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恒星内部核反应系统中g-T效应产生的振荡

Oscillations excited by g-T effect in the core nuclear reaction system of stars
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摘要 研究了恒星内部核反应系统中与粒子数密度涨落有关的振荡现象,分析了这类振荡的产生条件和特征频率。结果表明,引力及温度梯度(g-T)效应可以在氦核反应扩散模型中产生超临界的密度振荡。 Oscillations related to density fluctuation of particle number in the core nuclear reaction system of stars are investigated.It is shown that the supercritical density oscillations could be excited by gT effect in the model for helium nuclear reactiondiffusion system inside stars.The characteristic frequencies and producing criterion for the oscillations are analyzed.
出处 《西北大学学报(自然科学版)》 CAS CSCD 北大核心 2002年第6期622-624,共3页 Journal of Northwest University(Natural Science Edition)
基金 国家自然科学基金资助项目(19503002 19701021) 陕西师大重点科研基金项目
关键词 恒星 内部核反应系统 恒星振荡 g-T效应 温度梯度效应 特征频率 stellar cores stellar oscillations nuclear reactions g-T effect
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参考文献9

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