Dynamical Behavior of Nuclear Reaction Systems Disturbed by Fluid Motion in the Solar Core

Details Dynamical Behavior of Nuclear Reaction Systems Disturbed by Fluid Motion in the Solar Core Dynamical Behavior of Nuclear Reaction Systems Disturbed by Fluid Motion in the Solar Core

Nov 1993

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

Astrophysics and Space Science, Volume 209, Issue 2, pp.221-227

Astronomy and Astrophysics

Astrophysics

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 He3 has been analysed using developed nonequilibrium theory. We find that the system in the solar core is unstable in the layer extending from about 0.2R &sun; to 0.4R &sun; if the core is disturbed by fluid motion; this instability may be related to thermal diffusion.

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