Stability of the complete cycle in hydrogen combustion inside the stars

Details Stability of the complete cycle in hydrogen combustion inside the stars Stability of the complete cycle in hydrogen combustion inside the stars

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.179..285l&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 179, no. 2, May 1991, p. 285-292.

Astronomy and Astrophysics

Astrophysics

Convection-Diffusion Equation, Hydrogen, Nonequilibrium Thermodynamics, Nuclear Fusion, Stellar Interiors, Differential Equations, Dirichlet Problem, Helium, Hertzsprung-Russell Diagram

Scientific paper

Generating-function and linear-stability-analysis methods based on Prigogine's nonequilibrium thermodynamic theory are used to investigate the stability of the complete cycle in hydrogen combustion inside stars. Consideration is given to the complete cycle of hydrogen combustion allowing for the effect of diffusion, as well as the complete cycle in hydrogen combustion with both convection and diffusion.

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