“…b In the case of Cs 2 Au I Au III Cl 6 , a relation between computed EOS for both phases predicts a pressure-induced phase transition of ∼11.4 GPa that agrees with the measured 12 GPa (cf. Figure S1).…”
Section: Resultssupporting
confidence: 88%
“…The data points are represented by black circles, the red line is the profile (LeBail) fit. The pXRD analysis of all tested samples confirms the tetragonal structure of dicesium gold chloride as reported in refs and . All the diffraction peaks correspond to the tetragonal I 4 /mmm (no.…”
Section: Resultssupporting
confidence: 84%
“…The values of a and c do not change significantly in the series and are in good agreement with the reported literature. 37,39 An interesting feature is a preferential orientation effect observed for some of the samples. For a powderized sample with unoriented grains, the expected intensity ratio I(220)/I(112) is 0.34, whereas the observed I(220)/I(112) reaches 0.95 for Cs 2 Au 2 Cl 6 _1 and 2 for Cs 2 Au 2 Cl 6 _2.…”
Applied
cutting-edge electronic structure and phonon simulations
provide a reliable knowledge about the stability of perovskite structures
and their electronic properties, which are crucial for design of effective
nanomaterials. Gold is one of the exceptional elements, which can
exist both as a monovalent and a trivalent ion in the B site of a
double perovskite such as A2BIBIIIX6. However, until now, electronic properties of Cs2AuIAuIIIX6 have not been
sufficiently explored and this material was never synthesized using
Au1+ and Au3+ precursors in the preparation
route. Here, computational simulations combined with an experimental
study provide new insight into the properties and synthesis route
of Cs2AuIAuIIIX6 (X =
Cl, Br, and I) perovskites. First-principles calculations reveal that
tetragonal Cs2AuIAuIIIX6 (X = I, Br, Cl) molecules present a band gap of 1.10, 1.15, and
1.40 eV, respectively. Application of novel approaches in the simulations
of the VB-XPS for Cs2AuIAuIIICl6 allows replication of the observed spectrum and provides
strong evidence of the reliability of the obtained results for the
other perovskites Cs2AuIAuIIIX6, X = Br, I. Following theoretical findings, a one-step preparation
route of the Cs2AuIAuIIICl6 is developed using a combination of monovalent and trivalent gold
precursors at a relatively low temperature. It should be emphasized
that this is the first synthesis of this material at low temperatures,
allowing for obtaining highly crystalline Cs2Au2Cl6 particles with controlled morphology and without gold
impurities. The band gap of synthesized Cs2AuIAuIIICl6 is extended into the NIR spectral
range, where most other double perovskites are limited to higher energies,
limiting their usage in single junction solar cells or in photocatalysis.
The as-synthesized Cs2AuIAuIIICl6 exhibits high efficiency in a photocatalytic toluene degradation
reaction under visible light irradiation. The developed approach provides
information necessary for structure manipulation at the early stage
of its synthesis and offers a new and useful guidance for design of
novel improved lead-free inorganic halide perovskite with interesting
optical and photocatalytic properties.
“…b In the case of Cs 2 Au I Au III Cl 6 , a relation between computed EOS for both phases predicts a pressure-induced phase transition of ∼11.4 GPa that agrees with the measured 12 GPa (cf. Figure S1).…”
Section: Resultssupporting
confidence: 88%
“…The data points are represented by black circles, the red line is the profile (LeBail) fit. The pXRD analysis of all tested samples confirms the tetragonal structure of dicesium gold chloride as reported in refs and . All the diffraction peaks correspond to the tetragonal I 4 /mmm (no.…”
Section: Resultssupporting
confidence: 84%
“…The values of a and c do not change significantly in the series and are in good agreement with the reported literature. 37,39 An interesting feature is a preferential orientation effect observed for some of the samples. For a powderized sample with unoriented grains, the expected intensity ratio I(220)/I(112) is 0.34, whereas the observed I(220)/I(112) reaches 0.95 for Cs 2 Au 2 Cl 6 _1 and 2 for Cs 2 Au 2 Cl 6 _2.…”
Applied
cutting-edge electronic structure and phonon simulations
provide a reliable knowledge about the stability of perovskite structures
and their electronic properties, which are crucial for design of effective
nanomaterials. Gold is one of the exceptional elements, which can
exist both as a monovalent and a trivalent ion in the B site of a
double perovskite such as A2BIBIIIX6. However, until now, electronic properties of Cs2AuIAuIIIX6 have not been
sufficiently explored and this material was never synthesized using
Au1+ and Au3+ precursors in the preparation
route. Here, computational simulations combined with an experimental
study provide new insight into the properties and synthesis route
of Cs2AuIAuIIIX6 (X =
Cl, Br, and I) perovskites. First-principles calculations reveal that
tetragonal Cs2AuIAuIIIX6 (X = I, Br, Cl) molecules present a band gap of 1.10, 1.15, and
1.40 eV, respectively. Application of novel approaches in the simulations
of the VB-XPS for Cs2AuIAuIIICl6 allows replication of the observed spectrum and provides
strong evidence of the reliability of the obtained results for the
other perovskites Cs2AuIAuIIIX6, X = Br, I. Following theoretical findings, a one-step preparation
route of the Cs2AuIAuIIICl6 is developed using a combination of monovalent and trivalent gold
precursors at a relatively low temperature. It should be emphasized
that this is the first synthesis of this material at low temperatures,
allowing for obtaining highly crystalline Cs2Au2Cl6 particles with controlled morphology and without gold
impurities. The band gap of synthesized Cs2AuIAuIIICl6 is extended into the NIR spectral
range, where most other double perovskites are limited to higher energies,
limiting their usage in single junction solar cells or in photocatalysis.
