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Site Preference of Rare Earth Doping in Palladium‐Iron‐Arsenide Superconductors
Author(s) -
Stürzer Christine,
Schulz Anne,
Johrendt Dirk
Publication year - 2014
Publication title -
zeitschrift für anorganische und allgemeine chemie
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.354
H-Index - 66
eISSN - 1521-3749
pISSN - 0044-2313
DOI - 10.1002/zaac.201400268
Subject(s) - palladium , arsenide , doping , crystallography , materials science , superconductivity , ionic radius , ionic bonding , crystal structure , chemistry , gallium arsenide , ion , condensed matter physics , catalysis , physics , biochemistry , optoelectronics , organic chemistry
The solid solutions (Ca 1– y RE y Fe 1– x Pd x As) 10 Pd z As 8 with RE = La, Ce, and Pr were synthesized by solid state methods and characterized by X‐ray powder diffraction with subsequent Rietveld refinements [(CaFeAs) 10 Pt 3 As 8 ‐type structure (“1038 type”), P $\bar{1}$ , Z = 1]. Substitution levels (Ca/ RE , Fe/Pd, and Pd/□) obtained from Rietveld refinements coincide well with the nominal values according to EDS and the linear courses of the lattice parameters as expected from the ionic radii. The RE atoms favor the one out of five calcium sites, which is eightfold coordinated by arsenic. This leads to significant stabilization of the structure, and especially prevents palladium over‐doping in the iron‐arsenide layers as observed in the pristine compound (CaFe 1– x Pd x As) 10 Pd z As 8 . While the stabilization energy is estimated to about 40 kJ · mol –1 by electronic structure calculations, the reason for the diminished Fe/Pd substitution through RE doping is still not yet understood. We suggest that the electrons transferred from RE 3+ to the (Fe 1– x Pd x )As layer makes higher palladium concentrations unfavorable. Anyway the reduced palladium doping enables superconductivity with critical temperatures up to 20 K (onset) in the RE doped Pd1038 samples, which could not be obtained earlier due to palladium over‐doping in the active iron‐arsenide layers.