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Photoluminescence and optical properties of plasma-deposited amorphous Si<sub> <i>x</i> </sub>C<sub>1–<i>x</i> </sub> alloys
180
Citations
21
References
1981
Year
Optical MaterialsEngineeringLuminescence EfficiencyOptoelectronic DevicesChemistryLuminescence PropertyCarbon ConcentrationElectronic DevicesOptical PropertiesCompound SemiconductorMaterials SciencePlasma DecompositionPhotoluminescenceOptoelectronic MaterialsSemiconductor MaterialElectronic MaterialsApplied PhysicsAmorphous SolidOptoelectronicsSolar Cell Materials
Abstract Results on the photoluminescence, optical properties and photoconductivity of amorphous Si : C : H alloys prepared from the plasma decomposition of silane and ethylene are presented. Films deposited at substrate temperatures of 30 and 300°C have been studied with compositions ranging from 100 to 10% silicon. The photoluminescence spectra measured at 77 and 300 K show considerable discrepancies with respect to previously reported results. The emission is in the form of a single band which broadens and shifts towards higher photon energies as the carbon concentration is increased. The highest emission-peak energy of 2·05 eV is achieved for samples with 90 at.% C. The temperature quenching of the luminescence is reduced with increasing carbon concentration. For 90% C specimens there is less than a factor of 2 reduction in emission intensity between 77 and 300 K. As a consequence visible (yellow–orange) room-temperature luminescence can be clearly observed with the naked eye. The luminescence efficiency is minimum in films of composition near Si0·5C0·5 but increased for both carbon- and silicon-rich alloys. The photoconductivity in hydrogenated a-SiC decreases rapidly as the carbon concentration is increased and there is also a pronounced broadening of the absorption edge indicative of a wider range of localized tail states. The results are discussed in terms of models proposed for a-Si : H. The relative influence of phonon-coupling and disorder on the shift and line-width of the luminescence spectra is considered. It is suggested that the increase in the threshold quenching temperature observed in C-rich alloys is predominantly a consequence of a stronger Coulomb interaction.
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