𝔖 Bobbio Scriptorium
✦   LIBER   ✦

First High-Resolution Infrared Observation of the Symmetry-Forbidden ν5 Band of 10B2H6

✍ Scribed by J.-M. Flaud; Ph. Arcas; W.J. Lafferty; H. Bürger; G. Pawelke


Publisher
Elsevier Science
Year
2000
Tongue
English
Weight
161 KB
Volume
203
Category
Article
ISSN
0022-2852

No coin nor oath required. For personal study only.

✦ Synopsis


Spectra of 10 B monoisotopic diborane, B 2 H 6 , have been recorded at high resolution (2-3 ϫ 10 Ϫ3 cm Ϫ1 ) by means of Fourier transform spectroscopy in the region 700 -1300 cm Ϫ1 . A thorough analysis of the 18 a-type, 14 c-type, and 5 symmetryforbidden band has been performed. Of particular interest are the results concerning the 5 symmetry-forbidden band, which is observed only because it borrows intensity through an a-type Coriolis interaction with the very strong 18 infrared band located approximately 350 cm Ϫ1 higher in wavenumber. The 5 band has been observed around 833 cm Ϫ1 and consists of a well-resolved Q branch accompanied by weaker P-and R-branch lines. Very anomalous line intensities are seen, with the low K a transitions being vanishingly weak, and Raman-like selection rules observed. The determination of the upper state Hamiltonian constants proved to be difficult since the corresponding energy levels of each of the bands are strongly perturbed by nearby dark states. To account for these strong localized resonances, it was necessary to introduce the relevant interacting terms in the Hamiltonian. As a result the upper state energy levels were calculated satisfactorily, and precise vibrational energies and rotational and coupling constants were determined. In particular the following band centers were derived: 0 ( 5 ) ϭ 832.8496(70) cm Ϫ1 , 0 ( 14 ) ϭ 977.57843(70) cm Ϫ1 , and 0 ( 18 ) ϭ 1178.6346(40) cm Ϫ1 . (Type A standard uncertainties (1) are given in parentheses.


📜 SIMILAR VOLUMES


High-Resolution Infrared Study of the ν1
✍ R.L. Sams; T.A. Blake; S.W. Sharpe; J.-M. Flaud; W.J. Lafferty 📂 Article 📅 1998 🏛 Elsevier Science 🌐 English ⚖ 257 KB

Using high-resolution Fourier transform spectra, a thorough analysis of the 14 c-type, 17 a-type, and 18 a-type bands of both 11 B 2 H 6 and 10 B 11 BH 6 has been carried in the 10.3-, 6.2-, and 8.5-m spectral regions, respectively. From this analysis a large set of precise ground state combination

First Observation of the ν17–ν4 Differen
✍ J.-M. Flaud; W.J. Lafferty; H. Bürger; G. Pawelke; J.-L. Domenech; D. Bermejo 📂 Article 📅 2000 🏛 Elsevier Science 🌐 English ⚖ 141 KB

An analysis of the 17 -4 difference bands near 800 cm Ϫ1 of two isotopic species, 10 B 2 H 6 and 11 B 2 H 6 , of diborane has been carried out using infrared spectra recorded with a resolution of ca. 0.003 cm Ϫ1 . In addition, the 17 band of 10 B 2 H 6 has been recorded and assigned. Since this band

The High-Resolution Infrared Spectrum of
✍ F. Hegelund; H. Burger; O. Polanz 📂 Article 📅 1994 🏛 Elsevier Science 🌐 English ⚖ 477 KB

The gas-phase IR spectra of the fundamental band \(\nu_{5}\) around \(3100 \mathrm{~cm}^{-1}\) and the \(a, b\)-Coriolis interacting band systen \(\nu_{4}, \nu_{6}\) around \(1300 \mathrm{~cm}^{-1}\) of \(\mathrm{N}_{2} \mathrm{H}_{2}\) have been recorded with a resolution of ca. 0.008 and \(0.005 \

High-Resolution Infrared Study of the ν4
✍ F. Hegelund; H. Bürger; O. Polanz 📂 Article 📅 1996 🏛 Elsevier Science 🌐 English ⚖ 204 KB

The gas-phase IR spectra of the a,b-Coriolis interacting band system n 4 ,n 6 around 950 cm 01 and the n 5 band around 2300 cm 01 of N 2 D 2 have been recorded with a resolution of ca. 0.005 and 0.007 cm 01 , respectively. In the n 5 and n 6 bands both a-and b-type components are observed. In n 4 th

High-Resolution Infrared Spectra in the
✍ T.J. Cronin; X. Wang; G.A. Bethardy; David S. Perry 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 206 KB

High-resolution, infrared absorption spectra of the 6 (asymmetric C-H stretch) and 2 2 (H-C-H symmetric bend overtone) bands of jet-cooled CH 2 F 2 are reported with a sub-Doppler resolution of ϳ0.002 cm Ϫ1 . More than 600 transitions were observed in the range of 3002-3036 cm Ϫ1 , of which 268 were