Journal Article GSI-2024-00894

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Smooth trends in fermium charge radii and the impact of shell effects

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2024
Nature Publ. Group London [u.a.]

Nature 634(8036), 1075 - 1079 () [10.1038/s41586-024-08062-z]

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Note: This article is licensed under a Creative Commons Attribution 4.0 International License. The on-line measurements presented here were performed at the velocity filter SHIP at the GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt (Germany) in the frame of FAIR Phase-0. We thank the GSI ion source and accelerator operation groups for the preparation of a stable 48Ca and 40Ar beam, and the GSI target laboratory for providing high-quality targets. The isotopes used in this research were provided by the US Department of Energy Office of Science Isotope R&D and Production Program. The 253,254,255Es and 255,257Fm were supplied to Florida State University and the University of Mainz via the processing at the Radiochemical Engineering Development Center at Oak Ridge National Laboratory. Separation of the einsteinium and fermium at ORNL was supported in part by the US DOE Office of Science, Heavy Element Chemistry programme. This project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement number 861198-LISA-H2020-MSCA-ITN-2019 and under grant agreement number 654002 (ENSAR2). P. Chhetri acknowledges funding from the European Union’s Horizon 2020 programme under the Marie Skłodowsk-Curie grant agreement number 1010267662. E.K., E.R.R. and M.L. acknowledge funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement number 819957). This work has been supported by the Bundesministerium für Bildung und Forschung (BMBF, Germany) under project numbers 05P18UMCIA and 05P21UMFN3. T.W. acknowledges funding from the Bundesministerium für Bildung und Forschung (BMBF, Germany) under grant number 05P21RDFN1. C.E.D., H.D. and T.K. acknowledge funding by DFG Research Unit for 2202 (ECHo) with financial support under the contracts DU 1334/1-1 and DU 1334/1-2. The SLyMR1 calculations were performed by using high-performance computing resources from GENCI-TGCC, France (contract number A0110513012) and the CC-IN2P3 of the CNRS. M. Bender acknowledges support by the Agence Nationale de la Recherche, France, grant number 19-CE31-0015-01 (NEWFUN). P.-G.R. acknowledges support through the high-performance computers of the RRZE (Erlangen, Germany). S.G. acknowledges financial support from F.R.S.-FNRS (Belgium). S.G. and W.R. are research associates of the F.R.S.-FNRS. The present research benefited from computational resources made available on the Tier-1 supercomputers Zenobe and Lucia of the Fédération Wallonie-Bruxelles, infrastructure funded by the Walloon Region under grant agreement number 1117545. Further computational resources have been provided by the clusters Consortium des Équipements de Calcul Intensif (CÉCI), funded by F.R.S.-FNRS under grant number 2.5020.11 and by the Walloon Region. P.V.D., A.C., R.F., A.d.R, E.V., S.K., P. Chhetri, J. Romans, S.G. and W.R. acknowledge funding from the Research Foundation - Flanders (FWO) and from the EOS (number 30468642) project of the FWO and F.R.S.-FNRS under the Excellence of Science (EOS) programme. I.M. received funding from the Academy of Finland under project number 339245. T.A.-S. and the team at Florida State University and Colorado School of Mines are supported by the US Department of Energy, Office of Science, Office of Basic Energy Sciences, Heavy Element Chemistry programme under award number DE-SC0023693. W.N. acknowledges support from the US Department of Energy under award numbers DOE-DE-NA0004074 (NNSA, the Stewardship Science Academic Alliances programme), DE-SC0013365 (Office of Science, Office of Nuclear Physics) and DE-SC0023175 (Office of Science, Office of Advanced Scientific Computing Research and Office of Nuclear Physics, Scientific Discovery through Advanced Computing programme). This publication is funded by the Open Access Publishing Fund of GSI Helmholtzzentrum für Schwerionenforschung. The results presented in this work are part of the PhD theses of J.W. and E.R.

Contributing Institute(s):
  1. SHE Physik (SHP)
  2. HIM / SHE (MSH)
  3. SHE Chemie (SHC)
  4. Collaboration FAIR: SHE (SHE@FAIR)
Research Program(s):
  1. 612 - Cosmic Matter in the Laboratory (POF4-612) (POF4-612)
  2. DFG project G:(GEPRIS)491382106 - Open-Access-Publikationskosten / 2025-2027 / GSI Helmholtzzentrum für Schwerionenforschung (491382106) (491382106)
  3. FAIR Phase-0 - FAIR Phase-0 Research Program (GSI-FAIR-Phase-0) (GSI-FAIR-Phase-0)
  4. LISA - Laser Ionization and Spectroscopy of Actinide elements (861198) (861198)
  5. ENSAR2 - European Nuclear Science and Application Research 2 (654002) (654002)
  6. LRC - Laser Resonance Chromatography of Superheavy Metals (819957) (819957)
  7. 05P21UMFN3 - Verbundprojekt 05P2021 (ErUM-FSP T07) - Aufbau von NUSTAR bei FAIR: Entwicklung von Methoden zur hochauflösenden Laserspektroskopie (BMBF-05P21UMFN3) (BMBF-05P21UMFN3)
Experiment(s):
  1. U313: Laser spectroscopy of nobelium and lawrencium (POF3-612; Y7)
  2. U321: Laser spectroscopy of fermium, nobelium and lawrencium around N=152 (POF3-612; Y7)
  3. G-22-00051: Laser spectroscopy of californium, fermium, nobelium and lawrencium isotopes around N=152 (Station: Y7)

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Dataset: Laser spectroscopy of fermium isotopes probing trends in nuclear charge radii
[10.5281/zenodo.13342174] BibTeX | EndNote: XML, Text | RIS


 Record created 2024-11-07, last modified 2025-07-17