Papers

Peer-reviewed
2004

Halo structure of B-17 studied via its reaction cross section

NEW ERA OF NUCLEAR STRUCTURE PHYSICS
  • Y Yamaguchi
  • T Suzuki
  • T Ohtsubo
  • T Izumikawa
  • W Shinozaki
  • M Takahashi
  • R Koyama
  • S Watanabe
  • C Wu
  • A Ozawa
  • T Ohnishi
  • DQ Fang
  • T Suda
  • R Kanungo
  • H Jeppesen
  • Tanihata, I
  • M Fukuda
  • N Iwasa
  • Display all

First page
114
Last page
118
Language
English
Publishing type
Research paper (international conference proceedings)
DOI
10.1142/9789812702401_0017
Publisher
WORLD SCIENTIFIC PUBL CO PTE LTD

The reaction cross section for the neutron-rich nucleus B-17 on a carbon target has been measured at an energy of 77 AMeV by a transmission method. A large enhancement of 17B reaction cross section at low energy was observed. The density distribution of 17B was deduced through the energy dependence of the reaction cross section together with high-energy data using a finite-range Glauber-model calculation under an optical-limit approximation. It is confirmed that the neutron-tail in the density distribution is necessary for 17B in order to reproduce the measured reaction cross sections. Based on the assumption of a core (B-15) plus valence two-neutron picture, the mixture of v(2s(1/2)) and V(1d(5/2)) was studied without treating the correlation between two neutrons.

Link information
DOI
https://doi.org/10.1142/9789812702401_0017
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000229961300017&DestApp=WOS_CPL
ID information
  • DOI : 10.1142/9789812702401_0017
  • Web of Science ID : WOS:000229961300017

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