THE INFRARED DETECTION OF $HOSi^{+}$ AND $DOSi^{+}$

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1989

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Ohio State University

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The ν1 (O-H stretch) and ν3 (O-Si stretch) bands of HOSi+ have been observed, and molecular constants have been determined for both the upper and lower states of both bands. There is good agreement between our constants, and those calculated by Botschwina and Rosmus.1 We employed the difference frequency laser system to observe the ν1 band, whose origin is approximately 3660cm−1 and the diode laser to observe the ν3 band, whose origin is approximately 1130cm−1. Both bands were observed in a hollow cathode discharge, with approximately 15 kHz discharge modulation. The initial detection of the ion was made by discharging (CH3)3SiOH in a buffer of H2 and He, with high discharge current and water cooling. Later, it was discovered that better results could be obtained by mixing SiH4 and N2O with either H2 or H2 and He, with dry-ice and methanol cooling. It was not possible to observe HOSi+ with mixtures of SiH4 and H2O. We have observed several lines of the ν1 band of DOSi+ around 2700cm−1, but have no definitive assignment or molecular constants. This was produced in a similar manner to HOSi+, initially with (CH3)3SiOD in a buffer of D2 and He, and subsequently with SiH4 in a buffer of D2 and He. Attempts to observe the ν3 band of DOSi+ were unsuccessful.

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1 P. Botschwina and P. Rosmus. J. Chem. Phys. 82,1420 (1985).


Author Institution: Herzberg Institute of Astrophysics, National Research Council; Department of Chemistry, York University

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