Alan G. Sage
University of Bristol
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Physical Chemistry Chemical Physics | 2011
Alan G. Sage; Thomas A. A. Oliver; Daniel Murdock; Martin B. Crow; Grant A. D. Ritchie; Jeremy N. Harvey; Michael N. R. Ashfold
A recent review (Ashfold et al., Phys. Chem. Chem. Phys., 2010, 12, 1218) highlighted the important role of dissociative excited states formed by electron promotion to σ* orbitals in establishing the photochemistry of many molecular hydrides. Here we extend such considerations to molecular halides, with a particular focus on iodobenzene. Two experimental techniques (velocity mapped ion imaging (VMI) and time resolved infrared (IR) diode laser absorption) and electronic structure calculations have been employed in a comprehensive study of the near ultraviolet (UV) photodissociation of gas phase iodobenzene molecules. The VMI studies yield the speeds and angular distributions of the I((2)P(3/2)) and I*((2)P(1/2)) photofragments formed by photolysis in the wavelength range 330 ≥λ≥ 206 nm. Four distinct dissociation channels are observed for the I((2)P(3/2)) atom products, and a further three channels for the I*((2)P(1/2)) fragments. The phenyl (Ph) radical partners formed via one particular I* product channel following excitation at wavelengths 305 ≥λ≥ 250 nm are distributed over a sufficiently select sub-set of vibrational (v) states that the images allow resolution of specific I* + Ph(v) channels, identification of the active product mode (ν(10), an in-plane ring breathing mode), and a refined determination of D(0)(Ph-I) = 23,390 ± 50 cm(-1). The time-resolved IR absorption studies allow determination of the spin-orbit branching ratio in the iodine atom products formed at λ = 248 nm (ϕ(I*) = [I*]/([I] + [I*]) = 0.28 ± 0.04) and at 266 nm (ϕ(I*) = 0.32 ± 0.05). The complementary high-level, spin-orbit resolved ab initio calculations of sections (along the C-I bond coordinate) through the ground and first 19 excited state potential energy surfaces (PESs) reveal numerous excited states in the energy range of current interest. Except at the very shortest wavelength, however, all of the observed I and I* products display limiting or near limiting parallel recoil anisotropy. This encourages discussion of the fragmentation dynamics in terms of excitation to states of A(1) total symmetry and dissociation on the 2A(1) and 4A(1) (σ* ← n/π) PESs to yield, respectively, I and I* products, or via non-adiabatic coupling to other σ* ← n/π PESs that correlate to these respective limits. Similarities (and differences) with the available UV photochemical data for the other aryl halides, and with the simpler (and more thoroughly studied) iodides HI and CH(3)I, are summarised.
Molecular Physics | 2010
Alan G. Sage; Thomas A. A. Oliver; Richard N. Dixon; Michael N. R. Ashfold
The near-threshold photofragmentation dynamics of state-selected H2O+ cations have been investigated using velocity map ion imaging methods. The cations were prepared in the v = 0 level of the ground ( 2B1) electronic state, by 2 + 1 resonance enhanced multiphoton ionization via selected rotational levels of the H2O, 1B1, v = 0 state. Subsequent two photon excitation of the resulting H2O+ cations to 2B2 state levels lying above the lowest dissociation limit (i.e. at total energies in the range 46000–50600 cm−1) results in O–H bond fission and OH+ fragment ion formation. These fragments display isotropic recoil velocity distributions, which peak at low kinetic energy but extend to the highest speeds allowed by energy conservation. Ab initio calculations of key sections through the potential energy surfaces (PESs) for the ground and first few excited states of H2O+ suggest two possible mechanisms for the observed rotational and (when energetically allowed) vibrational excitation of the OH+ fragments. Both require initial non-adiabatic (vibronic coupling) from the photo-prepared state level to high levels of the 2A1 state, but involve different subsequent HO+−H bond fission mechanisms. One involves Renner–Teller coupling to the ground state PES, while the alternative requires spin-orbit induced coupling to the repulsive 4B1(4A″) state PES.
