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 in | Scientific reports Vol. 9; no. 1; p. 6835 |
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Main Authors | , , , , , , , |
Format | Journal Article |
Language | English |
Published |
London
Nature Publishing Group UK
02.05.2019
Nature Publishing Group |
Subjects | |
Online Access | Get full text |
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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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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 2045-2322 2045-2322 |
DOI: | 10.1038/s41598-019-43142-5 |