Abstract:Perovskites are of great technological and geological importance, in large part, due to their considerable compositional and structural flexibility. However, the formation of perovskites with neutral species on their A-sites is very unusual. The formation, phase transitions, and properties of [He 2 ][CaZr]F 6 , which is the first helium-containing perovskite to be made, are reported. It is likely that a large family of related materials can also be prepared. On compression in neon, the negative thermal expansi… Show more
“…The recent pressure-induced insertion of helium into the vacant A-site perovskite [CaZr]F 6 has attracted much interest and tantalized with the prospect that other members of this perovskite family could encapsulate this noble gas as well. , Because these experimental studies were unable to fully characterize the crystal structure of the [He] 2 [CaZr]F 6 phase above ∼1 GPa, we employed density functional theory (DFT) calculations to predict the most stable geometry at this pressure. The Fm3̅m→P21/c structural phase transition that occurs when [He] 2 [CaZr]F 6 is squeezed was found to be driven by a decrease in the pressure–volume term to the enthalpy.…”
Section: Discussionmentioning
confidence: 99%
“…57,58 The proclivity of helium incorporation into materials that contain hollow interstices was leveraged in the synthesis of the first heliumcontaining perovskite, [He] 2 [CaZr]F 6 , which was proposed as a gas storage material. 59,60 [CaZr]F 6 is a neutral hybrid double perovskite possessing vacant A-sites, and so, it is naturally porous. Helium could be inserted into the A-site cavities using mild pressures, with a solubility higher than in silica-glass or in cristobalite.…”
Section: ■ Introductionmentioning
confidence: 99%
“…It is not surprising that pressure causes this porous structure to undergo amorphization at a mere 0.5 GPa when neon is used as the pressure transmitting medium. 60 When helium is used as the pressure transmitting medium instead, the amorphization is delayed until ∼3.5 GPa, aided by an uptake of helium into the pores and accompanied by a phase transition of Fm3̅ m [He] 2 [CaZr]F 6 (Figure 1a) to an unknown space group (suggested to be either I4/m or P4/ mnc) above 1.8 GPa and at low temperature. 60 We found that the most stable phase at 1 GPa possessed the monoclinic P2 1 /c space group instead, and subsequent calculations showed that it was more stable than the proposed I4/m and P4/mnc phases (Figure S1).…”
Section: ■ Introductionmentioning
confidence: 99%
“…60 When helium is used as the pressure transmitting medium instead, the amorphization is delayed until ∼3.5 GPa, aided by an uptake of helium into the pores and accompanied by a phase transition of Fm3̅ m [He] 2 [CaZr]F 6 (Figure 1a) to an unknown space group (suggested to be either I4/m or P4/ mnc) above 1.8 GPa and at low temperature. 60 We found that the most stable phase at 1 GPa possessed the monoclinic P2 1 /c space group instead, and subsequent calculations showed that it was more stable than the proposed I4/m and P4/mnc phases (Figure S1). In the Fm m P c 3 2 / 1 transformation, the [CaZr]F 6 octahedra rotate in a way that resembles what would be expected for a transition to the P4/mnc spacegroup, with the main difference being an additional tilting along the cdirection that induces a staggered, rather than a linear, orientation of the He atoms within the channels, as shown in Figure 1b.…”
Evolutionary searches were employed to predict the most
stable
structures of perovskites with helium atoms on their A-sites up to
a pressure of 10 GPa. The thermodynamics associated with helium intercalation
into [CaZr]F6 under pressure, and the mechanical properties
of the parent perovskite and helium-bearing phase were studied via
density functional theory (DFT) calculations. The pressure–temperature
conditions where the formation of HeAlF3, HeGaF3, HeInF3, HeScF3, and HeReO3 is
favored from elemental helium and the vacant A-site perovskites were
found. Our DFT calculations show that entropy can stabilize the helium-filled
perovskites because the volume that the highly compressible noble
gas atom occupies within the perovskite pores may be larger than the
volume it adopts in its elemental form under pressure. We find that
helium incorporation will increase the bulk modulus of AlF3 from a value characteristic of tin (∼50 GPa) to one characteristic
of stainless-steel (∼160 GPa) and hinders the pressure-induced
rotation of its octahedra.
