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Unveiling the Ionization Energy of the CN Radical.

作者信息

Gans Bérenger, Boyé-Péronne Séverine, Garcia Gustavo A, Röder Anja, Schleier Domenik, Halvick Philippe, Loison Jean-Christophe

机构信息

Institut des Sciences Moléculaires d'Orsay (ISMO), UMR 8214 CNRS, Univ. Paris-Sud, Université Paris-Saclay , F-91405 Orsay, France.

Synchrotron SOLEIL , L'Orme des Merisiers, Saint Aubin BP 48, F-91192 Gif sur Yvette Cedex, France.

出版信息

J Phys Chem Lett. 2017 Sep 7;8(17):4038-4042. doi: 10.1021/acs.jpclett.7b01853. Epub 2017 Aug 15.

Abstract

The cyano radical is a ubiquitous molecule and was, for instance, one of the first species detected in astrophysical media such as comets or diffuse clouds. In photodissociation regions, the reaction rate of CN + CO → CN + CO is one of the critical parameters defining nitrile chemistry. The enthalpy of this charge transfer reaction is defined as the difference of ionization energies (E) between CN and CO. Although E(CO) is known accurately, the E(CN) values are more dispersed and deduced indirectly from thermodynamic thresholds only, all above E(CO), leading to the assumption that the reaction is fast even at low temperature. Using a combination of synchrotron radiation, electron/ion imaging coincidence techniques, and supporting ab initio calculations, we directly determine the first adiabatic ionization energy of CN at 13.956(7) eV, and we demonstrate that E(CN) < E(CO). The findings suggest a very slow reaction in the cold regions of interstellar media.

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