Konferenzpaper

Erschienen in: VIth International Conference on the Physics of Highly Charged Ions

Herausgeberliste: Richard, Patrick

Jahr der Veröffentlichung: 1993

Seiten: 618-621

ISBN: 1-56396-102-4

DOI Link: https://doi.org/10.1063/1.43674

Konferenz: 6th International Conference on the Physics of Highly Charged Ions

Serientitel: AIP conference proceedings

Serienzählung: 274

Abstract: 

We present secondary electron energy spectra of Ne^q+ (q=3,7,8,9,10), incident on a solid Pt(110) surface at different angles (10°–90°) with impact energies of 10 q keV. In the case of Ne¹⁰⁺ projectiles the filling of both K shell holes can be distringuished in the electron energy spectrum. It was found that the L shell is populated with 5 electrons during the first KLL Auger process (K²LL) and that the L shell is almost filled during the second one (K¹LL). The index denotes the number of vacancies in the K shell. The ^IK¹L′L/^IK²L′L intensity ratio varies as a function of the incidence angle and of the observation angle. Therefore, clear evidence is found for sub‐surface KLL Auger electron emission. Furthermore, a variation of the incident charge state of the Ne projectile from 10 to 7 results in a shift of the LMM Auger maxima to lower energies, which is consistent with corresponding Hartree‐Fock calculations.

Harvard-Zitierstil: Köhrbrück, R., Schippers, S., Hustedt, S., Heiland, W., Lecler, D., Kemmler, J., et al. (1993) Neutralization of Ne10+ ions interacting with a Pt(110) surface, in Richard, P. (ed.) VIth International Conference on the Physics of Highly Charged Ions. New York, NY: American Institute of Physics. pp. 618-621. https://doi.org/10.1063/1.43674

APA-Zitierstil: Köhrbrück, R., Schippers, S., Hustedt, S., Heiland, W., Lecler, D., Kemmler, J., Bleck-Neuhaus, J., & Stolterfoht, N. (1993). Neutralization of Ne10+ ions interacting with a Pt(110) surface. In Richard, P. (Ed.), VIth International Conference on the Physics of Highly Charged Ions. (pp. 618-621). American Institute of Physics. https://doi.org/10.1063/1.43674