| タイトル |
-
en
Surface diffusion of carbon atoms as a driver of interstellar organic chemistry
|
| 作成者 |
|
| アクセス権 |
open access |
| 主題 |
-
Other
en
Astrophysical dust
-
Other
en
Interstellar medium
-
Other
en
Laboratory astrophysics
-
Other
en
Physical chemistry
-
NDC
440
|
| 内容注記 |
-
Abstract
en
Many interstellar complex organic molecules (COMs) are believed to be produced on the surfaces of icy grains at low temperatures. Atomic carbon is considered responsible for the skeletal evolution processes, such as C–C bond formation, via insertion or addition reactions. Before reactions, C atoms must diffuse on the surface to encounter reaction partners; therefore, information on their diffusion process is critically important for evaluating the role of C atoms in the formation of COMs. In situ detection of C atoms on ice was achieved by a combination of photostimulated desorption and resonance-enhanced multiphoton ionization methods. We found that C atoms weakly bound to the ice surface diffused above approximately 30 K and produced C2 molecules. The activation energy for C-atom surface diffusion was experimentally determined to be 88 meV (1,020 K), indicating that the diffusive reaction of C atoms is activated at approximately 22 K on interstellar ice. The facile diffusion of C atoms at temperatures above 22 K on interstellar ice opens a previously overlooked chemical regime where the increase in complexity of COMs is driven by C atoms. Carbon addition chemistry can be an alternative source of chemical complexity in translucent clouds and protoplanetary disks with crucial implications in our current understanding on the origin and evolution of organic chemistry in our Universe.
|
| 日付 |
|
| 言語 |
|
| 資源タイプ |
journal article |
| 出版タイプ |
AM |
| 資源識別子 |
HDL
http://hdl.handle.net/2115/91291
|
| 関連 |
-
isVersionOf
DOI
https://doi.org/10.1038/s41550-023-02071-0
|
| 収録誌情報 |
|
| ファイル |
|
| コンテンツ更新日時 |
2024-03-16 |
