Hannover 2020 – scientific programme
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MO: Fachverband Molekülphysik
MO 5: MO Poster 1
MO 5.13: Poster
Monday, March 9, 2020, 17:00–19:00, Empore Lichthof
High-resolution infrared and millimeter-wave spectroscopy of CNHn+ (n = 0,4,6) ions — •Sven Thorwirth1, Oskar Asvany1, Charlie Markus2, Jose Domenech3, Thomas Salomon1, Philipp Schmid1, Matthias Töpfer1, Philip Schreier1, and Stephan Schlemmer1 — 1I. Physikalisches Institut, Universität zu Köln — 2Department of Chemistry, University of Illinois, Urbana, IL, U.S.A. — 3Instituto de Estructura de la Materia (IEM-CSIC), Madrid, Spain
Molecular ions play crucial roles in the astrochemistry associated with star formation and planetary atmospheres. In this project, we have studied three fundamental cations CNHn+ (n = 0,4,6) using action spectroscopic techniques in a 22-pole ion trap at a nominal temperature of 4K [1]. The fundamental diatomic CN+ [2] as well as protonated methylene imine, H2C=NH2+, and protonated methyl amine, H3C=NH3+, were all studied by their pure rotational spectra in the millimeter-wave region employing the method of rotational state-selective He-attachment [3]. CN+ and H2C=NH2+ were also studied at high spectral resolution in the infrared using LIICG (Laser Induced Inhibition of Complex Growth) [1,4].
[1] O. Asvany, S. Brünken, L. Kluge, and S. Schlemmer 2014, Appl. Phys. B 114, 203 [2] S. Thorwirth, P. Schreier, T. Salomon, S. Schlemmer, and O. Asvany 2019, Astrophys. J. Lett. 882, L6 [3] S. Brünken, L. Kluge, A. Stoffels, J. Peres-Rios, and S. Schlemmer 2017, J. Mol. Spectrosc. 322, 67 [4] S. Chakrabarty, M. Holz, E. K. Campbell, A. Banerjee, D. Gerlich, and J. P. Maier 2013, J. Phys. Chem. Lett. 4, 4051