2022
DOI: 10.1039/d2cp03414j
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Reaction of OH radicals with CH3NH2 in the gas phase: experimental (11.7–177.5 K) and computed rate coefficients (10–1000 K)

Abstract: Nitrogen-bearing molecules, like methylamine (CH3NH2), can be the building blocks of amino acids in the interstellar medium (ISM). At the ultralow temperatures of the ISM, it is important to know...

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Cited by 7 publications
(28 citation statements)
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“…However, the addition reaction between OH and CH 3 CN leading to CH 3 C(OH)N, competes with reaction (13) under low-pressure conditions at 10 K, with a computed rate coefficient of approximately 5 × 10 −14 cm 3 molecule −1 s −1 . As the temperature exceeds 200 K, the addition reaction becomes pressure-independent, and our calculated values align well with experimental data within the temperature range of 256 to 388 K. 51…”
Section: Resultssupporting
confidence: 85%
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“…However, the addition reaction between OH and CH 3 CN leading to CH 3 C(OH)N, competes with reaction (13) under low-pressure conditions at 10 K, with a computed rate coefficient of approximately 5 × 10 −14 cm 3 molecule −1 s −1 . As the temperature exceeds 200 K, the addition reaction becomes pressure-independent, and our calculated values align well with experimental data within the temperature range of 256 to 388 K. 51…”
Section: Resultssupporting
confidence: 85%
“…In the low-pressure regime, the canonical unified statistical (CUS) 25,26 model can be utilized. This model allows us to approximate the rate coefficient for the formation of the C + D products as:…”
Section: Kinetic Simulationsmentioning
confidence: 99%
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“…In the range 50–2000 K the rate constants are very fast, in the order of 10 −10 cm 3 molecule −1 s −1 . Note that this data is of a similar order to that obtained with the other two approaches 12,37 …”
Section: Theoretical Toolssupporting
confidence: 77%