太阳核聚变概率计算及太阳目前结构和状态的推测  

The Sun Nuclear Fusion Pro b a b ility Calculations and Speculation of Its Current Structure and State

作　　者：李学潜[1] 张邦固[2] 

机构地区：[1]南开大学物理科学学院,天津300071 [2]科学出版社,北京100717

出　　处：《物理通报》2013年第11期102-106,共5页Physics Bulletin

摘　　要：根据观测资料,计算得到类太阳恒星条件下的质子-质子聚变概率、太阳氢核数随时间变化的函数.恒星主序期光度的主要贡献来自质子-质子聚变这个基础反应.给出了太阳目前比较细致的结构及状态,并且基本通过了检验.借鉴恒星实际,作者建议在地球上实验新的（较低温对撞）聚变装置.A probability of proton - proton fusion has been got under condition of star similar the sun. A function of numbers of hydrogen in the sun has been got. In main sequence period luminosity of star mainly comes from proton - proton fusion. A careful present structure of sun has been got. And it has been tested. A proposal about fusion unit has been raised.

关 键 词：量子力学隧道效应 聚变概率 质子-质子聚变 太阳常数 太阳氢核数-时间函数 

分 类 号：P182.1[天文地球—天文学]