Abstract

Emission of visible light from forward and reverse biased silicon p-n junctions due to the radiative electron-hole recombination has been known since the mid-50s. The weak light emission was also seen from a silicon-dioxide dielectric in an integrated gate oxide capacitor formed between a polysilicon gate and an (n or p) well in an integrated circuit. The difference in carrier energies for each of these recombination mechanisms gives rise to a specific photon wavelength (energy) distribution in the visible range. All photoemitting events are characterized by a very low level light intensity due to the low quantum efficiency of about 10−5 - 10−4 photons per one electron-hole recombination.The first practical photoemission microscope was constructed by Khurana and Chiang. They took the advantage of the advances in night vision technology and used it for imaging the faint ("invisible") light coming from various silicon structures. A typical photoemission microscope consists of an x-y-z stage with the device holder, an optical microscope, a lightsensitive camera all set within a light-tight enclosure and a computer system for image acquisition and processing.

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