HICKSON, Kevin M.,; LOISON, Jean-Christophe,; WAKELAM, Valentine

doi:10.1016/j.cplett.2016.07.004

Metadatos

Mostrar el registro completo del ítem

Licencia de uso del documento

HICKSON, Kevin M.,
Institut des Sciences Moléculaires [ISM]

LOISON, Jean-Christophe,
Institut des Sciences Moléculaires [ISM]

WAKELAM, Valentine
AMOR 2016

Idioma

Article de revue

Este ítem está publicado en

Chemical Physics Letters. 2016-08, vol. 659, p. 70 - 75

Elsevier

Resumen en inglés

The atomic hydrogen formation channels of the C + C2H2 reaction have been investigated using a continuous supersonic flow reactor over the 52-296 K temperature range. H-atoms were detected directly at 121.567 nm by vacuum ultraviolet laser induced fluorescence. Absolute H-atom yields were determined by comparison with the H-atom signal generated by the C + C2H4 reaction. The product yields agree with earlier crossed beam experiments employing universal detection methods. Incorporating these branching ratios in a gas-grain model of dense interstellar clouds increases the c-C3H abundance. This reaction is a minor source of C3-containing molecules in the present simulations.< Leer menos

Metadatos

Licencia de uso del documento

Temperature dependent product yields for the spin forbidden singlet channel of the C(3P) + C2H2 reaction

Idioma

Este ítem está publicado en

Resumen en inglés

DOI

Orígen

Centros de investigación