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对流、核反应和太阳内部振荡 被引量:1

Convection, nuclear reactions and interior oscillations
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摘要 给出恒星内部对流与核反应耦合的一个动力学模型.借助标准太阳模型,证明了在太阳中心的核反应中,3He的粒子数密度产生和消灭过程均呈振荡状态.在能量产生的峰值区域内,3He的振荡周期大约为5min,代表着总能量产生的振荡特征.太阳内部的这一特性预期可以说明观察到的中微子流的时间变化. A model on the coupling of convection with nuclear reactions inside stars is prestnted. With the aid of standard solar models it is shown that particle number density of 3 He oscillates in producing and destroying in the core nuclear reactons. It is found that 3 He oscillates with the time period of order of about 5 min in the region where the energy generation rises up to the maximun. This means the oscillation existing in the total energy production. These new characteristics in the sun may explaine the observed time variations in the solar neutrino fluxes.
作者 杜九林
出处 《陕西师大学报(自然科学版)》 CSCD 北大核心 1997年第4期25-28,共4页 Journal of Shaanxi Normal University(Natural Science Edition)
基金 国家自然科学基金 陕西省自然科学基金
关键词 太阳振荡 核反应 对流 太阳内部振荡 中微子 solar interior solar oscillations nuclear reactions convection
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同被引文献9

  • 1杜九林,张民仓,鲁百佐.PPI反应决定的恒星结构稳定性与引力─温度梯度效应[J].陕西师大学报(自然科学版),1995,23(1):29-33. 被引量:2
  • 2Du Jiulin, Chen Fusheng. Stability of Thermonuclear Reaction Affected by Gravitational Force[J ]. Astrophys Space Sci, 1992,195: 349 - 357.
  • 3Du Jiulin, Chen Fusheng. Stability of Stellar Structure and Nonequilibrium Dynamical Characteristics of g - T Effects in Nuclear Reactions in Stellar Cores[J]. Astrophys Space Sci, 1993, 207:37- 46.
  • 4Du Jiulin. Dynamical Behavior of Nuclear Reaction System Disturbed by Fluid Motion in the Core[J]. Astrophys Space Sci,1993, 209:221 - 227.
  • 5Nicolis G and Prigogire I. Selforganization in Nonequilibrium System[ M ]. Jone Wiley and Sons. 1977.
  • 6Lang K R.Astrophysical Formulae[ M] . Springer - Verlay, Berlin, 1974.
  • 7Aller C W. Astrophysical Quantities(Third Edition)[M]. The Athlon Press, 1973.
  • 8Maryan Harwit. Astrophysical Concepts[ M]. John Wiley, 1973.
  • 9杜九林,史志强,陈福生.非平衡动力学中恒星结构稳定性研究[J].天体物理学报,1991,11(2):143-148. 被引量:2

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