The solubility of I s in supercritical xenon with and without added C H has been 2 6 6 Ž . Ž . measured at the temperatures T s 300.79 " 0.04 K and 318.70 " 0.02 K over the pressure range from 5 MPa to 10 MPa. The u.v. absorbance due to the charge transfer interaction Ž . Ž . between I acceptor and
Molecular product formation from the charge-transfer state of C6H6I2
✍ Scribed by Gary DeBoer; Joseph W. Burnett; Mark A. Young
- Publisher
- Elsevier Science
- Year
- 1996
- Tongue
- English
- Weight
- 440 KB
- Volume
- 259
- Category
- Article
- ISSN
- 0009-2614
No coin nor oath required. For personal study only.
✦ Synopsis
The C6H 6 and I z molecular product fragments of the C6H6-I2 charge-transfer state have been investigated. Wavelength resolved studies show considerable rotational excitation of the benzene fragment and corresponding velocity spectra indicate a degree of translational excitation as well, consistent with rapid 12 bond dissociation in a bent complex. Another product channel active in the gas phase complex that forms molecular iodine was identified from measurements of kinetic energy release in the 12 fragment. The reaction mechanism is pictured as a charge-recombination step in the initially excited charge-transfer state, yielding I2(X i + ~ ) and C6H6(~ 3Bl,). Comparisons are made to corresponding observations for arene-I 2 species in the condensed phase.
📜 SIMILAR VOLUMES
Activity coefficients for the Ar-N,, CZH6-C2H4, and CSHB-CO2 systems are calculated from published vapour-liquid equilibrium compositions at various pressures and temperatures. The activity coefficients are correlated using a two parameter model based on the principles of molecular thermodynamics. T
Ices containing \(\mathrm{H}_{2} \mathrm{O}\) and small amounts of simple hydrocarbons, either in the form of clathrates or as intimate physical mixtures, are thought to be common outer Solar System condensates that were incorporated into comets and other bodies in the outer Solar System. We have pr
The structure and energetics of the C H и I complex have been studied 6 6 2 1 1.55 eV difference between the vertical and adiabatic excitation energies of 4 AЈ and the dramatic geometry change in the CT state.