LOW-TEMPERATURE ION TRAP STUDIES OF N+( super(3)Pja) + H sub(2)(j) arrow right NH+ + H

• Published in: The Astrophysical journal Vol. 768; no. 1; pp. 1 - 8
• Main Authors: Zymak, I, Hejduk, M, MULIN, D, Plasil, R, GLOSIK, J, Gerlich, D
• Format: Journal Article
• Language: English
• Published: 01-05-2013
• Subjects: Astrochemistry; Collisions; Formations; Gas density; Hydrogen storage; Recording; Rotational states; Trapping
• ISSN: 0004-637X; 1538-4357
• DOI: 10.1088/0004-637X/768/1/86

Using a low-temperature 22-pole ion trap apparatus, detailed measurements for the title reaction have been performed between 10 K and 100 K in order to get some state specific information about this fundamental hydrogen abstraction process. The relative population of the two lowest H sub(2) rotational states, j = 0 and 1, has been varied systematically. NH+ formation is nearly thermo-neutral; however, to date, the energetics are not known with the accuracy required for low-temperature astrochemistry. Additional complications arise from the fact that, so far, there is no reliable theoretical or experimental information on how the reactivity of the N+ ion depends on its fine-structure (FS) state super(3)Pja . Since in the present trapping experiment, thermalization of the initially hot FS population competes with hydrogen abstraction, the evaluation of the decay of N+ ions over long storage times and at various He and H sub(2) gas densities provides information on these processes. First assuming strict adiabatic behavior, a set of state specific rate coefficients is derived from the measured thermal rate coefficients. In addition, by recording the disappearance of the N+ ions over several orders of magnitude, information on nonadiabatic transitions is extracted including FS-changing collisions.