Impact of buffer gas quenching on the $^1S_0$ $\to$ $^1P_1$ ground-state atomic transition in nobelium

6533b870fe1ef96bd12cfd9f

RESEARCH PRODUCT

Impact of buffer gas quenching on the $^1S_0$ $\to$ $^1P_1$ ground-state atomic transition in nobelium

Michael Block C. Wraith F. P. Heßberger Enrique Minaya Ramirez Werner Lauth F. Lautenschläger Dieter Ackermann P. Chhetri F. Giacoppo Jadambaa Khuyagbaatar Hartmut Backe Sebastian Raeder Mustapha Laatiaoui Christoph E. Düllmann Peter Kunz Alexander Yakushev S. Götz Rafael Ferrer Thomas Walther A. K. Mistry Julia Even Oliver Kaleja Bradley Cheal

subject

Ytterbium Quenching (fluorescence)Materials science Buffer gas chemistry.chemical_element Rate equation [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences Atomic and Molecular Physics and Optics Spectral line 010305 fluids & plasmas chemistry 0103 physical sciences Atomic Physics ddc:530 Nobelium Physics::Atomic Physics Atomic physics 010306 general physics Ground state Spectroscopy

description

International audience; Using the sensitive Radiation Detected Resonance Ionization Spectroscopy (RADRIS) techniquean 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 studyof nobelium and beyond, where atomic properties are currently unknown.

year	journal	country	edition	language
2017-07-01

10.1140/epjd/e2017-80122-x https://hal.science/hal-01582876

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