AN EXPLANATION FOR THE SOLAR NEUTRINO PROBLEM - A NEW MECHANISM OF THERMONUCLEAR REACTION

被引：0
|
作者：
WANG, HZ
机构：
来源：
PROCEEDINGS ASTRONOMICAL SOCIETY OF AUSTRALIA | 1991年 / 9卷 / 02期
关键词：
D O I：
10.1017/S1323358000024310
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A new mechanism of thermonuclear reaction is briefly introduced. It shows that a certain amount of thermonuclear reaction can take place in dense, low temperature (T < 1 x 10(5) K) plasmas. As most regions in the Sun are at moderate and low temperature, a sufficient amount of fusion energy is generated there, Therefore, the current standard solar models, in which the solar central temperature must be slightly lower than 15 x 10(6) K, must be modified, and this would make the flux of high-energy neutrinos conform with the observational results.
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页码：313 / 314
页数：2
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