Density fluctuations in the nuclear reaction–diffusion system and the oscillations inside stars

Du Jiulin

Physica A: Statistical Mechanics and its Applications, 2003, vol. 318, issue 3, 334-340

Abstract: Fluctuations in stellar nuclear reaction–diffusion system affected by the g–T 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 is a series of fluctuation waves and the density oscillations in stellar cores, while the g–T effect is responsible for producing the oscillations. These oscillations inside stars may lead to time oscillating of stellar nuclear energy generation.

Keywords: Density fluctuation; Oscillation; Stellar nuclear reaction; Stellar interior (search for similar items in EconPapers)
Date: 2003
References: View complete reference list from CitEc
Citations:

Downloads: (external link)
http://www.sciencedirect.com/science/article/pii/S0378437102013626
Full text for ScienceDirect subscribers only. Journal offers the option of making the article available online on Science direct for a fee of $3,000

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:eee:phsmap:v:318:y:2003:i:3:p:334-340

DOI: 10.1016/S0378-4371(02)01362-6

Access Statistics for this article

Physica A: Statistical Mechanics and its Applications is currently edited by K. A. Dawson, J. O. Indekeu, H.E. Stanley and C. Tsallis

More articles in Physica A: Statistical Mechanics and its Applications from Elsevier
Bibliographic data for series maintained by Catherine Liu ().