Stability analysis of C-N-O nuclear reaction inside the stars

Details Stability analysis of C-N-O nuclear reaction inside the stars Stability analysis of C-N-O nuclear reaction inside the stars

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.158..153c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 158, no. 1, Aug. 1989, p. 153-157.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Models, Cosmochemistry, Nuclear Astrophysics, Nuclear Reactions, Stellar Physics, Chemical Reactions, Convection, Differential Equations, Diffusion Theory, Dynamic Stability

Scientific paper

In view of the fact that the nuclear reactions inside the stars are very
strong, the effects of convection and diffusion are introduced in the
fundamental equation of the problem in modeling to the C-N-O nuclear
reaction. The stability of the nuclear reaction inside the star is
investigated.

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