TIME-OF-FLIGHT MASS MEASUREMENTS AND THEIR IMPORTANCE FOR NUCLEAR ASTROPHYSICS

被引:0
|
作者
Matos, M. [1 ]
Estrade, A. [1 ,2 ]
Amthor, A. M. [1 ,2 ]
Bazin, D. [1 ]
Becerril, A. [1 ,2 ]
Elliot, T. [1 ,2 ]
Famiano, M. [3 ]
Gade, A. [1 ,2 ]
Galaviz, D. [1 ]
Lorusso, G. [1 ,2 ]
Pereira, J. [1 ]
Portillo, M. [1 ]
Rogers, A. [1 ,2 ]
Schatz, H. [1 ,2 ]
Shapira, D. [4 ]
Smith, E. [5 ]
Stolz, A. [1 ]
Wallace, M. [6 ]
机构
[1] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[2] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[3] Western Michigan Univ, Dept Phys, Kalamazoo, MI 49008 USA
[4] Oak Ridge Natl Lab, Oak Ridge, TN USA
[5] Ohio State Univ, Columbus, OH 43210 USA
[6] Los Alamos Natl Lab, Los Alamos, NM USA
来源
ACTA PHYSICA POLONICA B | 2009年 / 40卷 / 03期
基金
美国国家科学基金会;
关键词
D O I
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中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Atomic masses play an important role in nuclear astrophysics. The lack of experimental values for nuclides of interest has triggered a rapid development of new mass measurement devices around the world, including Time-of-Flight (TOF) mass measurements offering an access to the most exotic nuclides. Recently, the TOF-B rho technique that includes a position measurement for magnetic rigidity correction has been implemented at the NSCL. An experiment with a similar TOF-B rho technique is approved and planned at the next generation radioactive beam facility (RIBF) at RIKEN.
引用
收藏
页码:695 / 698
页数:4
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