Breakdown curves of carbon-based molecules for astrochemistry - Archive ouverte HAL
Communication Dans Un Congrès Année : 2015

Breakdown curves of carbon-based molecules for astrochemistry

Résumé

Breakdown curves (BDC), which are energy dependent fragmentation branching ratios, constitute a kind of "identity card" of an excited molecule or cluster. We developed a method for constructing semi-empirical BDC, based on fragmentation measurements and structural known quantities of the considered species. Calculations of BDC have been performed within the statistical M3C theory. We will present a comparison of the two methods for some species and discuss application of these results to astrochemistry.
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hal-04780849 , version 1 (13-11-2024)

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M Chabot, K Béroff, P Gratier, A Jallat, V Wakelam, et al.. Breakdown curves of carbon-based molecules for astrochemistry. 29th International Conference on Photonic, Electronic, and Atomic Collisions (ICPEAC), Jul 2015, Tolède, Spain. ⟨10.1088/1742-6596/635/3/032107⟩. ⟨hal-04780849⟩
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