This book describes different theoretical models developed to
identify the near and mid infrared (IR) spectra of diatomic
molecules isolated in the gas phase or subjected to environmental
constraints, useful for the study of environmental sciences,
planetology and astrophysics. The applications presented show how
molecular interactions modify the near and mid IR spectra of
isolated diatomics under the effect of pressure, a nano-cage
(substitution site, Clathrate, Fullerene, Zeolite) or surfaces, to
identify the characteristics of the perturbing environment.
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