Isotope shifts from collinear laser spectroscopy of doubly charged yttrium isotopes

L. J. Vormawah, M. Vilén, R. Beerwerth, P. Campbell, B. Cheal, A. Dicker, T. Eronen, S. Fritzsche, S. Geldhof, A. Jokinen, S. Kelly, I. D. Moore, M. Reponen, S. Rinta-Antila, S. O. Stock, and A. Voss
Phys. Rev. A 97, 042504 – Published 16 April 2018

Abstract

Collinear laser spectroscopy has been performed on doubly charged ions of radioactive yttrium in order to study the isotope shifts of the 294.6-nm 5sS1/225pP1/22 line. The potential of such an alkali-metal-like transition to improve the reliability of atomic-field-shift and mass-shift factor calculations, and hence the extraction of nuclear mean-square radii, is discussed. Production of yttrium ion beams for such studies is available at the IGISOL IV Accelerator Laboratory, Jyväskylä, Finland. This newly recommissioned facility is described here in relation to the on-line study of accelerator-produced short-lived isotopes using collinear laser spectroscopy and application of the technique to doubly charged ions.

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  • Received 4 February 2018

DOI:https://doi.org/10.1103/PhysRevA.97.042504

©2018 American Physical Society

Physics Subject Headings (PhySH)

Accelerators & BeamsNuclear PhysicsAtomic, Molecular & OpticalInterdisciplinary Physics

Authors & Affiliations

L. J. Vormawah1, M. Vilén2, R. Beerwerth3,4, P. Campbell5, B. Cheal1,*, A. Dicker5, T. Eronen2, S. Fritzsche3,4, S. Geldhof2, A. Jokinen2, S. Kelly5, I. D. Moore2, M. Reponen2, S. Rinta-Antila2, S. O. Stock3,4, and A. Voss2

  • 1Department of Physics, University of Liverpool, Liverpool L69 7ZE, United Kingdom
  • 2Department of Physics, University of Jyväskylä, PB 35(YFL) FIN-40351 Jyväskylä, Finland
  • 3Helmholtz Institut Jena, Fröbelstieg 3, 07743 Jena, Germany
  • 4Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, 07743 Jena, Germany
  • 5School of Physics and Astronomy, University of Manchester, Manchester M13 9PL, United Kingdom

  • *bradley.cheal@liverpool.ac.uk

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Issue

Vol. 97, Iss. 4 — April 2018

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