Some remarks on solar neutrinos

被引：2
|
作者：
Gough, D
机构：
[1] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[2] Univ Cambridge, Dept Appl Math & Theoret Phys, Cambridge CB3 9EW, England
[3] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2003年 / 285卷 / 02期
关键词：
neutrinos; stellar stability; helioseismology;
D O I：
10.1023/A:1025436425736
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In 1970 Fred Hoyle encouraged a study of solar neutrino production which led to a long-term investigation of the influence of what have become known as 'non-standard' processes (i.e. processes that are not accounted for in the relatively naively constructed so-called 'standard' theoretical solar models). The outcome is a very much sounder understanding of the structure and dynamics of the Sun, which has yielded a knowledge of conditions in the energy-generating core so precise that one can set quite tight reliable constraints on neutrino-producing nuclear reactions, and thereby provide an important contribution to the study of neutrino transitions.
引用
收藏
页码：341 / 351
页数：11
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