Stability of the stellar structure in non-equilibrium thermodynamics

Details Stability of the stellar structure in non-equilibrium thermodynamics Stability of the stellar structure in non-equilibrium thermodynamics

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980acasn..21..172p&link_type=abstract

Acta Astronomica Sinica, vol. 21, June 1980, p. 172-179. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

3

Interstellar Gas, Nonequilibrium Thermodynamics, Stellar Structure, Systems Stability, Chemical Reactions, Entropy, Nonlinear Systems

Scientific paper

Using the criterion of excess entropy production about stability in
nonlinear and nonequilibrium thermodynamics, the stability of stellar
structure during PPI reaction in the stars of solar type is analyzed. It
is shown that the star must be stable if only Y less than 8.9, X = H(1),
Y = He(4). It is obviously satisfied for normal stars.

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