Your browser doesn't support javascript.
loading
Charge Radii of
Sommer, Felix; König, Kristian; Rossi, Dominic M; Everett, Nathan; Garand, David; de Groote, Ruben P; Holt, Jason D; Imgram, Phillip; Incorvati, Anthony; Kalman, Colton; Klose, Andrew; Lantis, Jeremy; Liu, Yuan; Miller, Andrew J; Minamisono, Kei; Miyagi, Takayuki; Nazarewicz, Witold; Nörtershäuser, Wilfried; Pineda, Skyy V; Powel, Robert; Reinhard, Paul-Gerhard; Renth, Laura; Romero-Romero, Elisa; Roth, Robert; Schwenk, Achim; Sumithrarachchi, Chandana; Teigelhöfer, Andrea.
Afiliación
  • Sommer F; Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany.
  • König K; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Rossi DM; Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany.
  • Everett N; GSI Helmholtzzentrum für Schwerionenforschung GmbH, Planckstr. 1, 64291 Darmstadt, Germany.
  • Garand D; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • de Groote RP; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Holt JD; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Imgram P; Department of Physics, University of Jyväskylä, Survontie 9, Jyväskylä FI-40014, Finland.
  • Incorvati A; TRIUMF 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Kalman C; Department of Physics, McGill University, Montréal, Québec H3A 2T8, Canada.
  • Klose A; Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany.
  • Lantis J; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Liu Y; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Miller AJ; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Minamisono K; Department of Chemistry, Michigan State University, East Lansing, Michigan 48824, USA.
  • Miyagi T; Department of Chemistry, Augustana University, Sioux Falls, South Dakota 57197, USA.
  • Nazarewicz W; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Nörtershäuser W; Department of Chemistry, Michigan State University, East Lansing, Michigan 48824, USA.
  • Pineda SV; Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA.
  • Powel R; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Reinhard PG; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Renth L; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Romero-Romero E; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Roth R; Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany.
  • Schwenk A; TRIUMF 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Sumithrarachchi C; ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH, D-64291 Darmstadt, Germany.
  • Teigelhöfer A; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
Phys Rev Lett ; 129(13): 132501, 2022 Sep 23.
Article en En | MEDLINE | ID: mdl-36206412
ABSTRACT
Nuclear charge radii of ^{55,56}Ni were measured by collinear laser spectroscopy. The obtained information completes the behavior of the charge radii at the shell closure of the doubly magic nucleus ^{56}Ni. The trend of charge radii across the shell closures in calcium and nickel is surprisingly similar despite the fact that the ^{56}Ni core is supposed to be much softer than the ^{48}Ca core. The very low magnetic moment µ(^{55}Ni)=-1.108(20) µ_{N} indicates the impact of M1 excitations between spin-orbit partners across the N,Z=28 shell gaps. Our charge-radii results are compared to ab initio and nuclear density functional theory calculations, showing good agreement within theoretical uncertainties.

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2022 Tipo del documento: Article País de afiliación: Alemania

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2022 Tipo del documento: Article País de afiliación: Alemania