5 research outputs found
Towards a Global Model of Spin-orbit Coupling in the Halocarbenes
We report a global analysis of spin-orbit coupling in the mono-halocarbenes, CH(D)X, where X = Cl, Br, and I. These are model systems for examining carbene singlet-triplet energy gaps and spin-orbit coupling. Over the past decade, rich data sets collected using single vibronic level emission spectroscopy and stimulated emission pumping spectroscopy have yielded much information on the ground vibrational level structure and clearly demonstrated the presence of perturbations involving the low-lying triplet state. To model these interactions globally, we compare two approaches. First, we employ a diabatic treatment of the spin-orbit coupling, where the coupling matrix elements are written in terms of a purely electronic spin-orbit matrix element which is independent of nuclear coordinates, and an integral representing the overlap of the singlet and triplet vibrational wavefunctions. In this way, the structures, harmonic frequencies, and normal mode displacements from ab initio calculations were used to calculate the vibrational overlaps of the singlet and triplet state levels, including the full effects of Duschinsky mixing. These calculations have allowed many new assignments to be made, particularly for CHI, and provided spin-orbit coupling parameters and values for the singlet-triplet gaps. In a second approach, we have computed and fit full geometry dependent spin-orbit coupling surfaces and used them to compute matrix elements without the product form approximation. Those matrix elements were used in similar fits varying the anharmonic constants and singlet-triplet gap to reproduce the experimental levels. The derived spin-orbit parameters for carbenes CHX (X = Cl, Br, and I) show an excellent linear correlation with the atomic spin-orbit constant of the corresponding halogen, indicating that the spin-orbit coupling in the carbenes is consistently around 14% of the atomic value
Reactive Pathways in the Chlorobenzene–Ammonia Dimer Cation Radical: New Insights from Experiment and Theory
Building
upon our recent studies of noncovalent interactions in
chlorobenzene and bromobenzene clusters, in this work we focus on
interactions of chlorobenzene (PhCl) with a prototypical N atom donor,
ammonia (NH<sub>3</sub>). Thus, we have obtained electronic spectra
of PhCl···(NH<sub>3</sub>)<sub><i>n</i></sub> (<i>n</i> = 1–3) complexes in the region of the
PhCl monomer S<sub>0</sub> −S<sub>1</sub> (ππ*)
transition using resonant 2-photon ionization (R2PI) methods combined
with time-of-flight mass analysis. Consistent with previous studies,
we find that upon ionization the PhCl···NH<sub>3</sub> dimer cation radical reacts primarily via Cl atom loss. A second
channel, HCl loss, is identified for the first time in R2PI studies
of the 1:1 complex, and a third channel, H atom loss, is identified
for the first time. While prior studies have assumed the dominance
of a π-type complex, we find that the reactive complex corresponds
instead to an in-plane σ-type complex. This is supported by
electronic structure calculations using density functional theory
and post-Hartree–Fock methods and Franck–Condon analysis.
The reactive pathways in this system were extensively characterized
computationally, and consistent with results from previous calculations,
we find two nearly isoenergetic arenium ions (Wheland intermediates;
denoted WH1, WH2), which lie energetically below the initially formed
dimer cation radical complex. At the energy of our experiment, intermediate
WH1, produced from <i>ipso</i>-addition, is not stable with
respect to Cl or HCl loss, and the relative branching between these
channels observed in our experiment is well reproduced by microcanonical
transition state theory calculations based upon the calculated parameters.
Intermediate WH2, where NH<sub>3</sub> adds ortho to the halogen,
decomposes over a large barrier via H atom loss to form protonated <i>o</i>-chloroaniline. This channel is not open at the (2-photon)
energy of our experiments, and it is suggested that photodissociation
of a long-lived (i.e., several ns) WH2 intermediate leads to the observed
products