“…The recent pressure-induced insertion of helium into the vacant A-site perovskite [CaZr]F 6 has attracted much interest and tantalized with the prospect that other members of this perovskite family could encapsulate this noble gas as well. , Because these experimental studies were unable to fully characterize the crystal structure of the [He] 2 [CaZr]F 6 phase above ∼1 GPa, we employed density functional theory (DFT) calculations to predict the most stable geometry at this pressure. The Fm3̅m→P21/c structural phase transition that occurs when [He] 2 [CaZr]F 6 is squeezed was found to be driven by a decrease in the pressure–volume term to the enthalpy.…”
Section: Discussionmentioning
confidence: 99%
“…57,58 The proclivity of helium incorporation into materials that contain hollow interstices was leveraged in the synthesis of the first heliumcontaining perovskite, [He] 2 [CaZr]F 6 , which was proposed as a gas storage material. 59,60 [CaZr]F 6 is a neutral hybrid double perovskite possessing vacant A-sites, and so, it is naturally porous. Helium could be inserted into the A-site cavities using mild pressures, with a solubility higher than in silica-glass or in cristobalite.…”
Section: ■ Introductionmentioning
confidence: 99%
“…It is not surprising that pressure causes this porous structure to undergo amorphization at a mere 0.5 GPa when neon is used as the pressure transmitting medium. 60 When helium is used as the pressure transmitting medium instead, the amorphization is delayed until ∼3.5 GPa, aided by an uptake of helium into the pores and accompanied by a phase transition of Fm3̅ m [He] 2 [CaZr]F 6 (Figure 1a) to an unknown space group (suggested to be either I4/m or P4/ mnc) above 1.8 GPa and at low temperature. 60 We found that the most stable phase at 1 GPa possessed the monoclinic P2 1 /c space group instead, and subsequent calculations showed that it was more stable than the proposed I4/m and P4/mnc phases (Figure S1).…”
Section: ■ Introductionmentioning
confidence: 99%
“…60 When helium is used as the pressure transmitting medium instead, the amorphization is delayed until ∼3.5 GPa, aided by an uptake of helium into the pores and accompanied by a phase transition of Fm3̅ m [He] 2 [CaZr]F 6 (Figure 1a) to an unknown space group (suggested to be either I4/m or P4/ mnc) above 1.8 GPa and at low temperature. 60 We found that the most stable phase at 1 GPa possessed the monoclinic P2 1 /c space group instead, and subsequent calculations showed that it was more stable than the proposed I4/m and P4/mnc phases (Figure S1). In the Fm m P c 3 2 / 1 transformation, the [CaZr]F 6 octahedra rotate in a way that resembles what would be expected for a transition to the P4/mnc spacegroup, with the main difference being an additional tilting along the cdirection that induces a staggered, rather than a linear, orientation of the He atoms within the channels, as shown in Figure 1b.…”
Evolutionary searches were employed to predict the most
stable
structures of perovskites with helium atoms on their A-sites up to
a pressure of 10 GPa. The thermodynamics associated with helium intercalation
into [CaZr]F6 under pressure, and the mechanical properties
of the parent perovskite and helium-bearing phase were studied via
density functional theory (DFT) calculations. The pressure–temperature
conditions where the formation of HeAlF3, HeGaF3, HeInF3, HeScF3, and HeReO3 is
favored from elemental helium and the vacant A-site perovskites were
found. Our DFT calculations show that entropy can stabilize the helium-filled
perovskites because the volume that the highly compressible noble
gas atom occupies within the perovskite pores may be larger than the
volume it adopts in its elemental form under pressure. We find that
helium incorporation will increase the bulk modulus of AlF3 from a value characteristic of tin (∼50 GPa) to one characteristic
of stainless-steel (∼160 GPa) and hinders the pressure-induced
rotation of its octahedra.
“…35 No bonding interaction was ever observed involving a He atom, disregarding the heavily debated and still hypothetical He@adamantane case. 36–39 Besides the many attempts to actively bind Ng atoms, they can alternatively be inserted into fullerenes, boron cages and clathrates (confinement strategy), from which they don’t escape due to kinetic stabilization, 40–51 trapped in ionic solid-state-compounds or metals, 52–55 or adsorbed in metal organic frameworks (MOFs). 56,57 Numerous computational studies analyzed the capability of other (mostly hypothetical) cage structures, such as closo -borane derivatives, BN-clusters, etc.…”
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