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 language | English |
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Pages (from-to) | 532-535 |
Number of pages | 4 |
Journal | Nuclear Physics A |
Volume | 746 |
Issue number | 1-4 SPEC.ISS. |
DOIs | |
Publication status | Published - 2004 Dec 27 |
ASJC Scopus subject areas
- Nuclear and High Energy Physics