The production mechanism for interstellar silicon compounds SiCN, its isomer SiNC, hydrogen cyanide HCN and its isomer HNC from the neutral-neutral reactions SiN + CH and SiC + NH was studied using ab initio molecular dynamics. Classical trajectories were calculated by the direct dynamics simulation
Ab initio molecular dynamics simulation on reaction
β Scribed by Jun-ichi Yamamoto
- Book ID
- 108286112
- Publisher
- Elsevier Science
- Year
- 2010
- Tongue
- English
- Weight
- 406 KB
- Volume
- 957
- Category
- Article
- ISSN
- 0166-1280
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