Determination of the branching ratio of CH$_3$OH + OH reaction on water ice surface at 10 K

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Hauptverfasser: Ishibashi, Atsuki, Hidaka, Hiroshi, Sameera, W. M. C., Oba, Yasuhiro, Watanabe, Naoki
Format: Preprint
Veröffentlicht: 2023
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author Ishibashi, Atsuki
Hidaka, Hiroshi
Sameera, W. M. C.
Oba, Yasuhiro
Watanabe, Naoki
author_facet Ishibashi, Atsuki
Hidaka, Hiroshi
Sameera, W. M. C.
Oba, Yasuhiro
Watanabe, Naoki
contents The CH$_3$O and CH$_2$OH radicals can be important precursors of complex organic molecules (COMs) in interstellar dust. The COMs presumably originating from these radicals were abundantly found in various astronomical objects. Because each radical leads to different types of COMs, determining the abundance ratio of CH$_3$O to CH$_2$OH is crucial for a better understanding of the chemical evolution to various COMs. Recent work suggested that the reaction between CH$_3$OH and OH on ice dust plays an important role in forming CH$_3$O and CH$_2$OH radicals. However, quantitative details on the abundance of these radicals have not been presented to date. Herein, we experimentally determined the branching ratio (CH$_3$O/CH$_2$OH) resulting from the CH$_3$OH + OH reaction on the water ice surface at 10 K to be 4.3 $\pm$ 0.6. Furthermore, the CH$_3$O product in the reaction would participate in subsequent diffusive reactions even at a temperature as low as 10 K. This fact should provide critical information for COMs formation models in cold molecular clouds.
format Preprint
id arxiv_https___arxiv_org_abs_2309_10351
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Determination of the branching ratio of CH$_3$OH + OH reaction on water ice surface at 10 K
Ishibashi, Atsuki
Hidaka, Hiroshi
Sameera, W. M. C.
Oba, Yasuhiro
Watanabe, Naoki
Astrophysics of Galaxies
The CH$_3$O and CH$_2$OH radicals can be important precursors of complex organic molecules (COMs) in interstellar dust. The COMs presumably originating from these radicals were abundantly found in various astronomical objects. Because each radical leads to different types of COMs, determining the abundance ratio of CH$_3$O to CH$_2$OH is crucial for a better understanding of the chemical evolution to various COMs. Recent work suggested that the reaction between CH$_3$OH and OH on ice dust plays an important role in forming CH$_3$O and CH$_2$OH radicals. However, quantitative details on the abundance of these radicals have not been presented to date. Herein, we experimentally determined the branching ratio (CH$_3$O/CH$_2$OH) resulting from the CH$_3$OH + OH reaction on the water ice surface at 10 K to be 4.3 $\pm$ 0.6. Furthermore, the CH$_3$O product in the reaction would participate in subsequent diffusive reactions even at a temperature as low as 10 K. This fact should provide critical information for COMs formation models in cold molecular clouds.
title Determination of the branching ratio of CH$_3$OH + OH reaction on water ice surface at 10 K
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2309.10351