Inverse kinematics proton scattering on 18Ne and mirror symmetry in A=18 nuclei

被引:17
|
作者
Riley, LA
Jewell, JK
Cottle, PD
Glasmacher, T
Kemper, KW
Alamanos, N
Blumenfeld, Y
Carr, JA
Chromik, MJ
Ibbotson, RW
Maréchal, F
Ormand, WE
Petrovich, F
Scheit, H
Suomijärvi, T
机构
[1] Florida State Univ, Dept Phys, Tallahassee, FL 32306 USA
[2] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[3] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[4] CEA, DSM, DAPNIA, SPhN Saclay, F-91191 Gif Sur Yvette, France
[5] Inst Phys Nucl, IN2P3, CNRS, F-91406 Orsay, France
[6] Florida State Univ, Supercomp Computat Res Inst, Tallahassee, FL 32306 USA
[7] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA
关键词
D O I
10.1103/PhysRevLett.82.4196
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The 0(g.s.)(+) --> 2(1)(+) transition in Ne-18 has been studied using the inverse kinematics reaction p(Ne-18, p') with a radioactive Ne-18 beam at 30 MeV/nucleon. Hadronic scattering data on the 0(g.s.)(+) -->2(1)(+) transition in the mirror nucleus O-18 are already available, so this is the first time that hadronic measurements have been available to test mirror symmetry in s-d shell nuclei. The angular distribution data for proton inelastic scattering in 18Ne and corresponding data for O-18 are well reproduced in microscopic model calculations using empirical proton and neutron transition densities determined for O-18. [S0031-9007(99)09179-6].
引用
收藏
页码:4196 / 4199
页数:4
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