Conspectus
Most chemical processes are triggered by electron
or charge transfer
phenomena (CT). An important class of processes involving CT are chemi-ionization
reactions. Such processes are very common in nature, involving neutral
species in ground or excited electronic states with sufficient energy
(X*) to yield ionic products, and are considered as the primary initial
step in flames. They are characterized by pronounced electronic rearrangements
that take place within the collisional complex (X···M)*
formed by approaching reagents, as shown by the following scheme,
where M is an atomic or molecular target: X* + M → (X···M)*
→ [(X+···M) ↔ (X···M+)]
e−
(X···M)+ + e– → final ions.
Despite
their important role in fundamental and applied research,
combustion, plasmas, and astrochemistry, a unifying description of
these basic processes is still lacking. This Account describes a new
general theoretical methodology that demonstrates, for the first time,
that chemi-ionization reactions are prototypes of gas phase oxidation
processes occurring via two different microscopic mechanisms whose
relative importance varies with collision energy, E
c, and separation distance, R. These
mechanisms are illustrated for simple collisions involving Ne*(3P2,0) and noble gases (Ng). In thermal and hyperthermal
collisions probing interactions at intermediate and short R, the transition state [(Ne···Ng)+]
e− is a molecular species described
as a molecular ion core with an orbiting Rydberg electron in which
the neon reagent behaves as a halogen atom (i.e., F) with high electron
affinity promoting chemical oxidation. Conversely, subthermal collisions
favor a different reaction mechanism: Ng chemi-ionization proceeds
through another transition state [Ne*······Ng],
a weakly bound diatomic-lengthened complex where Ne* reagent, behaving
as a Na atom, loses its metastability and stimulates an electron ejection
from M by a concerted emission–absorption of a “virtual”
photon. This is a physical radiative mechanism promoting an effective
photoionization. In the thermal regime of E
c, there is a competition between these two mechanisms. The proposed
method overcomes previous approaches for the following reasons: (1)
it is consistent with all assumptions invoked in previous theoretical
descriptions dating back to 1970; (2) it provides a simple and general
description able to reproduce the main experimental results from our
and other laboratories during last 40 years; (3) it demonstrates that
the two “exchange” and “radiative” mechanisms
are simultaneously present with relative weights that change with E
c (this viewpoint highlights the fact that the
“canonical” chemical oxidation process, dominant at
high E
c, changes its nature in the subthermal
regime to a direct photoionization process; therefore, it clarifies
differences between the cold chemistry of terrestrial and interstellar
environments and the energetic one of combustion and flames); (4)
the proposed method explicitly accounts for the influence of the degree
of valence orbital alignmen...