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恒星核反应扩散系统中的涨落

杜九林

陕西师范大学学报(自然科学版)2003,Vol.31Issue(1):33-38,6.
陕西师范大学学报(自然科学版)2003,Vol.31Issue(1):33-38,6.

恒星核反应扩散系统中的涨落

Fluctuations in stellar nuclear reaction-diffusion system

杜九林1

作者信息

  • 1. 陕西师范大学物理与信息技术学院,陕西,西安,710062
  • 折叠

摘要

Abstract

Fluctuations in stellar nuclear reaction-diffusion system affected by the gravity-temperature gradient effect are investigated and the oscillations related to the fluctuations of particle number density in the proceedings of the core nuclear reactions of stars are analyzed. It is shown that there are a series of fluctuation waves propagating in space and oscillations of particle number density in stellar cores, while the gravity-temperature gradient effect is responsible for producing the oscillations. These oscillations inside stars may lead to time oscillating of stellar nuclear energy generating. The production of the 8B and 7Be neutrino fluxes might not only be suppressed due to the nonlinear density enhancement of 3He but also be changing with time due to the oscillations of 3He.

关键词

核反应/涨落/振荡

Key words

nuclear reaction-diffusion system/fluctuation/stellar oscillations

分类

天文与地球科学

引用本文复制引用

杜九林..恒星核反应扩散系统中的涨落[J].陕西师范大学学报(自然科学版),2003,31(1):33-38,6.

基金项目

国家自然科学基金资助项目(19503002 ()

19701021) ()

陕西师范大学重点科研基金资助项目 ()

陕西师范大学学报(自然科学版)

OA北大核心CSCDCSTPCD

1672-4291

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