Mc. Mccarthy et al., Laboratory detection of five new linear silicon carbides: SiC3, SiC5, SiC6, SiC7, and SiC8, ASTROPHYS J, 538(2), 2000, pp. 766-772
The rotational spectra of five highly polar linear silicon-carbon chains Si
Cn, n = 3 and 5-8, were detected by Fourier transform microwave spectroscop
y in a supersonic molecular beam among the products of a gas discharge thro
ugh silane and diacetylene; SiC3 was detected as well by conventional milli
meter-wave absorption spectroscopy in a large glow discharge through silane
and acetylene. The electronic ground state was found to be X(1)Sigma(+) fo
r those with even n and X(3)Sigma(-) for those with odd n, in agreement wit
h recent ab initio calculations. The rotational and centrifugal distortion
constants of all five molecules were determined to high accuracy, as were t
he spin-spin and spin-rotation coupling constants for triplet SiC3, SiC5, a
nd SiC7. A fairly steep increase in the magnitude of the spin-spin constant
with chain length, similar to that found previously for the C-n and CnO ch
ains, was observed for the present silicon carbides. Of the five new silico
n carbides, SiC3 is of particular astronomical interest because radio emiss
ion lines of the isomeric ground state, a compact rhomboidal ring, have rec
ently been detected in IRC+10216 and because this chain is calculated to po
ssess a large dipole moment of 4.8 D and to lie only 5 kcal mol(-1) above g
round. From the laboratory data, the most intense transitions of SiC3 can n
ow be calculated to better than 1 km s(-1) in equivalent radial velocity at
frequencies up to 300 GHz.