8/9O3)12(PO2)45.229(2) 6.540(3) 23.599(7)
m=7 (monoclinic)
(WO3)14(PO2)4[16][a] 5.291(1) 6.557(2) 26.654(8) 90.19
(Rh2/21W19/21O3)14(PO2)45.245(2) 6.507(2) 26.693(8) 90.10(4)
(Rh0.07W0.93O3)14(PO2)4[a] 5.2510(4) 6.4949(5) 26.6854(19) 90.30(1)
[a] Lattice parameters from single-crystal measurement at room temperature (crystals from CVT, composition from structure refinement).
Figure 2. XRPD pattern (IP Guinier technique, Cu-Kα1) of (Rh2/21W19/
21O3)14(PO2)4after several consecutive steps of annealing starting with the
combustion product from SCS, rel. amounts (wt %) estimated with
MATCH!.[19]
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ature), and rhodium (see Eq. 1). The latter two solid phases
were identified by XRPD.
The progress of phase formation observed for the other
mm-MPTBs under consideration, (Rh1/6W5/6O3)8(PO2)4, (Ir1/6W5/
6O3)8(PO2)4and (Rh1/9W8/9O3)12(PO2)4is very similar to the one
described for (Rh2/21W19/21O3)14(PO2)4(see Tables S5-S7). How-
ever, there is variation in the temperature required to obtain
the single-phase mm-MPTB and in their decomposition temper-
atures. Single-phase powders of (Rh1/6W5/6O3)8(PO2)4and (Ir1/6W5/
6O3)8(PO2)4(both m=4) are formed already at about 800°C,
(Rh1/9W8/9O3)12(PO2)4(m=6) around 1050°C and (Rh2/21W19/
21O3)14(PO2)4(m=7) around 1100°C. Short annealing periods of
a few hours only slightly above their decomposition temper-
atures leads to stepwise loss of P4O10 and the formation of
elementary rhodium and the (Rh,W)-MPTB with the next higher
m(higher WO3content). Overall, the decomposition temper-
ature of the (Rh,W)-MPTBs increases with decreasing content of
rhodium/P4O10. This observation fits to the decomposition
behavior of pure rhodium phosphates (Rh(PO3)3, RhPO4), where
the activity of P4O10 is higher and decomposition in air begins
at 950°C.[18]
(1)
Based on their thermal decomposition temperatures and
the assumption that p(O2) should exceed 0.2 bar for a
detectable decomposition effect, an estimate of the thermody-
namic data DfH0
298;S0
298;Cp(coefficients A, B, C) of (Rh1/6W5/
6O3)8(PO2)4and (Rh2/21W19/21O3)14(PO2)4was possible using the
data of the binary oxides Rh2O3, WO3and P4O10. The estimation
follows a procedure applied by Schäfer for LaPO4.[20] For a
summary of thermodynamic data used in the context of this
paper, see Table S1.
Crystallization by chemical vapor transport
Crystals of the (Rh,W)-MPTBs (Rh1/6W5/6O3)8(PO2)4(m=4), (Rh1/
9W8/9O3)12(PO2)4(m=6) and (Rh2/21W19/21O3)14(PO2)4(m=7) have
been grown by chemical vapor transport (CVT)[21] in sealed silica
tubes (l=14 cm, d=1.5 cm) with chlorine as transport agent.
These show a dark greenish color, have edge lengths up to
300 μm and are isometric with a rectangular shape (Figure 3).
Pre-synthesized, single-phase powders (from SCS followed
by annealing in air) were used as starting materials for CVT.
Small amounts of PtCl2(~15 mg) were added for in situ
generation of chlorine, the transport agent. Temperature
gradients 950!900°C for (Rh1/6W5/6O3)8(PO2)4and 1090!
1050°C for (Rh1/9W8/9O3)12(PO2)4and (Rh2/21W19/21O3)14(PO2)4were
applied. Ampoules were kept in the furnaces for 14 d. Under
the given experimental conditions no decomposition of the
(Rh,W)-MPTBs was observed. However, transport of (Rh1/9W8/
9O3)12(PO2)4and (Rh2/21W19/21O3)14(PO2)4in the temperature
gradient 950!900°C led to deposition of (Rh1/6W5/6O3)8(PO2)4in
the sink due to non-stationary behavior of the system. For a
general explanation of non-stationary transport behavior
see.[21,22]
Chemical vapor transport of (Rh1/6W5/6O3)8(PO2)4with chlor-
ine as transport agent was modelled with the computer
program CVTrans[23] using thermodynamic data given in
Table S1. According to the modelling and in agreement with
literature on CVT of WO3and Rh2O3the transport active gas
species are WO2Cl2, RhCl3, P4O10, and O2(see Eq. 2).[18,21]
(2)
Crystal structure analyses
The (Rh,W)-MPTB at m=4 and m=7 are isotypic to their pure
tungsten MPTB counterparts (WO3)8(PO2)4(P212121,Z=1)[14] and
(WO3)14(PO2)4(P21/n,Z=1).[16] Table 3 provides a summary on
data collection and refinement of the crystal structures. Atomic
coordinates and isotropic displacement parameters are shown
in Table 4 and Table 5 (Anisotropic displacement parameters
see Table S2 and Table S3). Refinements for both (Rh,W)-MPTB
were hampered by twinning, cation disorder, and possibly
stacking faults all of which are typical for monophosphate
tungsten bronzes as has been pointed out in literature several
times.[25] Due to the limited quality of the refinements we refrain
from discussing interatomic distances (see Figures S8 and S9) in
detail. Nevertheless, the distances are very similar to those
observed for the pure MPTBs. The refinements do provide clear
information on the metal sites with rhodium/tungsten mixed
Table 2. Lattice parameter a[Å] of the metastable intermediate phases with ReO3-like XRPD pattern as a function of temperature [°C] during formation of
the different (Rh,W)-MPTBs.
