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Spectral characteristics of low threshold microdisks

机译:低阈值微小的光谱特性

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Semiconductor microdisks present a device with interesting physics but without an obvious practical application. The 'conventional' microdisk structure uses a pedestal to hold the boundary of a semiconductor disk in air leading to essentially a parallel array of edge emitters. We form disks by epitaxial lift-off which opens up several possibilities, as, in the use of a disk as an evanescent wave, in plane waveguide filter in silica based waveguides or as arrays of vertical emitters by placing the disks on reflectors. Arrays are of thin (150-700 nm) semiconductor (InGaAsP, /spl lambda/g = 1.55 /spl mu/m at room temperature) disks and rings on glass substrates. To date work has concentrated on disk thickness /spl lambda//2n due to the microcavity effect of enhanced coupling of spontaneous emission to waveguide modes. We have measured lasing in disks with thickness significantly greater than /spl lambda//2n.
机译:半导体微小管提供具有有趣物理的设备,但没有明显的实际应用。 “传统”的Microdisk结构使用基座以将半导体盘的边界保持在空气中,该边界基本上是边缘发射器的平行阵列。我们通过外延升降机形成磁盘,其开辟了几种可能性,如在二氧化硅的波导的平面波导过滤器中,通过将磁盘放置在反射器上,在二氧化硅的波导中或作为垂直发射器的阵列中的平面波导。阵列具有薄(150-700nm)半导体(IngaASP,/ SPL Lambda / g = 1.55 / spl mu / m在室温下)磁盘和玻璃基板上的环。迄今为止工作集中在磁盘厚度> / SPL Lambda // 2n上,由于增强的自发发射到波导模式的耦合的微观效应。我们在厚度上测量了厚度明显大于/ SPL Lambda // 2n的磁盘。

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