Density distribution of proton drip-line nucleus 17Ne

  • K. Tanaka*
  • , M. Fukuda
  • , M. Mihara
  • , M. Takechi
  • , T. Chinda
  • , T. Sumikama
  • , S. Kudo
  • , K. Matsuta
  • , T. Minamisono
  • , T. Ohtubo
  • , T. Suzuki
  • , S. Momota
  • , T. Izumikawa
  • , T. Yamaguchi
  • , T. Onishi
  • , A. Ozawa
  • , I. Tanihata
  • , Zheng Tao
  • *Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

17Ne is one of the candidates for a proton-halo nucleus. In order to make the halo structure of 17Ne clear, we studied the density distribution of 17Ne through the reaction cross sections σR. As a consequence, it is suggested from σR data that 17Ne has a long tail in the density, which is consistent with an occupancy of the 2s1/2 orbital by the two valence protons.

Original languageEnglish
Pages (from-to)532-535
Number of pages4
JournalNuclear Physics A
Volume746
Issue number1-4 SPEC.ISS.
DOIs
StatePublished - 27 Dec 2004
Externally publishedYes

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