Published January 2011 | Version v1
Journal article

Isotope-shift measurements of stable and short-lived lithium isotopes for nuclear-charge-radii determination

  • 1. Institut fuer Kernchemie, Universitaet Mainz, D-55099 Mainz (Germany)
  • 2. GSI Helmholtzzentrum fuer Schwerionenforschung GmbH, D-64291 Darmstadt (Germany)
  • 3. TRIUMF, Vancouver, British Columbia, V6T 2A3 (Canada)
  • 4. Pacific Northwest National Laboratory, Richland, Washington 99352 (United States)
  • 5. Department of Physics, University of Windsor, Windsor, Ontario, N9B 3P4 (Canada)
  • 6. Faculty of Physics, University of Warsaw, PL-00-681 Warsaw (Poland)
  • 7. Faculty of Chemistry, Adam Mickiewicz University, Grunwaldzka 6, PL-60-780 Poznan (Poland)
  • 8. Department of Physics, University of New Brunswick, Fredericton, New Brunswick, E3B 5A3 (Canada)

Description

Changes in the mean square nuclear charge radii along the lithium isotopic chain were determined using a combination of precise isotope shift measurements and theoretical atomic structure calculations. Nuclear charge radii of light elements are of high interest due to the appearance of the nuclear halo phenomenon in this region of the nuclear chart. During the past years we have developed a laser spectroscopic approach to determine the charge radii of lithium isotopes which combines high sensitivity, speed, and accuracy to measure the extremely small field shift of an 8-ms-lifetime isotope with production rates on the order of only 10 000 atoms/s. The method was applied to all bound isotopes of lithium including the two-neutron halo isotope 11Li at the on-line isotope separators at GSI, Darmstadt, Germany, and at TRIUMF, Vancouver, Canada. We describe the laser spectroscopic method in detail, present updated and improved values from theory and experiment, and discuss the results.

Additional details

Publishing Information

Journal Title
Physical Review. A
Journal Volume
83
Journal Issue
1
Journal Page Range
p. 012516-012516.33
ISSN
1050-2947
CODEN
PLRAAN

Optional Information

Notes
(c) 2011 American Institute of Physics