600 700 750 800 1000
(Rh1/6W5/6O3)8(PO2)4not det. 3.786(8) 3.783(7) not det. not det.
(Rh1/9W8/9O3)12(PO2)43.792(9) 3.785(7) not det. 3.776(3) 3.713(7)
(Rh2/21W19/21O3)14(PO2)43.780(5) 3.781(6) not det. 3.776(4) 3.718(7)
Figure 3. Crystals of (Rh1/6W5/6O3)8(PO2)4(left, middle) and (Rh2/21W19/21
O3)14(PO2)4(right) obtained by CVT.
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occupancy. In addition, the refinements for both (Rh,W)-MPTB
suggest slightly higher tungsten content than expected for the
ideal compositions with rhodium(III) and tungsten(VI):
(Rh0.15W0.85O3)8(PO2)4instead of (RhIII1/6WVI5/6O3)8(PO2)4(m=4)
and (Rh0.07W0.93O3)12(PO2)4instead of (RhIII2/21 WVI19/21O3)14(PO2)4
(m=7); Table 3, Table 4, and Table 5. Details on the refinements
are given in the Experimental Section. Graphical representations
of the two crystal structures are given in Figure 4. Both show
ReO3-like slabs, which are four octahedra wide for the m=4
phase and seven for the phase at m=7. These slabs are linked
by phosphate tetrahedra. In both structures the [MO6] octahe-
dra joining the ReO3-like slabs together are linked to three [PO4]
tetrahedra and they are exclusively occupied by tungsten.
These are sites M2 in the m=4 phase and M3 in the m=7
phase (see Table 4 and Table 5; numbering of atom sites as in
the original papers on the pure tungsten MPTBs). In contrast,
[MO6] with only one or no adjacent phosphate group are partly
occupied by rhodium. For the m=7 phase even a systematic
increase of Rh3+occupancy with increasing distance from the
phosphate tetrahedra (from the interface between the ReO3-like
slabs) is observed. This cation ordering is rather surprising since
valence sum considerations would suggest just the opposite
ordering scheme for Rh3+/W6+, as is shown by the following
considerations along the lines of Paulings rules and Browns
equal valence rule.[27] In the crystal structures of the mono-
phosphate tungsten bronzes all oxygen atoms are twofold
coordinated (P+W, P+Rh, W+W, W+Rh, Rh+Rh). Assuming
ideal valence distribution within the coordination polyhedra
[PO4] (vP-O =5/4), [WO6] (vW-O =6/6), and [RhO6] (vRh-O =3/6) leads
to “overbonded” oxygen when coordinated by P+W (ΣvO=9/
4). For W+W (ΣvO=12/6), P+Rh (ΣvO=7/4), W+Rh (ΣvO=9/6),
Rh+Rh (ΣvO=6/6) the valence sum for oxygen drops from ideal
to strongly “underbonded”. Allowing slight alteration of
interatomic distances would result in some relaxation.[28]
However, exchanging tungsten by rhodium in [MO6] octahedra
linked to phosphate would already avoid all unfavorable
valence sums for oxygen, i.e. those in contrast to Paulings rule
of preservation of local electroneutrality.[27] Yet, this is not
observed. One explanation might lay in an additional contribu-
tion to lattice energy from charge density modulation along the
crystallographic c-axis in these structures. In other words, slabs
with over bonded and under bonded oxygen (surplus of
positive and negative charges, respectively) would stack along
the crystallographic c-axis.
All crystals of (Rh1/9W8/9O3)12(PO2)4(m=6) selected for SXRD
structure analysis showed diffuse streaks in sections of the
reciprocal space (see Figure S10). No reasonable integration of
the reflections was possible. We relate this problem to the
presence of severe stacking faults and variable thickness of the
ReO3-like slabs.
