Nuclear data on unstable nuclei for astrophysics

被引：1
|
作者：
Smith, MS [1 ]
Meyer, RA
Bardayan, DW
Blackmon, JC
Chae, K
Guidry, MW
Hix, WR
Kozub, RL
Lingerfelt, EJ
Ma, ZW
Scott, JP
机构：
[1] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA
[2] RAME Inc, Teaticket, MA USA
[3] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA
[4] Tennessee Technol Univ, Dept Phys, Cookeville, TN 38505 USA
来源：
NUCLEAR PHYSICS A | 2004年 / 746卷
关键词：
D O I：
10.1016/j.nuclphysa.2004.09.092
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
Recent measurements with radioactive beams at ORNL's Holifield Radioactive Ion Beam Facility (HRIBF) have prompted the evaluation of a number of reactions involving unstable nuclei needed for stellar explosion studies. We discuss these evaluations, as well as the development of a new computational infrastructure to enable the rapid incorporation of the latest nuclear physics results in astrophysics models. This infrastructure includes programs that simplify the generation of reaction rates, manage rate databases, and visualize reaction rates, all hosted at a new website www.nucastrodata.org.
引用
收藏
页码：569C / 572C
页数：4
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