Nucleosynthesis in classical novae

被引：108

作者：

Jose, Jordi ^{[1
]}

Hernanz, Margarita

Iliadis, Christian

机构：

[1] Univ Politecn Cataluna, Dept Fis & Engn Nucl, Barcelona, Spain

[2] Univ Politecn Cataluna, IEEC, Barcelona, Spain

[3] CSIC, Inst Ciencias Espai, Bellaterra, Spain

[4] CSIC, IEEC, Bellaterra, Spain

[5] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27515 USA

[6] Triangle Univ Nucl Lab, Durham, NC 27706 USA

来源：

NUCLEAR PHYSICS A | 2006年 / 777卷

关键词：

D O I：

10.1016/j.nuclphysa.2005.02.121

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：

Classical novae are dramatic stellar explosions with an energy release that is only overcome by supernovae and gamma-ray bursts. These unique cataclysmic events constitute a crucible where different scientific disciplines merge, including astrophysics, nuclear and atomic physics, cosmo-chemistry, high-energy physics or computer science. In this review, we focus on the nucleosynthesis accompanying nova outbursts. Theoretical predictions are compared with the elemental abundances inferred from observations of the nova ejecta as well as with the isotopic abundance ratios measured in meteorites. Special emphasis is given to the interplay between nova outbursts and the Galactic abundance pattern and on the synthesis of radioactive nuclei for which gamma-ray signals are expected. Finally, we analyze the key role played by nuclear physics in our understanding of the nova phenomenon by means of recent experiments and a thorough account of the impact of nuclear uncertainties. (c) 2005 Elsevier B.V. All rights reserved.

引用

页码：550 / 578

页数：29

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