Competing Si2CH4–H2 and SiCH2–SiH4 Channels in the
Bimolecular Reaction of Ground-State Atomic Carbon (C(3Pj)) with Disilane (Si2H6, X1A1g) under Single Collision Conditions
posted on 2023-02-15, 15:06authored byDababrata Paul, Bing-Jian Sun, Chao He, Zhenghai Yang, Shane J. Goettl, Tao Yang, Bo-Yu Zhang, Agnes H. H. Chang, Ralf I. Kaiser
The
bimolecular gas-phase reaction of ground-state atomic carbon
(C(3Pj)) with disilane (Si2H6, X1A1g) was explored under single-collision
conditions in a crossed molecular beam machine at a collision energy
of 36.6 ± 4.5 kJ mol–1. Two channels were observed:
a molecular hydrogen elimination plus Si2CH4 (reaction 1) pathway and a silane loss channel along with the formation
of SiCH2 (reaction 2), with branching ratios of 20 ±
3 and 80 ± 4%, respectively. Both channels involved indirect
scattering dynamics via long-lived Si2CH6 reaction
intermediate(s); the latter eject molecular hydrogen and silane in
“molecular” elimination channels within the rotational
plane of the fragmenting intermediate nearly perpendicularly to the
total angular momentum vector. These molecular elimination channels
are associated with tight exit transition states as reflected in a
significant electron rearrangement as visible from the chemical bonding
in the light reaction products molecular hydrogen and silane. Once
these hydrogenated silicon-carbide clusters are formed within the
inner envelope of carbon stars such as of IRC + 10216, the stellar
wind can drive both Si2CH4 and SiCH2 to the outside sections of the envelope, where they can be photolyzed.
This is of particular importance to unravel potential formation pathways
to disilicon monocarbide (Si2C) observed recently in the
circumstellar shell of IRC + 10216.