Dynamical behavior of nuclear reaction systems disturbed by fluid motion in the solar sore

Details Dynamical behavior of nuclear reaction systems disturbed by fluid motion in the solar sore Dynamical behavior of nuclear reaction systems disturbed by fluid motion in the solar sore

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.209..221j&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 209, no. 2, p. 221-227

Astronomy and Astrophysics

Astrophysics

Dynamic Stability, Euler Equations Of Motion, Hydrostatics, Solar Interior, Stellar Cores, Thermodynamic Equilibrium, Pressure Effects, Proton-Proton Reactions, Stellar Models, Thermal Diffusion

Scientific paper

Using Euler's equation of motion, the equation for disturbed fluid motion against a hydrostatic equilibrium has been derived, and the nonequilibrium dynamical equation of a P-PI nuclear reaction system driven by He-3 has been analyzed using developed nonequilibrium theory. We find that the system in the solar core is unstable in the layer extending from about 0.2 solar radius to 0.4 solar radius if the core is disturbed by fluid motion; this instability may be related to thermal diffusion.

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