Table 3. Summary on data collection and refinement of the crystal
structures of (Rh0.15W0.85O3)8(PO2)4and (Rh0.07W0.93O3)14(PO2)4.
Empirical formula Rh1.33W6.67P4O32 Rh1.33W12.67P4O50
Structural formula (Rh0.167W0.833O3)8(PO2)4(Rh0.095W0.905O3)14(PO2)4
Refined formula (Rh0.146W0.854O3)8(PO2)4Rh1.04W12.96P4O32
Formula weight 2012.40 3413.47
Crystal system orthorhombic monoclinic
Space group P212121(no. 19) P21/n(no. 14)
T(K); λ(Å) 293(2); 0.71073 293(2); 0.71073
a(Å)[a] 5.2232(3) 5.2510(4)
b(Å)[a] 6.4966(3) 6.4949(5)
c(Å)[a] 17.3819(9) 26.6854(19)
β(°)[a] 90 90.30(1)
Z1 1
V 3); Dcalc (gcm3) 589.82(5); 5.665 910.09(12); 6.228
Crystal dimensions
(mm3); color
0.055×0.03×0.03;
dark green
0.068×0.042×0.021;
dark green
F(0 0 0) 874 1466
Absorption semi-empirical
(multiscan)[24]
semi-empirical
(multiscan)[24]
μ(mm1); ext. coef. 33.648; 0.0026(2) 40.453; 0
Measured refls. ind. 10119; 1714 7312; 2074
No. of parameters 58 100
Theta range (°) 3.35–29.91 3.05–27.59
Index ranges 7h7, 9k9,
24l23 6h6, 7k8,
34l33
GooF 1.108 1.131
Rint 0.0653 0.1217
R1[I>2σ(I)] 0.0315 0.0600
R1; wR2(all data) 0.0374; 0.0742 0.0649; 0.1687
[a] Lattice parameters from single-crystal measurement.
Table 4. (Rh1/6W5/6O3)8(PO2)4. Atomic coordinates and isotropic displace-
ment parameters.
Atom x y z s. o. f. Ueq 2]
W1 0.2502(2) 0.41042(6) 0.04236(2) 0.708(6) 0.0142(2)
Rh1 0.2502(2) 0.41042(6) 0.04236(2) 0.292(6) 0.0142(2)
W2 0.25049(15) 0.24727(5) 0.37161(2) 1 0.00929(12)
P 0.2478(10) 0.0604(3) 0.18620(11) 1 0.0079(4)
O1 0.963(2) 0.2898(14) 0.0006(6) 1 0.018(2)
O2 0.213(3) 0.2505(13) 0.1383(5) 1 0.026(2)
O3 0.228(2) 0.1205(10) 0.2701(4) 1 0.016(2)
O4 0.033(2) 0.0487(15) 0.4064(5) 1 0.017(2)
O5 0.532(2) 0.1202(15) 0.4044(5) 1 0.018(2)
O6 0.549(2) 0.399(2) 0.3281(6) 1 0.025(2)
O7 0.022(2) 0.477(2) 0.3288(6) 1 0.022(2)
O8 0.281(2) 0.4091(12) 0.4599(4) 1 0.021(2)
Table 5. (Rh2/21W19/21O3)14(PO2)4. Atomic coordinates and isotropic displace-
ment parameters.
Atom x y z s. o. f. Ueq 2]
W1 0 0.5 0 0.822(16) 0.0222(5)
Rh1 0 0.5 0 0.178(16) 0.0222(5)
W2 0.0011(4) 0.16144(13) 0.11289(3) 0.954(12) 0.0146(4)
Rh2 0.0011(4) 0.16144(13) 0.11289(3) 0.046(12) 0.0146(4)
W3 0.0001(3) 0.00523(11) 0.32958(2) 1 0.0088(3)
W4 0.0020(5) 0.32824(14) 0.44491(3) 0.875(13) 0.0200(4)
Rh4 0.0020(5) 0.32824(14) 0.44491(3) 0.125(13) 0.0200(4)
P1 0.506(2) 0.3156(7) 0.29117(17) 1 0.0084(9)
O1 0.553(4) 0.018(6) 0.0033(18) 0.5 0.010(7)
O2 0.540(4) 0.158(2) 0.5602(6) 1 0.019(4)
O3 0.039(4) 0.167(2) 0.3847(6) 1 0.021(4)
O4 0.038(4) 0.012(3) 0.1772(6) 1 0.024(4)
O5 0.485(6) 0.381(2) 0.2375(6) 1 0.023(3)
O6 0.206(5) 0.133(4) 0.4713(9) 1 0.039(6)
O7 0.709(4) 0.212(4) 0.4725(8) 1 0.030(5)
O8 0.301(4) 0.043(3) 0.0871(7) 1 0.019(4)
O9 0.795(4) -0.028(3) 0.0892(8) 1 0.025(4)
O10 0.286(4) 0.312(3) 0.1476(8) 1 0.025(5)
O11 0.780(4) 0.364(3) 0.1491(7) 1 0.018(4)
O12 0.229(3) 0.227(3) 0.3022(7) 1 0.018(4)
O13 0.694(4) 0.157(3) 0.2979(8) 1 0.021(4)
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Electron microscopic investigation
SAED pattern and HRTEM images taken from crushed crystals of
(Rh0.15W0.85O3)8(PO2)4and (Rh0.07W0.93O3)14(PO2)4are displayed in
Figure 5. The lattice parameters derived from both SAED
patterns accord well with the values obtained from XRD. No
hints were found for the presence of superstructures.
