Hole-doped layered
BiCuSeO phases include substitutionally doped
Bi1–x
A
x
CuSeO (A = alkali, alkaline earth) as well as vacancy-doped Bi1−δCu1‑γSeO and Bi1−δCuSeO. To probe how their Seebeck coefficients
are related to their hole density p, we calculated
the Seebeck coefficient for defect-free BiCuSeO as a function of the
hole density, which is generated by lowering the Fermi level from
the valence band maximum (VBM). In addition, we calculated the Seebeck
coefficient for Bi1−δCuSeO (δ = 1/32,
1/16) with a large number of Bi vacancies. The Seebeck coefficients
of the hole-doped BiCuSeO phases are governed by the electronic states
lying within ∼0.5 eV from the VBM. These states are composed
of largely Cu 3d xz/yz and Se 4p x/y states and possess the character
of a uniform one-dimensional (1D) chain rather than a uniform two-dimensional
(2D) lattice expected for a layered phase. The observed S-vs-p relationship for Bi1–x
A
x
CuSeO (A = alkali, alkaline earth)
as well as Bi1−δCu1‑γSeO (δ = 0, 0.025; γ = 0, 0.025) and Bi1−δCuSeO (δ = 0.0, 0.025) is very well reproduced by the calculated
relationship for defect-free BiCuSeO within the rigid band approximation.
The observed S-vs-p relationship
reflects the quantum confinement effect of uniform 1D chains, despite
that the hole-doped BiCuSeO phases consist of 2D layers, (Cu2Se2)2– and (Bi2O2)2+. The drastic decrease in the S values
of Bi1−δCuSeO with large δ (= 0.05,
0.075, 0.10) arises from the loss of the quantum confinement effect
in the (Cu2Se2)2– layers;
that is, the uniform 1D chain character is lost because of their geometry
distortion induced by a large number of Bi vacancies.
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