Stability of thermonuclear reaction affected by gravitational force

Details Stability of thermonuclear reaction affected by gravitational force Stability of thermonuclear reaction affected by gravitational force

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.195..349d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 195, no. 2, p. 349-357.

Astronomy and Astrophysics

Astrophysics

6

Gravitational Effects, Nonequilibrium Thermodynamics, Stellar Interiors, Stellar Structure, Thermonuclear Reactions, Stability, Stochastic Processes, Temperature Gradients

Scientific paper

The theory of nonequilibrium thermodynamics is used to obtain a reaction-diffusion equation describing a thermonuclear reaction system affected by gravitational force and temperature gradient. The CNO cycle is taken as an example to investigate the effects of the gravitational force and temperature gradient on the stability of nuclear reaction inside the star. The stability criterion of the stellar structure is analyzed, and some attractive results are discussed.

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