The HRTEM images are in agreement with the structure
models deduced from SXRD refinement, as it can be seen from
overlaying a structural image based on coordination polyhedra
(Figure 5). The characteristic fish-bone pattern with rows of
ReO3-like slabs and phosphate groups in between are nicely
matched. A prominent characteristic of these MPTB structures
are the pentagonal tunnels, which are formed between the
ReO3-slabs and phosphate groups and display a better white-
contrast every second time along [001]. In previous electron-
microscopic studies this effect was also observed and inves-
tigated. The contrast in MPTB’s is very sensitive to crystal tilting
near [100] and the crystal thickness.[29] The varying contrast
therefore can be explained with a slight misalignment to the
zone axis [100] and an unfavorable crystal size.
Images taken with lower magnifications show highly
ordered ReO3-like slabs with equal thickness, therefore, provid-
ing no hints on stacking faults. This result disagrees with the
observation, that the intensities of the reflections (0 0 2) and (0
0 4) (see Tables S4–S7 and Figures S1–S4) calculated from SXRD
data differ from the observed intensities of the XRPD data. It is
also in contrast to the observation of significant diffuse
scattering observed by SXRD for all (Rh,W)-MPTB. Several
explanations are possible: Stacking faults occur in some crystals
only and are not seen in the areas investigated by HRTEM or
the ratio of rhodium/tungsten differs between ReO3-like slabs
within a crystal.
Electronic spectra and magnetic behavior of the (Rh,W)-MPTB
Powders of the (Rh,W)-MPTBs (m=4 and 7) are dark green in
contrast to the orange-yellow of Rh(PO3)3(C-type; [RhIIIO6]
chromophore), which we discuss here as reference material. The
color difference is in line with powder reflectance measure-
ments of the three compounds shown in Figure 6. For Rh(PO3)3
the two strong absorption bands at 21500 cm1and
28000 cm1can be assigned to the ligand field transitions
1A1!1T1g and 1A1g!1T2g of the octahedral [RhIIIO6] chromophore.
Graphical evaluation according to Tanabe and Sugano[30] results
in B=430 cm1and Δ=23200 cm1. These values are in good
agreement with those determined for the [RhIIIF6] chromophore
in K3RhF6(B=460 cm1,Δ=22300 cm1).[31] In contrast to
Rh(PO3)3and K3RhF6the (Rh,W)-MPTBs show a broad absorption
band in the NIR/vis ranging from 5000 cm1to 14000 cm1and
a second in the vis/UV ranging from 19000 cm1to 29000 cm1
(see Figure 6). The minimum around 17000 cm1readily
explains their green color. The absorption in the NIR/vis is
reminiscent to those observed for blue heteropolytungstates,[32]
mixed-valent tungsten oxides, e.g. WO3-δ,[33] W20O58[34] or for
electrochromic tungsten bronzes, e.g. NaxWO3[35] and might
thus point to the presence of some W5+besides W6+and Rh3+.
The ligand-field transitions for the [RhIIIO6] chromophore are not
resolved in the (Rh,W)-MPTBs, most likely they are super-
imposed by LMCT (O2!W6+).
Angular overlap modelling (AOM)[36] has been used to
reproduce the d-electron energy levels of Rh3+in Rh(PO3)3. For
the AOM calculations the PC program CAMMAG[37] in a modified
version[38] was used. Best fit AOM parameters obtained from the
optical spectrum of Rh(PO3)3are B=490 cm1(β=0.80), C=
1960 cm1,ζ=1408 cm1,eσ(RhO) ~ d(RhO)5.0 and
eσ(RhO)max =11300 cm1. Isotropic π-interaction RhO was
assumed to be 1/4 of the corresponding σ-interaction
{eπ(RhO)=1/4 eσ(RhO}. As can be seen from the comparison
in Figure 6, results from AOM match well with the observed
energies for the transitions 1A1g!3T1g,1A1g!3T2g,1A1g!1T1g, and
1A1g!1T2g of the [RhIIIO6] chromophore.
