Nuclear astrophysics at DANCE

被引：0

作者：

Reifarth, R ^{[1
]}

Alpizar-Vicente, A ^{[1
]}

Hatarik, R ^{[1
]}

Bredeweg, TA ^{[1
]}

Esch, EI ^{[1
]}

Greife, U ^{[1
]}

Haight, RC ^{[1
]}

Kronenberg, A ^{[1
]}

O'Donnell, JM ^{[1
]}

Rundberg, RS ^{[1
]}

Schwantes, JM ^{[1
]}

Ullmann, JL ^{[1
]}

Vieira, DJ ^{[1
]}

Wouters, JM ^{[1
]}

机构：

[1] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

来源：

INTERNATIONAL CONFERENCE ON NUCLEAR DATA FOR SCIENCE AND TECHNOLOGY, PTS 1 AND 2 | 2005年 / 769卷

关键词：

D O I：

暂无

中图分类号：

TL [原子能技术]; O571 [原子核物理学];

学科分类号：

0827 ; 082701 ;

摘要：

One of the most interesting nuclear physics challenges is obtaining a detailed understanding of the nucleosynthesis processes of the elements. Knowledge about the stellar sites, and how they are governed by stellar evolution and cosmology are crucial in understanding the overall picture. Information on reaction rates for neutron- and charged-particle-induced reactions have a direct impact on existing stellar models. Except for the stable isotopes, very few neutron-induced reactions in the energy range of interest have been measured to date. DANCE measurements on stable and unstable isotopes will provide many of the missing key reactions that are needed to understand the nucleosynthesis of the heavy elements.

引用

页码：1323 / 1326

页数：4

共 16 条

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