https://doi.org/10.1140/epjd/e2017-80122-x
Regular Article
Impact of buffer gas quenching on the 1S0 → 1P1 ground-state atomic transition in nobelium
1 Technische Universität Darmstadt, 64289 Darmstadt, Germany
2 GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt, Germany
3 Grand Accélérateur National d’Ions Lourds, BP 55027-14076 Caen Cedex 05, France
4 Johannes Gutenberg-Universität, 55099 Mainz, Germany
5 Helmholtz-Institut Mainz, 55099 Mainz, Germany
6 University of Liverpool, L69 7 ZE Liverpool, UK
7 KVI-Center for Advanced Radiation Technology, 9747 AA Groningen, The Netherlands
8 KU Leuven, 3001 Leuven, Belgium
9 TRIUMF, Vancouver, BC V6T 2A3, Canada
10 Institut de Physique Nucléaire Orsay, 91406 Orsay, France
a
e-mail: P.chhetri@gsi.de
Received: 22 February 2017
Published online: 19 July 2017
Using the sensitive Radiation Detected Resonance Ionization Spectroscopy (RADRIS) technique an optical transition in neutral nobelium (No, Z = 102) was identified. A remnant signal when delaying the ionizing laser indicated the influence of a strong buffer gas induced de-excitation of the optically populated level. A subsequent investigation of the chemical homologue, ytterbium (Yb, Z = 70), enabled a detailed study of the atomic levels involved in this process, leading to the development of a rate equation model. This paves the way for characterizing resonance ionization spectroscopy (RIS) schemes used in the study of nobelium and beyond, where atomic properties are currently unknown.
Key words: Atomic Physics
© EDP Sciences, Società Italiana di Fisica, Springer-Verlag 2017