Towards a converged barrier height for the entrance channel transition state of the N(2D)+CH4 reaction and its implication for the chemistry in Titan’s atmosphere
Author:
Publisher
Elsevier BV
Subject
Physical and Theoretical Chemistry,General Physics and Astronomy
Reference17 articles.
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5. Production of NH(X3Σ−) radicals in the reaction of N(22D) with CH4: nascent rotational and vibrational distributions of NH
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1. A computational characterization of the reaction mechanisms for the reactions N(2D) + CH3CN and HC3N and implications for the nitrogen-rich organic chemistry of Titan;Computational and Theoretical Chemistry;2023-11
2. A low temperature investigation of the N(2D) + CH4, C2H6 and C3H8 reactions;Physical Chemistry Chemical Physics;2019
3. Diffusion and reactivity of ground-state nitrogen atoms N(4S) between 3 and 15 K: application to the hydrogen abstraction reaction from methane under non-energetic conditions;Monthly Notices of the Royal Astronomical Society;2015-05-12
4. The neutral photochemistry of nitriles, amines and imines in the atmosphere of Titan;Icarus;2015-02
5. CRITICAL REVIEW OF N, N + , N + 2 , N ++ , And N ++ 2 MAIN PRODUCTION PROCESSES AND REACTIONS OF RELEVANCE TO TITAN'S ATMOSPHERE;The Astrophysical Journal Supplement Series;2013-01-29
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