| Home > Publications database > Elpasolite-type superstructures in inverse perovskite nitrides |
| Journal Article | IMPULSE-2025-00025 |
; ; ; ;
2024
Pergamon Press
Oxford [u.a.]
Please use a persistent id in citations: doi:10.1016/j.progsolidstchem.2024.100444
Abstract: We present a range of inverse perovskite nitrides with an elpasolite-type superstructure. (Ca3N0.682(9))Sn and (Ca3N0.559(7))Pb are variants of the previously described (Ca3N)Sn and (Ca3N)Pb which contain less nitrogen and crystallize in . (Ba3N0.5)Sn and (Ba3N0.5)Pb resemble the previously reported perovskites (Ba3Nx)Sn and (Ba3Nx)Pb, but with both the superstructure and octahedral tilting, resulting in space group . (Ca3N0.77(2))Si, (Ca3N0.669(6))Ge, (Sr3N0.5)Ge and (Ba3N0.5)Ge all crystallize in P21/n. Among these, only (Ca3Nx)Ge has been previously described as (Ca3N)Ge. (Ca3N0.77(2))Si is notably the first compound in which mutually isolated N3− and Si4− ions coexist. There also exists a version with composition (Ca3N0.86(6))Si, which crystallizes in the cubic perovskite aristotype structure with space group . Similarly, there are versions of (Sr3N0.5)Ge, (Ba3N0.5)Sn and (Ba3N0.5)Pb with elevated nitrogen contents, less strongly tilted octahedra and no apparent superstructure. Electronic structure calculations indicate a metallic nature of the title compounds, with rather narrow improper band gaps for the strontium and barium compounds.
Keyword(s): Chemical Reactions and Advanced Materials (1st) ; Chemistry (2nd) ; Crystallography (2nd)
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