Understanding of the chemical processes that govern formation and destruction of nitrogen
oxides (NO x) in combustion processes continues to be a challenge. Even though this area …

A new era in chemical kinetics was heralded 20 years ago by the results reported by
Bertrand Rowe, then at the Laboratoire d AØrothermique in Meudon.[1] Using an apparatus …

In the context of recent observations, microphysical models, and laboratory data, a
photochemical model of Titan's atmosphere, including updated chemistry focusing on rate …

The implementation of variational transition state theory (VTST) for long-range asymptotic
potential forms is considered, with particular emphasis on the energy and total angular …

We introduce a new 1D coupled Radiative/Convective-Photochemical-Microphysical model
for a planetary atmosphere and apply it to Titan. The model incorporates detailed radiation …

The nitric oxide (NO) formation in methane (CH 4) flames has been widely investigated, with
quite a few kinetic mechanisms available in the literature. However, studies have shown that …

The field of astrochemistry concerns the formation and abundance of molecules in the
interstellar medium, star-forming regions, exoplanets, and solar system bodies. These …

A CRESU (Cine′ tique de Re′ action en Ecoulement Supersonique Uniforme) apparatus
has been used to measure rate constants for the reactions of the ethynyl radical (C2H) with …

A major aim of astrochemistry is to explain the nature and abundance of the molecules
observed in the interstellar medium (ISM). Three kinds of activity are involved:(a) the …

In order to investigate seasonal variations of the composition of Titan's low stratosphere, we
developed a two-dimensional (latitude–altitude) photochemical and transport model. Large …