Dissociative Recombination

Dissociative recombination is a process where a positive molecular ion recombines with an electron, and as a result, the neutral molecule dissociates. This reaction is important for extraterrestrial and atmospheric chemistry. On Earth, dissociative recombination is practically non-existent, as free electrons would react with any molecule (even neutral molecules) they encounter. Even in the best laboratory conditions, dissociative recombination is hard to observe.

In astrophysics, dissociative recombination is one of the main paths via which molecules are broken down, and other molecules are formed. The existence of dissociative recombination is possible due to the vacuum of the interstellar medium. A typical example of dissociative recombination in astrophysics is:

Other articles related to "dissociative recombination":

Hydrogen Cyanide - Occurrence - HCN in Space
... via a neutral-neutral reaction (CH2 + N → HCN + H) and via dissociative recombination (HCNH+ + e- → HCN + H) ... The dissociative recombination pathway is dominant by 30% however, the HCNH+ must be in its linear form ... Dissociative recombination with its structural isomer, H2NC+, exclusively produces hydrogen isocyanide (HNC) ...