𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Solvent effect on the Raman parameters of the ν (BrBr) band

✍ Scribed by Guido Maes; ThéRèse Zeegers-Huyskens

Publisher
John Wiley and Sons
Year
1978
Tongue
English
Weight
399 KB
Volume
7
Category
Article
ISSN
0377-0486

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

Effective Rotation–Vibration Parameters
Effective Rotation–Vibration Parameters for the ν8and ν4+ ν12Bands of Ethane
✍ M. Hepp; M. Herman 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 147 KB

The jet-cooled spectrum of ethane in the region of the nu8 perpendicular fundamental vibration at 1472 cm-1 was recorded with a Fourier transform spectrometer at 0.01 cm-1 instrumental resolution. About 1150 lines were assigned to 18 subbands of nu8 ranging from K"DeltaK = -9 to +8. About 160 lines

Raman polarizabilities of the ν2, ν5 ban
Raman polarizabilities of the ν2, ν5 bands of CD3Cl
✍ R. Escribano; M. García Hernández; M. Mejías; S. Brodersen 📂 Article 📅 1985 🏛 John Wiley and Sons 🌐 English ⚖ 353 KB

The Raman spectrum of the Coriolis interacting u2, us bands of CD,CI was recorded with a resolution of cu 0.6 cm-'. Using the vibrational-rotational parameters of Yamada and Hirota, a computer simulation of the Raman contour was performed, yielding relative values of Raman polarizability derivatives

The ν5 Raman band of CH3CD3
The ν5 Raman band of CH3CD3
✍ Per Jensen; Svend Brodersen 📂 Article 📅 1982 🏛 John Wiley and Sons 🌐 English ⚖ 426 KB

## Abstract The ν~5~ Raman band of CH~3~CD~3~ was photographed with a resolution of about 0.4 cm^−1^ and analysed by an iterative method, in which the peak wavenumbers of the observed and computed contours are compared directly. Precise values for ν~0~ and Δ__B__ were obtained, whereas it only coul

The High-Resolution Raman Spectrum of th
The High-Resolution Raman Spectrum of the ν4Band of Diborane
✍ J.L. Doménech; D. Bermejo; J.-M. Flaud; W.J. Lafferty 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 92 KB

The high-resolution Raman spectra of the 4 bands of 11 B 2 H 6 and 11 B 10 BH 6 have been recorded and analyzed. The recordings have been made using a high-resolution spectrometer based on the inverse Raman effect. Q branches have been observed, but P and R branches were too weak to be seen, and sim