For RhIII(PO3)3and the (Rh,W)-MPTBs with the ideal compo-
sitions (RhIII1/6WVI5/6O3)8(PO2)4and (RhIII2/21WVI19/21O3)14(PO2)4one
could expect diamagnetic behavior due to the d0configuration
of W6+and the 1A1g electronic ground state of Rh3+(d6,low-
spin). However, considering a second-order Zeeman effect for
Figure 4. Crystal structures of (Rh1/6W5/6O3)8(PO2)4(left) and (Rh2/21W19/21O3)14(PO2)4(right) with schematic coordination polyhedra. Projections along [100]; dark
grey: phosphate tetrahedra; grey: WO6octahedra; light grey: octahedra MO6with mixed occupancy Rh/W (graphics software DIAMOND v.4.5.1.[26])
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Rh3+would lead to a small magnetic moment independent of
temperature (TIP) according to van Vleck’s equation.[39] Indeed,
this expectation is perfectly met by the temperature independ-
ent susceptibility observed for Rh(PO3)3,χTIP = +
100·106emu·mol1(Figure 7). This value is also in agreement
with measurements for Rh3+(e.g. RhCl3:χTIP = +85·106
emu·mol1;[40] Rh2(SO4)3·12 H2O: χTIP = +95·106emu·mol1;[40]
[Rh3O(CH3COO)6(py)3]ClO4:χTIP = +280·106emu·mol1;[41] all χ
per formula unit). Furthermore, the results from angular overlap
modelling that already matched the excited state energies for
the [RhIIIO6] chromophore are fully consistent with the observed
TIP for rhodium(III) metaphosphate (Figure 7). In contrast, the
(Rh,W)-MPTBs show much higher molar susceptibilities
(χTIP(Rh1.164W6.836P4O32)= +299·106emu·mol1,
χTIP(Rh1.04W12.96P4O32)= +470·106emu·mol1;both obtained
from a linear fit to the respective graphs of χmol ·Tvs. Tshown in
Figure S11, plot of μeff vs. Tsee Figure S12) which cannot be
rationalized on basis of the exclusive presence of [RhIIIO6]
(Figure 7).
Figure 5. Top: Selected area electron diffraction (SAED) pattern of (Rh1/6W5/6O3)8(PO2)4(a) and (Rh2/21W19/21O3)14(PO2)4(c) in [1 0 0] zone axis orientation. Bottom:
Fourier-filtered HRTEM image (CM30 T) of (Rh1/6W5/6O3)8(PO2)4(b) and (Rh2/21W19/21O3)14(PO2)4(d) in [1 0 0] zone axis orientation with overlaid structure of the
MPTBs.
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Subtracting χTIP(Rh3+)= +100·106emu·mol1from χmol, exp
of the (Rh,W)-MPTBs still leaves for both significant contribu-
tions to the overall magnetic susceptibility. Two explanations,
both related to the presence of W5+(d1electronic system, 2T2g
electronic ground state for the octahedral chromophore [W5+
O6]), appear to be possible. Neither would lead to simple Curie-
Weiss-behavior. Magnetic behavior of sodium tungsten bronzes
NaxWO3might serve as comparison.[42] Therein reported
susceptibilities, due to the Pauli paramagnetism[43] of delocal-
ized electrons, are far too small to provide a reasonable
explanation for the TIP of the (Rh,W)-MPTBs. A second approach
for understanding might be based on the paramagnetism of
localized electrons in W5+. Yet, due to strong spin-orbit
coupling and the wide variability of ligand field effects in 5d
ions predictions on the paramagnetic behavior of W5+contain-
ing compounds are hard to make. Comparison to simple,
magnetically well characterized systems (e.g. CsWVF6[44],
CsWVCl6[45]) suggests a rather high content of up to 50% W5+of
the total tungsten content of the (Rh,W)-MPTBs. This seems to
be unrealistically high by any means. Given the overall rather
small susceptibilities of the (Rh,W)-MPTBs leaves eventually just
the assumption of contributions of unidentified paramagnetic
impurities as explanation. In this context it is worth noting that
magnetic susceptibility data obtained for two batches of the
(Rh,W)-MPTB at m=4 (powder synthesis and crushed crystals
from CVT) were almost identical. Clearly, characterization of the
electronic structure of the (Rh,W)-MPTBs requires additional
work, which is ongoing.
Chemical composition of the (Rh,W)-MPTBs
Seemingly, different experimental data (synthesis, SXRD, optical
spectroscopy, magnetic measurements) for the (Rh,W)-MPTBs
suggest different chemical composition for these phases. Thus,
a critical review of these data with respect to the chemical
composition of the phases under investigation is justified.
Syntheses based on the ideal compositions (exclusively Rh3+
and W6+) (Rh1/6W5/6O3)8(PO2)4(phase at m=4) and (Rh2/21W19/
21O3)14(PO2)4(phase at m=7) led to single phase powder
samples according to XRPD analysis of the solid reaction
products. By-phases as consequence of deviations in composi-
tion will only be observable for an estimated amount higher
than 3%wt.