Journal of Chemical Physics | 2013
Alan G. Sage; Thomas A. A. Oliver; Graeme A. King; Daniel Murdock; Jeremy N. Harvey; Michael N. R. Ashfold
The wavelength dependences of C-Y and O-H bond fission following ultraviolet photoexcitation of 4-halophenols (4-YPhOH) have been investigated using a combination of velocity map imaging, H Rydberg atom photofragment translational spectroscopy, and high level spin-orbit resolved electronic structure calculations, revealing a systematic evolution in fragmentation behaviour across the series Y = I, Br, Cl (and F). All undergo O-H bond fission following excitation at wavelengths λ ≲ 240 nm, on repulsive ((n∕π)σ∗) potential energy surfaces (PESs), yielding fast H atoms with mean kinetic energies ∼11,000 cm(-1). For Y = I and Br, this process occurs in competition with prompt C-I and C-Br bond cleavage on another (n∕π)σ∗ PES, but no Cl∕Cl∗ products unambiguously attributable to one photon induced C-Cl bond fission are observed from 4-ClPhOH. Differences in fragmentation behaviour at longer excitation wavelengths are more marked. Prompt C-I bond fission is observed following excitation of 4-IPhOH at all λ ≤ 330 nm; the wavelength dependent trends in I∕I∗ product branching ratio, kinetic energy release, and recoil anisotropy suggest that (with regard to C-I bond fission) 4-IPhOH behaves like a mildly perturbed iodobenzene. Br atoms are observed when exciting 4-BrPhOH at long wavelengths also, but their velocity distributions suggest that dissociation occurs after internal conversion to the ground state. O-H bond fission, by tunnelling (as in phenol), is observed only in the cases of 4-FPhOH and, more weakly, 4-ClPhOH. These observed differences in behaviour can be understood given due recognition of (i) the differences in the vertical excitation energies of the C-Y centred (n∕π)σ∗ potentials across the series Y = I < Br < Cl and the concomitant reduction in C-Y bond strength, cf. that of the rival O-H bond, and (ii) the much increased spin-orbit coupling in, particularly, 4-IPhOH. The present results provide (another) reminder of the risks inherent in extrapolating photochemical behaviour measured for one molecule at one wavelength to other (related) molecules and to other excitation energies.
Chemical Science | 2013
Ondřej Tkáč; Alan G. Sage; Stuart J. Greaves; Andrew J. Orr-Ewing; Paul J. Dagdigian; Qianli Ma; Millard H. Alexander
Rotationally inelastic scattering of methyl radicals (CD3 and CH3) in collisions with helium is examined by a combination of velocity map imaging experiments and quantum scattering calculations. In the experiments a beam of methyl radicals seeded in Ar intersects a beam of He atoms at 90° at a collision energy of 440 ± 35 cm−1 (CD3 + He) or 425 ± 35 cm−1 (CH3 + He). The methyl radicals are prepared photolytically in a gas expansion that cools them to 15 K, giving a distribution over a small number of initial (low) rotational angular momentum states. By resonance-enhanced multi-photon ionization detection, we obtain velocity map images which are specific to a single rotational angular momentum quantum number n′ of the methyl radicals, but averaged over a small subset of the projection quantum number k′. We extract resolved angular scattering distributions for n′ = 2–9 (for CD3). We compare these to predictions of scattering calculations performed based on a recent potential energy surface [P. J. Dagdigian and M. H. Alexander, J. Chem. Phys. 2011, 135, 064306] in which the methyl radical was fixed at its equilibrium geometry. The fully (n, k) → (n′, k′) resolved differential cross sections obtained from the calculations, when combined in weighted sums over initial (n, k) levels corresponding to the 15 K experimental radical temperature, and final k′ levels that are not resolved in the spectroscopic detection scheme, show excellent agreement with the experimental measurements for all final states probed. This agreement gives confidence in the calculated dependence of the scattering on changes in both the n and k quantum numbers.
ChemPhysChem | 2013
Kiera M. Jones; Jadwiga A. Milkiewicz; Benjamin J. Whitaker; Alan G. Sage; Graham A. Worth
Ultrafast photodissociation of the 2 1A′ state of ClNO, which has an absorption spectrum peaking at 335 nm, is studied by computational and experimental methods. New potential-energy surfaces are calculated for the 1 and 2 1A′ states at the multireference configuration interaction (MRCI) level. Wavepacket dynamics simulations performed both exactly and by using the multiconfiguration time-dependent Hartree method yield essentially identical results. Transition dipole moments at a range of geometries are included in these calculations to correctly model the excitation. Vibrational and rotational state distributions of the NO product are obtained both computationally by analysing the quantum flux on the 2 1A′ surface and experimentally by use of 3D resonant multiphoton ionisation (REMPI), a variant of the velocity map imaging technique. The nascent NO is found to be only marginally vibrationally excited, with 91 % formed in v=0. The calculated NO rotational distribution peaks in the j=45–55 region, which compares favourably to experiment.
Physical Chemistry Chemical Physics | 2010
Michael N. R. Ashfold; Graeme A. King; Daniel Murdock; Michael G. D. Nix; Thomas A. A. Oliver; Alan G. Sage
Physical Chemistry Chemical Physics | 2010
Michael N. R. Ashfold; Graeme A. King; Daniel Murdock; Michael G. D. Nix; Thomas A. A. Oliver; Alan G. Sage
Chemical Physics | 2008
Alan G. Sage; Michael G. D. Nix; Michael N. R. Ashfold
Archive | 2015
Daniel Murdock; Greg T. Dunning; Michael N. R. Ashfold; Katharina Roettger; Rebecca A. Ingle; Alan G. Sage; Stephanie J. Harris; Ryan S. McMullen; Philip M. Coulter; Hugo J. B. Marroux; Jack Warren; Michael P. Grubb; Daisuke Koyama; Gareth M. Roberts; Andrew J. Orr-Ewing
Archive | 2011
Thomas A. A. Oliver; Graeme A. King; Alan G. Sage; Michael N. R. Ashfold