Fragmentation of multiply charged hydrocarbon molecules CnHq+ (n ≤ 4, q ≤ 9) produced in high-velocity collisions: Branching ratios and kinetic energy release of the H+ fragment

K. Béroff, N. T. Van-Oanh, M. Chabot, T. Tuna, T. Pino, G. Martinet, A. Le Padellec, Y. Carpentier, and L. Lavergne
Phys. Rev. A 84, 032705 – Published 6 September 2011

Abstract

Fragmentation branching ratios for channels involving H+ emission and associated kinetic energy release of the H+ fragment [KER(H+)] have been measured for multicharged CnHq+ molecules produced in high velocity (3.6 a.u.) collisions between CnH+ projectiles and helium atoms. For CHq+ (q ≤ 4) molecules, measured KER(H+) were found well below predictions of the simple point charge Coulomb model (PCCM) for all q values. Multireference configuration interaction (MRCI) calculations for ground as well as electronic excited states were performed which allowed a perfect interpretation of the CHq+ experimental results for low charges (q = 2–3) as well as for the highest charge (q = 4). In this last case we could show, on the basis of ionization cross sections calculations and experimental measurements performed on the same systems at slightly higher velocity (4.5 a.u.), the prominent role played by inner-shell ionization followed by Auger relaxation and could extract the lifetime of this Auger relaxation giving rise to the best agreement between the experiment and the calculations. For dissociation of C2Hq+ and C3Hq+ with the highest charges (q ≥ 5), inner-shell ionization contributed in a prominent way to the ion production. In these two cases it was shown that measured KER(H+) were in good agreement with PCCM predictions when those were corrected for Auger relaxation with the same Auger lifetime value as in CH3+.

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  • Received 7 July 2011

DOI:https://doi.org/10.1103/PhysRevA.84.032705

©2011 American Physical Society

Authors & Affiliations

K. Béroff1, N. T. Van-Oanh2, M. Chabot3, T. Tuna3, T. Pino1, G. Martinet3, A. Le Padellec4, Y. Carpentier1,*, and L. Lavergne5

  • 1Institut des Sciences Moléculaires d’Orsay (ISMO), UMR CNRS 8214, Université Paris Sud 11, bât.210, F-91405 Orsay Cedex, France
  • 2Laboratoire de Chimie Physique (LCP), UMR CNRS 8000, Université Paris Sud 11, Bât.349, F-91405 Orsay Cedex, France
  • 3Institut de Physique Nucléaire d’Orsay (IPNO), IN2P3- CNRS, Université Paris Sud 11, F-91406 Orsay Cedex, France
  • 4Institut de Recherche en Astrophysique et Planétologie (IRAP), UMR CNRS 5187, Université de Toulouse, 9 avenue du Colonel Roche, F-31028 Toulouse Cedex 9, France
  • 5Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE) UPMC, UPD, CNRS-IN2P3, 4 Place Jussieu, F-75005 Paris, France

  • *Present address: Laboratory Astrophysics Group of the Max Planck Institute for Astronomy at the Friedrich Schiller University Jena, Institute of Solid State Physics, Helmholtzweg 3, D-07743 Jena, Germany.

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Vol. 84, Iss. 3 — September 2011

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