Structure refinements from SXRD data suggest small
deviations from the ideal Rh/W ratio with slightly higher
tungsten content than expected. Even though there is some
correlation between site occupancy factors for Rh/W and the
corresponding displacement parameters, we believe that the
rhodium content of the two (Rh,W)-MPTBs is indeed slightly
lower than expected for the ideal composition. Yet, the
composition from SXRD might be regarded as the lower limit of
rhodium content. While no hints on stacking faults in the
(Rh,W)-MPTBs were obtained from HRTEM and SAED, diffuse
scattering observed in SXRD patterns point to such defects
which possibly will lead to deviations in stoichiometry.
Color and powder reflectance spectra of the (Rh,W)-MPTBs
are strikingly different than what is observed for the perfectly
stoichiometric and electronically well-defined metaphosphate
RhIII(PO3)3. Strong bands in the NIR/vis region suggest mixed-
valency W5+/W6+, yet already less than 1% of W5+would be
sufficient to cause such an absorption behavior, as is evidenced
by the deep blue color of under-stoichiometric WO3-δ.[33,34]
Magnetic susceptibility data of (Rh1/6W5/6O3)8(PO2)4and (Rh2/
21W19/21O3)14(PO2)4do show, as expected, weak paramagnetism.
Figure 6. Powder reflectance spectra of (Rh1/6 W5/6O3)8(PO2)4(top) and
(Rh2/21W19/21O3)14(PO2)4(middle) diluted with BaSO4(50:50 ratio) in compar-
ison to a spectrum of pure Rh(PO3)3C-type (bottom). Ticks at the bottom are
representing zero-phonon excitations for Rh(PO3)3from the best fit angular
overlap modelling (AOM; see text).
Figure 7. Molar (per formula unit) magnetic susceptibilities of
Rh1.164W6.836P4O32 (m=4), Rh1.04W12.96P4O32 (m=7) and Rh(PO3)3in a field of
104G.
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Yet, the absolute numbers cannot be rationalized solely based
on the TIP expected for Rh3+.
Results from EDS analyses (see Table 6) of crystals from CVT
seem also to indicate a slightly smaller ratio Rh/W than related
to the ideal compositions of the (Rh,W)-MPTBs. Yet, these
analyses (including a ZAF correction) overestimate the light
elements (phosphorus content) and underestimate heavy
elements (Rh, W).
Summarizing these critical considerations, we believe that
the obtained (Rh,W)-MPTBs do indeed show a slightly lower
ratio Rh/W than that of the “ideal” compositions. Clearly, these
phases do contain a small but significant amount of W5+.
Structural investigations did not give any hint on variations of
the metal/phosphorus ratio in the (Rh,W)-MPTBs.
Conclusions
In extension of previous work it is shown that in MPTBs
(WO3)2m(PO2)4substitution of W5+by appropriate combinations
of Rh3+(or Ir3+) and W6+is possible. Thus, new mm-MPTBs with
the ideal compositions (Rh1/6W5/6O3)8(PO2)4, (Rh1/9W8/9O3)12(PO2)4,
(Rh2/21W19/21O3)14(PO2)4(m=4, 6, 7) and (Ir1/6W5/6O3)8(PO2)4(only
m=4) were obtained.
Solution combustion synthesis with subsequent annealing
of the combustion products provides access to these new mm-
MPTBs. Furthermore, the progress of phase formation during
annealing (amorphous!ReO3-related phase!two-phase off-
equilibrium mixtures!mm-MPTB equilibrium phase) allows a
unique glimpse into the processes related to stepwise crystal-
lization and equilibration of an amorphous, solid starting
material. Thermodynamically metastable mixed-metal phos-
phates with ReO3-related XRPD pattern were established as
single-phase intermediates. Their formation emphasizes the
hitherto not recognized versatility of SCS for synthesis of
thermodynamically metastable solids.
Thermal decomposition behavior of the (Rh,W)-MPTBs is in
agreement with only a rather small stabilization of these phases
relative to W2O3(PO4)2, WO3, and Rh2O3and the thermal
decomposition products thereof WO3, Rh and gaseous P4O10.
Therefore, crystallization of the (Rh,W)-MPTBs by chemical vapor
transport (transport agent chlorine) is possible.
Structure refinement of the (Rh,W)-MPTBs at m=4 and 7
show cation distributions Rh/W that are in contrast to Paulings
electroneutrality rule. An overall stabilization due to alternating
layers with small positive/negative charges could be a reason.
Optical spectra and magnetic behavior of the obtained
(Rh,W)-MPTBs suggest mixed-valency W5+/6+and, as a conse-
quence, a small tungsten surplus with respect to the ideal
formulae. Eventually, in the course of our investigation on the
(Rh,W)-MPTBs a ligand field analysis for C-type Rh(PO3)3based
on powder reflectance and magnetic measurements has been
carried out as reference for the chromophore [RhIIIO6].
