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Molecular Physics
An International Journal at the Interface Between Chemistry and Physics
Volume 112, 2014 - Issue 18: 23rd Colloquium on High-Resolution Molecular Spectroscopy HRMS Budapest 2013
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Invited Articles

From quantum chemistry to dissociation kinetics: what we need to knowFootnote

Pages 2374-2383 | Received 25 Feb 2014, Accepted 15 May 2014, Published online: 23 Jun 2014

Figures & data

Figure 1. Falloff curves of the rate constants k at for non-dissociative electron attachment to SF6 (modelling from Ref. [Citation8]; dashed lines: only collisional stabilisation, full lines: collisional plus radiative stabilisation of SF6 −*).

Figure 1. Falloff curves of the rate constants k at for non-dissociative electron attachment to SF6 (modelling from Ref. [Citation8]; dashed lines: only collisional stabilisation, full lines: collisional plus radiative stabilisation of SF6 −*).

Figure 2. Specific rate constants for electron detachment (k det, SF6 → SF6 + e) and dissociation (k dis, SF6 → SF5 + F) of SF6 −* (modelling from Ref. [Citation10]; the energies E should be decreased by 0.17 eV after re-evaluation [Citation6] of E a).

Figure 2. Specific rate constants for electron detachment (k det, SF6 − → SF6 + e−) and dissociation (k dis, SF6 − → SF5 − + F) of SF6 −* (modelling from Ref. [Citation10]; the energies E should be decreased by 0.17 eV after re-evaluation [Citation6] of E a).

Figure 3. Dissociative electron attachment cross sections of SF6 as a function of electron energy E el and gas temperature T gas (experimental points from Ref. [Citation11]; modelling from Ref. [Citation10], dashed curves: total cross sections).

Figure 3. Dissociative electron attachment cross sections of SF6 as a function of electron energy E el and gas temperature T gas (experimental points from Ref. [Citation11]; modelling from Ref. [Citation10], dashed curves: total cross sections).

Figure 4. Branching fractions R = [SF5 ] / ([SF6 ] + [SF5 ]) for dissociative electron attachment to SF6 (filled experimental points after 4 ms of reaction time, open experimental points after 14 ms, from Ref. [Citation4]; low-pressure decrease of R: collisional stabilisation of primary SF6 −*, high-pressure increase of R: collisional thermal dissociation of SF6 after primary collisional stabilisation of primary SF6 −*).

Figure 4. Branching fractions R = [SF5 −] / ([SF6 −] + [SF5 −]) for dissociative electron attachment to SF6 (filled experimental points after 4 ms of reaction time, open experimental points after 14 ms, from Ref. [Citation4]; low-pressure decrease of R: collisional stabilisation of primary SF6 −*, high-pressure increase of R: collisional thermal dissociation of SF6 − after primary collisional stabilisation of primary SF6 −*).

Figure 5. Falloff curves for H + CH3 (+ M) → CH4 (+ M) (full lines: modelling from Ref. [Citation13], experimental data given in Ref. [Citation13]).

Figure 5. Falloff curves for H + CH3 (+ M) → CH4 (+ M) (full lines: modelling from Ref. [Citation13], experimental data given in Ref. [Citation13]).

Figure 6. Falloff curves for CH4 (+ M) → CH3 + H (+ M) (M = CH4, modelling from Ref. [Citation13], experimental data given in Ref. [Citation13]).

Figure 6. Falloff curves for CH4 (+ M) → CH3 + H (+ M) (M = CH4, modelling from Ref. [Citation13], experimental data given in Ref. [Citation13]).

Figure 7. Falloff curves for CH4 (+ M) → CH3 + H (+ M) (M = Ar, T = 2200 K; full and dashed lines: modelling from Ref. [Citation14], experimental data given in Ref. [Citation14]).

Figure 7. Falloff curves for CH4 (+ M) → CH3 + H (+ M) (M = Ar, T = 2200 K; full and dashed lines: modelling from Ref. [Citation14], experimental data given in Ref. [Citation14]).

Figure 8. High-pressure limiting rate constants for CH4 → CH3 + H (theoretical modelling from Ref. [Citation14]; lines: modelling with potential of Equation (3.1) and C/D = 2.5, points: modelling with the ab initio potential of Refs [Citation16, 17]; upper line and points: isotropic potential, i.e. PST, lower line, and points: anisotropic potential).

Figure 8. High-pressure limiting rate constants for CH4 → CH3 + H (theoretical modelling from Ref. [Citation14]; lines: modelling with potential of Equation (3.1) and C/D = 2.5, points: modelling with the ab initio potential of Refs [Citation16, 17]; upper line and points: isotropic potential, i.e. PST, lower line, and points: anisotropic potential).

