THE RATE OF THE REACTION BETWEEN H AND DCN

Authors
Citation
E. Herbst et D. Talbi, THE RATE OF THE REACTION BETWEEN H AND DCN, Astronomy and astrophysics (Berlin), 338(3), 1998, pp. 1080-1083
Citations number
17
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
00046361
Volume
338
Issue
3
Year of publication
1998
Pages
1080 - 1083
Database
ISI
SICI code
0004-6361(1998)338:3<1080:TROTRB>2.0.ZU;2-2
Abstract
It has been suggested that the slightly endothermic reaction between H and DCN to produce HCN and D serves to deplete DCN in hot core region s of giant molecular clouds. We have calculated the rate of this react ion for a range of temperatures up to 500 K with a combination of ab i nitio quantum chemical and dynamical techniques. We find that the reac tion has two potential barriers lying between the reactants and produc ts. These barriers permit only a very slow reaction except at high tem peratures. We calculate that the rate coefficient k of the reaction fo llows the formula k (cm(3) s(-1)) = 2 10(-11) Gamma(t)exp(-4931/T), wh ere Gamma(t) is a tunneling correction. The estimated rate coefficient at 300 K is 5 10(-18) cm(3) s(-1); this rate coefficient is far too s mall to be important in the destruction of DCN.