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Matter radii of 32-35Mg

  • R. Kanungo*
  • , A. Prochazka
  • , W. Horiuchi
  • , C. Nociforo
  • , T. Aumann
  • , D. Boutin
  • , D. Cortina-Gil
  • , B. Davids
  • , M. Diakaki
  • , F. Farinon
  • , H. Geissel
  • , R. Gernhäuser
  • , J. Gerl
  • , R. Janik
  • , B. Jonson
  • , B. Kindler
  • , R. Knöbel
  • , R. Krücken
  • , M. Lantz
  • , H. Lenske
  • Y. Litvinov, B. Lommel, K. Mahata, P. Maierbeck, A. Musumarra, T. Nilsson, C. Perro, C. Scheidenberger, B. Sitar, P. Strmen, B. Sun, Y. Suzuki, I. Szarka, I. Tanihata, Y. Utsuno, H. Weick, M. Winkler
*Corresponding author for this work
  • Saint Mary's University Halifax
  • GSI Helmholtz Centre for Heavy Ion Research
  • Justus Liebig University Giessen
  • University of Santiago de Compostela
  • TRIUMF
  • National Technical University of Athens
  • Technical University of Munich
  • Comenius University
  • Chalmers University of Technology
  • Max Planck Institute for Nuclear Physics
  • University of Catania
  • National Institute for Nuclear Physics
  • Niigata University
  • RIKEN
  • The University of Osaka
  • Japan Atomic Energy Agency

Research output: Contribution to journalArticlepeer-review

Abstract

The interaction cross sections of 32-35Mg at 900A MeV have been measurmed using the fragment separator at GSI. The deviation from the r 0A1/3 trend is slightly larger for Mg35, signaling the possible formation of a longer tail in the neutron distribution for Mg35. The radii extracted from a Glauber model analysis with Fermi densities are consistent with models predicting the development of neutron skins.

Original languageEnglish
Article number021302
JournalPhysical Review C - Nuclear Physics
Volume83
Issue number2
DOIs
StatePublished - 9 Feb 2011

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