Figure 9. Dependence of transitional mode frequencies on the C–C bond length r in C2F4 (quantum-chemical calculations from Ref. [Citation30], α/Å−1 = anisotropy parameter, see the text).

Figure 9. Dependence of transitional mode frequencies on the C–C bond length r in C2F4 (quantum-chemical calculations from Ref. [Citation30], α/Å−1 = anisotropy parameter, see the text).

Figure 10. High-pressure limiting rate constants for 2 CF2 → C2F4 (line: SACM/CT calculations from Ref. [Citation30] with α/β ≈ 0.23, experimental data given in Ref. [Citation30]).

Figure 10. High-pressure limiting rate constants for 2 CF2 → C2F4 (line: SACM/CT calculations from Ref. [Citation30] with α/β ≈ 0.23, experimental data given in Ref. [Citation30]).

Figure 11. Minimum-energy path potential V(R) for HO2 → H + O2 (a 0 = 0.529 Å, from Ref. [Citation32]; points and full line: ab initio potential of Ref. [Citation31], dashed and dotted lines: simpler analytical potentials, see Ref. [Citation32]).

Figure 11. Minimum-energy path potential V(R) for HO2 → H + O2 (a 0 = 0.529 Å, from Ref. [Citation32]; points and full line: ab initio potential of Ref. [Citation31], dashed and dotted lines: simpler analytical potentials, see Ref. [Citation32]).

Figure 12. Transition-state switching in the adiabatic channel potential curves Vi (R) for HO2 → H + O2 (SACM calculations from Ref. [Citation32]; B = 1.446 cm−1, dash–dotted line: MEP potential of , other lines: channel potentials for l = j = 1, 3, 5, … from bottom to top, see Ref. [Citation32]).

Figure 12. Transition-state switching in the adiabatic channel potential curves Vi (R) for HO2 → H + O2 (SACM calculations from Ref. [Citation32]; B = 1.446 cm−1, dash–dotted line: MEP potential of Figure 11, other lines: channel potentials for l = j = 1, 3, 5, … from bottom to top, see Ref. [Citation32]).

Figure 13. Capture rate constants k cap for H + O2 → HO2 (from Ref. [Citation32], dashed line: with isotropic long-range potential, upper full line: PST with MEP potential of , lower full line: with anisotropic ab initio potential from Ref. [Citation31]).

Figure 13. Capture rate constants k cap for H + O2 → HO2 (from Ref. [Citation32], dashed line: with isotropic long-range potential, upper full line: PST with MEP potential of Figure 11, lower full line: with anisotropic ab initio potential from Ref. [Citation31]).

Figure 14. Falloff curves for H + O2 + M → HO2 + M (from Ref. [Citation28], M = N2, experimental points given in Ref. [Citation28], T = 300, 400, …, 900, and 1200 K from bottom to top).

Figure 14. Falloff curves for H + O2 + M → HO2 + M (from Ref. [Citation28], M = N2, experimental points given in Ref. [Citation28], T = 300, 400, …, 900, and 1200 K from bottom to top).

Figure 15. Long-range potential energy curves for C + HO → CHO (from Ref. [Citation34], numbers = Ω values).

Figure 15. Long-range potential energy curves for C + HO → CHO (from Ref. [Citation34], numbers = Ω values).

Figure 16. Association rate constants for C + HO → CHO (from Ref. [Citation35]; k ass = k rec,∞, dashed line: calculation with single electronic state and Equation (4.1), full line: calculation with full mixing of electronic states accounting for spin–orbit and rotronic coupling).

Figure 16. Association rate constants for C + HO → CHO (from Ref. [Citation35]; k ass = k rec,∞, dashed line: calculation with single electronic state and Equation (4.1), full line: calculation with full mixing of electronic states accounting for spin–orbit and rotronic coupling).

Figure 17. Experimental (points) and modelled (lines) low temperature rate constants for HO + O → H + O2 (from the Kinetic Database for Astrochemistry (KIDA) [Citation38]).

Figure 17. Experimental (points) and modelled (lines) low temperature rate constants for HO + O → H + O2 (from the Kinetic Database for Astrochemistry (KIDA) [Citation38]).

Figure 18. Rate constants for HO + O → H + O2 (various models from Ref. [Citation40] compared with experimental points, for details see Ref. [Citation40]; high temperature points from the reverse reaction converted with the equilibrium constant).

Figure 18. Rate constants for HO + O → H + O2 (various models from Ref. [Citation40] compared with experimental points, for details see Ref. [Citation40]; high temperature points from the reverse reaction converted with the equilibrium constant).