Experimental Section
X-ray powder diffraction.Powder diffraction pattern for phase
identification and purity control were recorded at ambient
temperature using an imaging plate (IP) Guinier camera (HUBER
G670, Cu-Kα1radiation, λ=1.54059 Å, 15 minutes exposure time
in the angular range 4°2θ<100°). The observed powder
diffraction pattern of (Rh1/6W5/6O3)8(PO2)4, (Rh2/21W19/21O3)14(PO2)4,
(Rh1/9W8/9O3)12(PO2)4and (Ir1/6W5/6O3)8(PO2)4are compared to
simulations which are based on the data from single crystal
structure analysis or isotypic compounds with matched lattice
parameters and a suitable chemical composition (Figure 1).
Tables containing the assigned reflections from the Guinier
photograph are available online as Supplementary Material
(Table S1–4).
Single-crystal X-ray diffraction.Suitable crystals of (Rh1/6 W5/6
O3)8(PO2)4and (Rh2/21W19/21O3)14(PO2)4were selected carefully
under a polarizing microscope and glued to glass fibers.
Diffraction data (graphite-monochromated Mo-Kα1 radiation; λ=
0.71073 Å) were collected using a Bruker Nonius k-CCD area-
detector diffractometer (BRUKER AXS B.V., Delft, Netherlands)
which was controlled by the Nonius “Collect” software.[46] For
data processing the software package “HKL2000: Denzo &
Scalepack” was employed.[47] A semi-empirical absorption correc-
tion based on multiscans was applied to the diffraction data
using the program package Platon.[48]
(Rh1/6W5/6O3)8(PO2)4: Starting parameters for the structure refine-
ment were obtained by the dual space structure solution algorithm
(SHELXT[49]) and refined with a full-matrix least-squares technique
(SHELX-97,[50] WinGX[51]). Space group P212121as for the pure
tungsten MPTB (WO3)8(PO2)4[14] was assumed. The two independent
metal sites were in a first step treated as fully occupied by tungsten.
Site W1 (notation as given in literature[14] for (WO3)8(PO2)4) showed
in contrast to W2 a rather large displacement parameter. In the
next refinement step for site M1 mixed occupancy W/Rh was
assumed. Refinement was carried out using the EXYZ and EADP
constraints for W/Rh on site M1 and assuming full occupancy. No
hint was found for mixed occupation of site M2. The refinement led
to 1.17 Rh and 6.83 W in the unit cell instead of 1.33 Rh and 6.67 W,
as it was expected from charge neutrality (Rh3+, W6+) consider-
ations. It should be noted in this context that any effort to constrain
the ADPs for sites M1 and M2 yielded significantly higher rhodium
contents in the unit cell (e.g. 1.75 Rh; 6.25 W) but drastically worse
residuals. Eventually, anisotropic displacement parameters could be
introduced for sites M1 and M2. Phosphorus and oxygen could only
be refined isotropically, due to occurrence of physically mean-
ingless (“n.p.d.”) atomic displacement parameters. Racemic twin-
ning was accounted for and led to the volume ratio V1/V2=0.52(5).
The remaining highest electron density (1.82 e3) was found close
to O8 with similar residual electron density close to other oxygen
sites. We attribute these maxima to the limitations of the isotropic
refinement. The deepest minimum in electron density (2.78 e3)
was found close to site M1. It is interpreted as an effect of
discontinuation of the Fourier series. The flaws in this refinement
Table 6. Ideal and analytical composition of “(Rh1/6W5/6O3)8(PO2)4 (m=4)
and “(Rh2/21W19/21O3)14(PO2)4 (m=7).
m=4m=7
Rh [%] W [%] P [%] Rh [%] W [%] P [%]
ideal composition 11.11 55.56 33.33 7.41 70.37 22.22
SXRD 9.7(1) 57.0(1) 33.33 5.8(5) 72.(5) 22.22
EDS (REM)[a] 11.0(8) 50(2) 39(3) 7.1(6) 67(3) 26(2)
[a] Area measurement of single crystals
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(despite acceptable residuals R1=3.2%, wR2=7.4%) mirror those
reported for many other refinements of MPTB type compounds.
(Rh2/21W19/21O3)14(PO2)4: Starting parameters for the structure refine-
ment were obtained by Direct Methods (SHELX-97[50]). Space group
P21/nas for the isotypic MPTB (WO3)14(PO2)4[16] as assumed in the
refinement (full-matrix least-squares refinement: SHELX-97,[50]
WinGX[51]). Assuming full occupancy of the metal sites, three (W1,
W2, W4) out of four tungsten sites showed unusually high isotropic
displacement parameters. Therefore, except for site W3, mixed
occupancy Rh/W was introduced using the EXYZ and EADP
constraints for each of the three sites. Even after accounting for
twinning (mirror plane perpendicular to the crystallographic c-axis,
as reported in literature for (WO3)14(PO2)4[25]) refinement of aniso-
tropic displacement parameters was only possible for the metal
and phosphorus sites. Eventually, for oxygen atom O1 occupying
the Wyckhoff site 2da split position with half occupancy of the
general site 4ewas introduced. From the refinement 1.04 rhodium
and 12.96 tungsten in the unit cell were obtained in contrast to
1.33 Rh and 12.67 W for the ideal composition. The value of Rint =
0.12 indicates low quality of the diffraction data, which is typical for
many refinements of MPTB structures.
