Shell model studies for nuclear astrophysics

被引：2

作者：

Langanke, K. ^{[1
,2
,3
]}

Martinez-Pinedo, G. ^{[1
,2
]}

机构：

[1] GSI Helmholtzzentrum Schwerionenforsch, 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：

11TH INTERNATIONAL SPRING SEMINAR ON NUCLEAR PHYSICS: SHELL MODEL AND NUCLEAR STRUCTURE - ACHIEVEMENTS OF THE PAST TWO DECADES | 2015年 / 580卷

关键词：

WEAK-INTERACTION RATES; CHANDRASEKHAR-MASS MODELS; GAMOW-TELLER STRENGTH; MONTE-CARLO; ELECTRON-CAPTURE; RATE TABLES; LEVEL DENSITIES; SUPERNOVAE; COLLAPSE; EVOLUTION;

D O I：

10.1088/1742-6596/580/1/012033

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Shell model studies have contributed in recent years significantly to improve nuclear input required in simulations of the dynamics of astrophysical objects and their associated nucleosynthesis. This manuscript highlights a few examples like electron capture rates of importance for the evolution of core-collapse supernovae and the nucleosynthesis in thermonuclear supernovae, neutrino-nucleus cross sections with relevance to the supernova neutrino spectra and finally half lives of neutron-rich nuclei with magic neutron numbers which serve as waiting points in the mass flow of the astrophysical r-process.

引用

页数：6

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