Recent progress and some open questions in nuclear astrophysics

被引：3
|
作者：
Langanke, K. [1 ,2 ,3 ]
Martinez-Pinedo, G. [1 ,2 ]
机构：
[1] GSI Helmholtzzentrum Schwerionenforsch, Planckstr 1, D-64291 Darmstadt, Germany
[2] Tech Univ Darmstadt, Inst Kernphys, D-64291 Darmstadt, Germany
[3] Frankfurt Inst Adv Studies, D-60438 Frankfurt, Germany
来源：
PHYSICA SCRIPTA | 2015年 / T166卷
关键词：
supernova; electron capture; shell model; WEAK-INTERACTION RATES; MODEL MONTE-CARLO; CHANDRASEKHAR-MASS MODELS; GAMOW-TELLER STRENGTH; SHELL-MODEL; R-PROCESS; RATE TABLES; NUCLEOSYNTHESIS; COLLAPSE; SUPERNOVAE;
D O I：
10.1088/0031-8949/2015/T166/014001
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We discuss recent advances in modelling two topics of current interest in nuclear astrophysics: electron capture onto nuclei in core-collapse supernovae and simulations of the astrophysical r-process in neutron-star mergers. Despite this progress open questions remain. The answers to these questions will highly benefit from experimental data expected from current and future radioactive ion beam facilities, in particular from the Facility for Antiproton and Ion Research which is currently under construction at the GSI Helmholtzzentrum fur Schwerionenforschung in Darmstadt, Germany.
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页数：4
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