The properties of halo structure for 17B-Reference-Cited by-同舟云学术

The properties of halo structure for 17B

Published:2008-06-22 Issue:7 Volume:51 Page:781-787
ISSN:1672-1799
Container-title:Science in China Series G: Physics, Mechanics and Astronomy
language:en
Short-container-title:Sci. China Ser. G-Phys. Mech. Astron.

Author:

Hu ZhengGuo,Wang Meng,Xu HuShan,Sun ZhiYu,Wang JianSong,Xiao GuoQing,Zhan WenLong,Xiao ZhiGang,Mao RuiShi,Li Chen,Zhang XueYing,Zhang HongBin,Zhao TieCheng,Xu ZhiGuo,Wang Yue,Chen RuoFu,Huang TianHeng,Fu Fen,Gao Qi,Han JianLong,Zhang XueHeng,Zheng Chuan,Yu YuHong,Guo ZhongYan

Publisher

Springer Science and Business Media LLC

Link

http://link.springer.com/content/pdf/10.1007/s11433-008-0083-9.pdf

Reference12 articles.

1. Jonson B. Light dripline nuclei. Phys Rep, 2004, 389: 1–59

2. Ren Z Z, Xu G O. A three-body model of 11Li, 14Be and 17B. Phys Lett B, 1990, 252: 311–313

3. Suzuki T, Kanungo R, Bochkarev O, et al. Nuclear radii of 17,19B and 14Be. Nucl Phys A, 1999, 658: 313–326

4. Suzuki T, Ogawa Y, Chiba M, et al. Momentum distribution of 15B fragments from the breakup of 17B. Phys Rev Lett, 2002, 89: 012501-1

5. Yamaguchi Y, Wu C, Suzuki T, et al. Density distribution of 17B from a reaction cross-section measurement. Phys Rev C, 2004, 70: 054320

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