The as-synthesized Cs2AuIAuIIICl6 exhibits high efficiency in a photocatalytic toluene degradation
reaction under visible light irradiation. The developed approach provides
information necessary for structure manipulation at the early stage
of its synthesis and offers a new and useful guidance for design of
novel improved lead-free inorganic halide perovskite with interesting
optical and photocatalytic properties.
“… a ARTEMIS program, S 0 2 = 0.84, AuCs 2 Cl 6 was accepted as initial model structure . Experimental spectra fits were performed in k -space if not indicated otherwise. b MSmultiple scattering, Au–Cl1–Au–Cl2. …”
Chloride-bearing
fluids are widespread in the Earth’s interior
from low-temperature subsurface conditions to deep lithosphere. The
concentration of chloride salts varies from diluted aqueous solutions
to concentrated brines and anhydrous (dry) chloride melts beneath
volcanoes. Here we report an investigation of the state of Au in hydrothermal
chloride fluids and anhydrous melts by means of in situ X-ray absorption
spectroscopy combined with ab initio molecular dynamics simulations
and thermodynamic modeling. The experiments included registration
of Au L3-edge X-ray absorption near edge structure/extended
X-ray absorption fine structure spectra of Au-bearing fluids in the
temperature range from 350 to 575 °C at pressures of 150–4500
bar. Spectra of Au dissolved in dry CsCl/NaCl/KCl + K2S2O8 melt were recorded at 650 °C. It was found
that Au is coordinated by two Cl atoms (R
Au–Cl = 2.25–2.28 Å). The alkali metal atoms (Me) were detected
in the distant coordination sphere of Au at R
Au‑Me = 3.3–4.1 Å. The alkali metal cations
in the vicinity of Au–Cl complex partly compensate the positive
charge located on Au and, by this way, affect the Au–Cl distance.
An increase of the fluid pressure causes expansion of the second coordination
sphere composed of the alkali metal cations, which leads to the increase
of the positive Au charge and results in slight contraction of the
first coordination sphere of Au. Accordingly, the transport of Au
in high-temperature chloride-bearing natural ore-forming fluids of
moderate to high densities (>0.3 g·cm–3)
can
be explicitly described by the formation of the AuCl2
– at any salt concentration from low-salinity fluids
to hydrosaline liquids and anhydrous melts. In general, this means
that the hydrothermal fluid chemistry simplifies with increasing temperature.
“…RbTlCl 3 , have very recently been discussed as new potential hosts for non-trivial electronic properties [9,10]. The structurally and electronically related compounds CsAuX 3 with X = Cl, Br, and I crystallize in the space group I 4/mmm in a distorted variation of the perovskite structure [11][12][13]. The gold atoms in CsAuX 3 are mixed valent with Au(I) and Au(III) centers, which occupy two different crystallographic sites at ambient conditions [14,15].…”
We report on high-pressure p ≤ 45 GPa resistivity measurements on the perovskite-related mixedvalent compound CsAuBr 3 . The compounds high-pressure resistivity can be classified into three regions: For low pressures (p < 10 GPa) an insulator to metal transition is observed; between p = 10 GPa and 14 GPa the room temperature resistivity goes through a minimum and increases again; above p = 14 GPa a semiconducting state is observed. From this pressure up to the highest pressure of p = 45 GPa reached in this experiment, the room-temperature resistivity remains nearly constant. We find an extremely large resistivity reduction between ambient pressure and 10 GPa by more than 6 orders of magnitude. This decrease is among the largest reported changes in the resistivity for this narrow pressure regime. We show -by an analysis of the electronic band structure evolution of this material -that the large change in resistivity under pressure in not caused by a crossing of the bands at the Fermi level. We find that it instead stems from two bands that are pinned at the Fermi level and that are moving towards one another as a consequence of the mixed-valent to single-valent transition. This mechanism appears to be especially effective for the rapid buildup of the density of states at the Fermi level. arXiv:1909.06874v1 [cond-mat.mtrl-sci]
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