Giant bowing of the band gap and spin-orbit splitting energy in GaP1−xBix dilute bismide alloys

Using spectroscopic ellipsometry measurements on GaP 1− x Bi x /GaP epitaxial layers up to x  = 3.7% we observe a giant bowing of the direct band gap ( E g Γ ) and valence band spin-orbit splitting energy (Δ SO ). E g Γ (Δ SO ) is measured to decrease (increase) by approximately 200 meV (240 meV) wi...

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Published inScientific reports Vol. 9; no. 1; p. 6835
Main Authors Bushell, Zoe L., Broderick, Christopher A., Nattermann, Lukas, Joseph, Rita, Keddie, Joseph L., Rorison, Judy M., Volz, Kerstin, Sweeney, Stephen J.
Format Journal Article
LanguageEnglish
Published London Nature Publishing Group UK 02.05.2019
Nature Publishing Group
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Summary:Using spectroscopic ellipsometry measurements on GaP 1− x Bi x /GaP epitaxial layers up to x  = 3.7% we observe a giant bowing of the direct band gap ( E g Γ ) and valence band spin-orbit splitting energy (Δ SO ). E g Γ (Δ SO ) is measured to decrease (increase) by approximately 200 meV (240 meV) with the incorporation of 1% Bi, corresponding to a greater than fourfold increase in Δ SO in going from GaP to GaP 0.99 Bi 0.01 . The evolution of E g Γ and Δ SO with x is characterised by strong, composition-dependent bowing. We demonstrate that a simple valence band-anticrossing model, parametrised directly from atomistic supercell calculations, quantitatively describes the measured evolution of E g Γ and Δ SO with x . In contrast to the well-studied GaAs 1− x Bi x alloy , in GaP 1− x Bi x substitutional Bi creates localised impurity states lying energetically within the GaP host matrix band gap. This leads to the emergence of an optically active band of Bi-hybridised states, accounting for the overall large bowing of E g Γ and Δ SO and in particular for the giant bowing observed for x  ≲ 1%. Our analysis provides insight into the action of Bi as an isovalent impurity, and constitutes the first detailed experimental and theoretical analysis of the GaP 1− x Bi x alloy band structure.
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ISSN:2045-2322
2045-2322
DOI:10.1038/s41598-019-43142-5