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Molecular-rotation-induced splitting of the binary ridge in the velocity map of sub-eV H+ ions ejected from H2 molecules by ion impact

Z. Juhász1,*, S. T. S. Kovács1, V. Vizcaïno2, P. Herczku1, S. Demes1, R. Rácz1, B. Sulik1, S. Biri1, N. Sens2 et al.

D. V. Mifsud3,1 and J.-Y. Chesnel2

  • 1Institute for Nuclear Research (Atomki), Debrecen H-4026, Hungary
  • 2Centre de Recherche sur les Ions, les Matériaux, et la Photonique (CIMAP), UMR 6252 CEA-CNRS-ENSICAEN-UNICAEN, Normandie Université, 14000 Caen, France
  • 3Centre for Astrophysics and Planetary Science, School of Physical Sciences, University of Kent, Canterbury CT2 7NH, United Kingdom

  • *zjuhasz@atomki.hu

Phys. Rev. A 107, L010801 – Published 19 January, 2023

DOI: https://doi.org/10.1103/PhysRevA.107.L010801

Abstract

In studies of ion-induced molecular fragmentation, the challenging measurement of the velocity distribution of fragments emitted below 1-eV kinetic energy is rarely achieved, although most fragments have an energy below this value. Here, we study H+ fragment emission in collisions of 10-keV O+ ions with H2 molecules using a field-free time-of-flight technique developed specifically to detect sub-eV fragments. We find that, in the velocity map, the binary ridge due to direct H+ knockout is split into two parts arising from the rotational motion of the H2 molecule, and that this split scales with rotational velocity. The velocity distribution of the nuclei in the original molecule is determined and the thermally populated J=1 rotational level is found to be the dominant contributor, although asymmetry in the split indicates projectile-induced rotational transitions between M sublevels. These rotation effects influence fragment emission probabilities, thus carrying important consequences for the radiation-induced hydrogen loss and H2 dissociation in the atmospheres or exospheres of planets and moons.

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