The Hoyle state in 12C

被引:184
作者
Freer, M. [1 ]
Fynbo, H. O. U. [2 ]
机构
[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[2] Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark
关键词
Nuclear structure; Nuclear clustering; Nucleosynthesis; MONTE-CARLO CALCULATIONS; EXCITED-STATES; BETA-DECAY; TRANSITION WIDTHS; NUCLEAR-REACTIONS; RADIATIVE DECAY; ALPHA-PARTICLES; BRANCHING RATIO; 7.65-MEV STATE; 7.66-MEV STATE;
D O I
10.1016/j.ppnp.2014.06.001
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
The 7.65 MeV, J(pi) = 0(+), second excited state in C-12 is known as the Hoyle-state after Fred Hoyle. In the 1950s Hoyle proposed the existence of the state in order to account for the stellar abundance of carbon. Aside from its key role in the synthesis of the elements it is believed to possess a rather unusual structure, where the dominant degrees of freedom are those of alpha-particle clusters rather than nucleons. An understanding of the properties of the Hoyle state, for example its radius and excitations, has been the focus of a major experimental activity. Similarly, unravelling precisely why a cluster state should arise at precisely the right energy to promote synthesis of carbon has been a central theoretical challenge. To a significant extent, the Hoyle-state has become a cornerstone for state-of-the-art nuclear theory. This review examines the present status of both theory and experiment and indicates directions for future developments to resolve some of the remaining open questions. Crown Copyright (C) 2014 Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 23
页数:23
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