Electronic states of Ar2F and Kr2F

Abstract
Ab initio POL CI calculations have been performed on the low‐lying states of Ar2F and Kr2F. The results support a simple diatomics‐in‐molecules description of Rg2F (Rg=rare gas). In each case only one ionic state (2 2B2) is found to be stable (by 0.6 eV) relative to Rg+F+Rg. The equilibrium geometry is found to be an isosceles triangle where the Rg–Rg distance is 0.02 Å shorter than that in the 2Σ+u state of Rg+2 and the Rg–F distance is 0.14 Å greater than that in the 2 2Σ+ state of RgF. There are two dipole‐allowed emissions (2 2B2→1 2A1, 2 2B2→1 2B2) of comparable strength and wavelength (267 and 274 nm, respectively, in Ar2F and 357 and 368 nm, respectively, in Kr2F). The calculated wavelengths are in good agreement with the broad bands at 290 and 400 nm observed in e‐beam pumped Ar or Kr/F2 mixtures, confirming the earlier assignment of these bands to Ar2F and Kr2F, respectively. The radiative lifetime of the 2 2B2 is calculated to be 132 ns for both Ar2F and Kr2F. There are four dipole‐allowed absorptions from the 2 2B2 state, one of which (2 2B2→3 2A1) is very strong and corresponds to the 2Σ+u2Σ+g transition in Ar+2 and Kr+2. The effect of the F on this transition is negligible, so that the calculated wavelengths (320 nm in Ar2F and 344 nm in Kr2F) and oscillator strengths are basically unchanged from the rare gas dimer ions. Therefore, Ar2F and Kr2F may be at least as important as the Ar+2 and Kr+2 absorbers in the KrF laser. Spin–orbit coupling has been included at the equilibrium geometry of the 2 2B2 state using a simple atoms‐in‐molecules approach. The stability of the 2 2B2 (now 4 2Γ) state is decreased slightly so that De(Rg+F+Rg) is 0.57 eV for Ar2F and 0.49 eV for Kr2F. The emission wavelengths and radiative lifetime for the 2 2B2 state in Ar2F are unchanged, as are the wavelengths and strength of the 2 2B2→3 2A1 absorption. In Kr2F the emission wavelengths are shifted slightly to 361 and 371 nm, while the radiative lifetime becomes 133 ns. The 2 2B2→3 2A1 absorption in Kr2F shifts to 336 nm and the strength decreases by 5%. Consideration of the geometry dependence of the transition moment and emission wavelength indicates that vibrational averaging should not change the radiative lifetimes for Ar2F and Kr2F significantly. Recent experimental measurements of the Ar2F (185±45 ns) and the Kr2F (176±20 ns) lifetimes are in good agreement with the calculated values. Finally, the calculations indicate that Rg+2F should be formed by three‐body quenching of Rg+F rather than reaction of rare gas excimers with molecular fluorine. The latter exothermic reaction produces highly excited Rg+2F, which falls apart into Rg+F+Rg. These conclusions are supported by recent experimental results.