Revealing Radical Reactivity | Chemical & Engineering News
Volume 89 Issue 51 | p. 37 | Concentrates
Issue Date: December 19, 2011

Revealing Radical Reactivity

Low-temperature spectroscopic technique to track radical-radical reactions should aid study of star formation
Department: Science & Technology
News Channels: Analytical SCENE
Keywords: radical reaction, reaction mechanism, low temperature, supersonic, CRESU technique, interstellar

Radical-radical reactions are notoriously difficult to track, but a twist on a standard technique has enabled researchers to study the reaction of N∙ with HO∙ to form ∙NO and H∙ (Science, DOI: 10.1126/science.1213789). The method and results should promote the study of radical reactions and better understanding of such chemistry in interstellar clouds—the regions of the universe where stars form. A group led by Kevin M. Hickson of France’s National Center for Scientific Research and the University of Bordeaux adapted a technique for low-temperature reactions that involves allowing a gas to expand from a high-pressure reservoir through a nozzle into a vacuum chamber, creating a cold, supersonic jet of gas. The researchers created N∙ from N2 by microwave discharge just upstream of the reservoir and HO∙ by pulsed-laser photolysis of H2O2 directly in the supersonic flow. They then monitored the concentrations of HO∙ and the product ∙NO by laser-induced fluorescence. The team used the results to calculate rate constants for the reaction from 56 to 296 K. The results agree with theoretical predictions and should help improve chemical models of interstellar clouds, which are at 10 K, the researchers say.

Chemical & Engineering News
ISSN 0009-2347
Copyright © American Chemical Society

Leave A Comment

*Required to comment