H2SiO
Silanone, X 1A1
Species tag 046519
Version1*
Date of EntryNov. 2012
ContributorH. S. P. Müller

The experimental lines are from
(1) S. Bailleux, M. Bogey, C. Demuynck, J.-L. Destombes, and A. Walters, 1994, J. Chem. Phys. 101, 2729.
The reported uncertainties of "better than 50 kHz" appear to be too conservative by far. We have used 20 kHz, which appears to be slightly conservative still. Watson's S-reduction was used here. Since DK was only slightly determined and rather small compared to an ab initio value, an estiamted value was kept fixed in the fit. Some closely spaced asymmetry doublets show essentially symmetric, fairly large deviations. These lines have been omitted from the fit here. The deviations may be caused by the Stark effect. Unresolved doublets were retained, but those with calculated splitting of more than 1 MHz were not merged. Predictions with uncertainties larger than 0.3 MHz should be viewed with caution. The data set is deemed to be sufficient for observational purposes.
The dipole moment is from an ab initio calculation by
(2) B. Ma and H. F. Schaefer III, 1994, J. Chem. Phys. 101, 2734.
At low temperatures, it may be necessary to discern between ortho-H2SiO and para-H2SiO. The ortho and para states are described by Ka being odd and even, respectively. The nuclear spin-weights are 3 and 1 for ortho-H2SiO and para-H2SiO, respectively. The JKaKc = 111 is the lowest ortho state. It is 6.1173 cm–1 above ground.
Separate para and ortho predictions are available up to J = 10 and Ka = 3 along with separate para and ortho partition function values. Note: the spin-weight of 3 for the separate ortho predictions has been eliminated.

Lines Listed679
Frequency / GHz< 1556
Max. J45
log STR0-5.3
log STR1-3.3
Isotope Corr.-0.0363
Egy / (cm–1)0.0
 µa / D3.82
 µb / D 
 µc / D 
 A / MHz166658.
 B / MHz18678.56
 C / MHz16743.60
 Q(300.0)7702.1212
 Q(225.0)5000.6894
 Q(150.0)2721.7623
 Q(75.00)963.3430
 Q(37.50)341.6950
 Q(18.75)121.2845
 Q(9.375)41.2095
 Q(5.000)13.7664
 Q(2.725)4.6786
detected in ISM/CSMno


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