Electron microscopic investigation.TEM images were conducted on
a FEI-Philips CM30 T/LaB6microscope operated at 300 kV and
equipped with a Gatan CCD for image recording. The samples were
prepared by suspending a little amount in cyclohexane using an
ultrasonic bath, applying a drop of the dispersion on a holey
carbon film reinforced by a copper grid and evaporating the
solvent. Digital TEM images were processed using the Gatan Digital
Micrograph software.[52]
To get an image along the [100] zone axis, a suitable crystal was
tilted along dynamic electron diffraction (“Kikuchi-lines”) towards a
simulated pattern. A diffraction pattern was taken and evaluated to
confirm the zone axis, afterwards a HRTEM image was prepared.
The HRTEM images were Fourier filtered using the Gatan Micro-
scopy Suite. After an analysis of the real space distances, a model
from the SXRD solution could be superimposed over the HRTEM
image. EDS analysis were carried out on a Hitachi SU3800 with a
tungsten cathode operated at 10 kV. For quatification the EDAX
detector “Octane Elect Super EDS” (peltier element cooling) and a
ZAF correction were used. Results were obtained as mean values
from several examined single-crystals.
Electronic absorption spectroscopy.Powder reflectance spectra
were measured at room temperature using modified CARY-14 (UV-
region) and CARY-17 (vis/NIR-region) spectrophotometers (OLIS,
USA) equipped with integrating (Ulbricht) spheres. Four different
setups for measurement (step width, band width, scan rate,
detector) were applied to cover the range from 5000 cm1to
40000 cm1. In the UV range (200 nm–600 nm) 800 data points
(step width 0.5 nm, scan rate 1 nm · sec1, band width 0.6 nm), in
the visible range (300 nm–900 nm) 600 data points (step width
1.0 nm, scan rate 1 nm · sec1, band width 1.2 nm) and in the near-
infrared range (600 nm–2200 nm) 500 data points (step width
4 nm, scan rate 2 nm · sec1, band·width 5 nm) were recorded. For
detection in the UV/vis region a photomultiplier detector (PMT) was
used, in case of the vis region with an aperture width of 0.06 nm. In
the near-infrared region a semiconducting lead(II)sulfide detector
with variant gap widths (1.4 nm–2.2 nm) was utilized. The spectra
are represented as a ration of K/S vs. wavenumber (Kubelka-Munk
function).[53]
Magnetic measurements.Magnetic measurements were carried out
using a vibrating sample magnetometer (Quantum design, USA).
The strength of the external magnet field was 104Oe in the
temperature range from 2 K to 300 K. Magnetic susceptibilities
were measured during cooling and heating. At each temperature
step a series of ten measurements were taken. Only close to
ambient temperature, slight differences between the data obtained
on cooling or heating were observed. The susceptibility data shown
in Figure 7 have been corrected for capsule and diamagnetic
contributions.[54] Furthermore, a low content of ferromagnetic
impurity was corrected with a Honda-Owen plot. Therefore,
measurements with a different external field (0 to 20000 Oe) were
conducted at 150 and 300 K for all samples. All susceptibilities are
given for 1 mole (formula unit) of the compound. In case of the
MPTBs the sum formula according to SXRD was used.
Deposition Numbers 2062902 (for Rh0.15W0.85O3)8(PO2)4(phase at
m=4)), and 2062903 (for Rh0.07W0.93O3)12(PO2)4(phase at m=7))
contain the supplementary crystallographic data for this paper.
These data are provided free of charge by the joint Cambridge
Crystallographic Data Centre and Fachinformationszentrum Karls-
ruhe Access Structures service www.ccdc.cam.ac.uk/structures.
Acknowledgements
We thank Norbert Wagner for magnetic measurements, Nils
Kannengießer for measurements of the UV/vis/NIR spectra and
Volker Bendisch (all of Inorganic Chemistry at Bonn University) for
photographs of the single-crystals. Funding by BASF SE, coopera-
tive work and discussions throughout the cooperation project
“PGM Phosphates” are gratefully acknowledged. Open access
funding enabled and organized by Projekt DEAL.
Conflict of Interest
The authors declare no conflict of interest.
Keywords: Equilibrium relations ·MPTB ·Rhodium ·Iridium ·
Solid-state chemistry ·Solid-state structure
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Manuscript received: January 19, 2021
Revised manuscript received: March 10, 2021
Accepted manuscript online: March 12, 2021
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