4-(trimethylsilyl)morpholine O(CHCH)NSi(CH) (TMSM) was investigated as a single-source precursor for SiCNO films synthesis. Optical emission spectroscopy of plasma generated from TMSM/He, TMSM/H, and TMSM/NH gas mixtures revealed the presence of N, CH, H, CN, and CO species. The last two are suggested to be responsible for the lowering of carbon concentration in the films in comparison with the precursor.
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