Four
novel ternary Zintl phase compounds belonging to the Ca11–x
RE
x
Sb10–y
(RE = La, Ce,
Nd, Sm; 0.18(4) ≤ x ≤ 0.43(2), 0.14(1)
≤ y ≤ 0.41(1)) system have been synthesized
by arc-melting, and the Ho11Ge10-type crystal
structure has been characterized for the isotypic title compounds
by both powder and single crystal X-ray diffraction analyses. The
intrinsically complex crystal structure is viewed as an assembly of
the three distinctively shaped cationic polyhedra built from either
seven or nine cations and the anionic frameworks constructed by the
“dumbbell-shaped” Sb2 and the “square-shaped”
Sb4 moieties. All of the four trivalent rare-earth metals
were successfully introduced as n-type dopants to
partially substitute divalent Ca atoms in the parental compound Ca11Sb10, which resulted in generating two or three
Ca2+/RE3+ mixed-cationic sites. In particular,
during these substitutions, we observed a unique site preference of
Ca2+ and RE3+ among four available cationic
sites, where the rare-earth metals with the higher electronegativities
than Ca occupied particular atomic sites having the higher Q values.
This type of site preference was conclusively explained by theoretical
investigations using the tight-binding linear muffin-tin orbital method.
Despite the successful n-type doping, the increased
electrical conductivities σ and the decreased Seebeck coefficients S of Ca10.75(3)Nd0.25Sb9.82(1) and Ca10.82(4)Sm0.18Sb9.86(1) compared to those of Ca11Sb10 still presented the p-type rather than n-type characters. These unexpected behaviors should be
attributed to ca. 7–20% of Sb3 deficiencies found at the “square-site”
(Wyckoff 8h), which spontaneously occurred to reduce
an energetically unfavorable antibonding character of the interatomic
interaction between two Sb3 atoms at the square-site. Total and partial
density of states of a hypothetical structural model Ca10.5Nd0.5Sb10, an SEM image of single
crystals of Ca10.57(2)La0.43Sb9.59(1), and a TGA result of Ca10.82(4)Sm0.18Sb9.86(1) are also provided.