首页> 外文期刊>Journal of Crystal Growth >Strongl band gap narrowing in quasi-binary (GaSb)_1-x(InAs)_x crystals grown from melt
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Strongl band gap narrowing in quasi-binary (GaSb)_1-x(InAs)_x crystals grown from melt

机译:从熔体生长的准二元(GaSb)_1-x(InAs)_x晶体的能带隙变窄

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摘要

Large crystals of a quays-binary semiconductor alloy (gabs)_1-x(ins)_x with x=0.02-0.05 have been grown from melt for he first time. The family of quasi-binary crystals (gabs)_1-x(ins)_x grown and reported here are different from the conventional Ga_1-xIn_xAs_ySb_1-y quaternaries due to grown behavior and physical properties. Significant narrowing of the band gap was observed in these crystals compared to the conventional quaternary Ga_1-xIn_xAs_ySb_1-y (with x=y). With an InAs content of about 2-5 at /100, band gaps in the range of 0.6-0.65 eV have been demonstrated. The possible origins of the band gap narrowing (i.e., high bowing parameter) include chemical and structural alterations in the grown crystals, resulting from the association of Ga-Sb and In-As in the melt.
机译:首次从熔体中生长出具有x = 0.02-0.05的准二元半导体合金(gabs)_1-x(ins)_x的大晶体。由于生长行为和物理特性,此处生长和报道的准二元晶体(gabs)_1-x(ins)_x族不同于常规的Ga_1-xIn_xAs_ySb_1-y四元晶体。与常规四元Ga_1-xIn_xAs_ySb_1-y(x = y)相比,在这些晶体中观察到带隙显着缩小。当InAs含量为/ 100时约为2-5时,带隙在0.6-0.65 eV范围内。带隙变窄的可能起源(即高弯曲参数)包括生长的晶体中化学和结构的改变,这是由于熔体中Ga-Sb和In-As的缔合而引起的。

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