The spontaneous emission of 3.3 µm light emitting diodes (LEDs) and lasers based on InAs alloys were studied as a function of hydrostatic pressure. An increase in light output with increasing pressure has been observed, with a general comparison of the performances of type I and type II structures given in terms of the radiative and non-radiative processes involved. The experimental results provide evidence that the socalled CHSH Auger process is insignificant in these devices. However, Auger recombination mechanisms are still shown to dominate the response of these type II LEDs in contrast to type I lasers where competing radiative processes appear more significant.
IntroductionThere is increasing interest in mid-infrared LEDs that operate in the 2 -5 µm spectral region. The main target of such devices is to provide sufficient output power for the development of selective, highly efficient optical gas sensors capable of identifying target gases such as CH 4 , CO 2 and CO. The alloy systems based on InAs substrate are promising materials for the fabrication of midinfrared light sources for such applications [1]. The principal challenges for efficient room temperature operation are to reduce non-radiative mechanisms such as Auger recombination processes [2 -4] .Hydrostatic pressure has been extensively used to study the recombination mechanisms that occur in semiconductor LEDs and laser structures [5]. However, this previous pressure work has been limited to wavelength ranges of interest for telecommunications applications [5]. Here we extend pressure studies into the mid-infrared wavelength region.In this work the LEDs and lasers were grown on InAs substrates by liquid phase epitaxy (LPE), with a conventional horizontal sliding boat immersed in ultra-pure hydrogen. The resulting samples were processed into mesa etched LEDs using standard photolithographic techniques [6]. In this investigation, light output was measured as a function of hydrostatic pressure at room temperature using He gas compressor [7].